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  <front>
    <journal-meta><journal-id journal-id-type="publisher">JM</journal-id><journal-title-group>
    <journal-title>Journal of Micropalaeontology</journal-title>
    <abbrev-journal-title abbrev-type="publisher">JM</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">J. Micropalaeontol.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">2041-4978</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/jm-38-1-2019</article-id><title-group><article-title>Record of Early to Middle Eocene paleoenvironmental changes from lignite
mines, western India</article-title><alt-title>Record of Early to Middle Eocene paleoenvironmental changes</alt-title>
      </title-group><?xmltex \runningtitle{Record of Early to Middle Eocene paleoenvironmental changes}?><?xmltex \runningauthor{S. Khanolkar and J. Sharma}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Khanolkar</surname><given-names>Sonal</given-names></name>
          <email>sonal.k.12@gmail.com</email>
        <ext-link>https://orcid.org/0000-0002-7911-1699</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Sharma</surname><given-names>Jyoti</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Department of Earth Sciences, Indian Institute of Technology Kanpur,
Kanpur, India</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Department of Geology, K. J. Somaiya College of Science and
Commerce,<?xmltex \hack{\break}?>
University of Mumbai, Mumbai, India</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Sonal Khanolkar (sonal.k.12@gmail.com)</corresp></author-notes><pub-date><day>18</day><month>January</month><year>2019</year></pub-date>
      
      <volume>38</volume>
      <issue>1</issue>
      <fpage>1</fpage><lpage>24</lpage>
      <history>
        <date date-type="received"><day>21</day><month>May</month><year>2018</year></date>
           <date date-type="rev-recd"><day>21</day><month>November</month><year>2018</year></date>
           <date date-type="accepted"><day>3</day><month>December</month><year>2018</year></date>
      </history>
      <permissions>
        
        
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://jm.copernicus.org/articles/.html">This article is available from https://jm.copernicus.org/articles/.html</self-uri><self-uri xlink:href="https://jm.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://jm.copernicus.org/articles/.pdf</self-uri>
      <abstract>
    <p id="d1e94">Various Eocene hyperthermal events have been recorded from lignite sections
of western India in the past decade. To infer the paleoenvironment, during a
warm paleotropical climate of India, we have assessed multiple microfossil
groups like pollen/spores, dinoflagellates and foraminifera from Early Eocene
lignite mine sections from the Cambay (Surkha) and Barmer (Giral) basins and
Middle Eocene sections from the Kutch Basin (Matanomadh and Panandhro mines)  of
western India. The Surkha and Giral sections exhibit a dominance of
rainforest elements (<italic>Arengapollenites achinatus, Longapertites retipilatus</italic>), thermophilic mangrove palm <italic>Nypa</italic> and (sub)tropical
dinoflagellate cyst <italic>Apectodinium, Cordosphaeridium</italic> and
<italic>Kenleyia</italic>. This palynomorph assemblage is indicative of a marginal
marine setting within a hot and humid climate. During the Middle Eocene, the
diversity of dinocyst assemblage increased and a decrease in percentage of
mangrove elements was observed in the  Matanomadh and Panandhro mine sections of
the Kutch Basin as compared to the Early Eocene sections of western India.
Bloom of triserial planktic (<italic>Jenkinsina columbiana</italic>) and rectilinear
benthic  (<italic>Brizalina</italic> sp., <italic>Trifarina advena rajasthanensis</italic>) foraminifera indicates eutrophic conditions of deposition during the Late
Lutetian–Early Bartonian in the lignite sections of the Kutch Basin which later changed
to oligotrophic, open marine conditions towards the Bartonian (planktic E12
zone). This change to oligotrophic conditions coincides with a drastic
increase in diversity of planktic foraminifera in the top portion of lignite
mines of the Kutch Basin which may be correlated with the Kirthar–Wilson Bluff
transgression event in the Bartonian observed across  basins in India, Pakistan and
Australia potentially linked to sea level rise around the Middle
Eocene Climatic Optimum.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><caption><p id="d1e123">Paleoposition of the Cambay, Kutch and Barmer basins in India during the
<bold>(a)</bold> Early Eocene and <bold>(b)</bold> Middle Eocene.</p></caption>
      <?xmltex \igopts{width=355.659449pt}?><graphic xlink:href="https://jm.copernicus.org/articles/38/1/2019/jm-38-1-2019-f01.jpg"/>

    </fig>

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
<sec id="Ch1.S1.SS1">
  <title>General introduction</title>
      <p id="d1e148">The Early and Middle Eocene exhibited a very warm climate, but towards the
Late Eocene, the atmosphere cooled and shifted from hothouse to icehouse
conditions (Zachos et al., 2001). The tropical temperatures during the
Early Eocene increased by 5 to 6 <inline-formula><mml:math id="M1" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, and there was little or no ice cover
observed at the poles during these warming events (Pearson et al., 2001).
There has been a plethora of records studied from the high latitudes with
respect to microfossils and their change in size, diversity and abundance to
adapt to the Paleogene warming events, especially the deep-sea drilling
projects which have provided insight into continuous stratigraphic records
(Clay Kelly et al., 1996; Kelly et al., 1998; Thomas and Shackleton, 1996;
Arenillas et al., 1999; Giusberti et al., 2009; Alegret et al., 2010; Stassen
et al., 2012; Zachos et al., 2001). The low-latitude records of the Paleogene
which are stratigraphically continuous are comparatively sparse (Jaramillo et
al., 2006, 2010; Zamagni et al., 2012; Pearson et al., 2001; Khanolkar and
Saraswati, 2015; Cramwinckel et al., 2018; Naafs et al., 2018). Some of the
low-latitude Eocene sections from Tanzania, India and Java have recently
provided insight into temperatures in the tropics during the Eocene epoch (Evans
et al., 2018). However, there is a need to produce robust records from
well-preserved<?pagebreak page2?> paleotropical Eocene sections to assess the response of flora and
fauna to the greenhouse conditions which prevailed.</p>
      <p id="d1e160">The Indian subcontinent (Fig. 1) has well-preserved records of Paleogene
marine and continental sediments deposited along its western sedimentary
basins ranging from the Eocene (shallow benthic zone: SBZ 5/6–SBZ 11 and SBZ
17; age: 56–49 Myr) to the Oligocene (SBZ 22b–SBZ 23;
age: 28.1–23 Myr) (Saraswati et al., 2018). The humid hothouse during the
Early Paleogene enhanced the development of tropical rainforests and gave
rise to extensive development of lignite deposits in the Indian subcontinent.
The sea level highstands which co-occur with these high temperatures, such as
that in western India (Samanta et al., 2013; Prasad et al., 2013), probably
facilitated the development and preservation of the lignite deposits (Sluijs
et al., 2008). These lignite deposits were formed in the restricted marine
basins and are coeval with the warming events in the Paleogene. The Early
Eocene lignite deposits were developed in the Cambay and Barmer basins, while
the Middle Eocene lignite deposits are observed in the Kutch and Barmer
basins. These lignite mine sections have recorded some of the warming events
like Paleocene Eocene Thermal Maximum (PETM), Eocene Thermal Maximum 2
(ETM 2), Early Eocene Climatic Optimum (EECO) from the Cambay Basin and
Middle Eocene Climatic Optimum (MECO) from the Kutch Basin (Samanta et al.,
2013; Khanolkar et al., 2017; Clementz et al., 2011). The earlier works on
these lignite mines emphasized the determination of paleoenvironmental
conditions focusing on one microfossil group like pollen and spores or
dinocysts or foraminifera (Sharma and Saraswati, 2015; Garg et al., 2008;
Khanolkar et al., 2017). A lacuna exists in using an integrated approach to
decipher the paleodepositional and paleoenvironmental conditions across the
Early and Middle Eocene sections from paleotropical sites in India.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><caption><p id="d1e165">Eocene Stratigraphy of the Barmer, Cambay and Kutch basins in India.</p></caption>
          <?xmltex \igopts{width=384.112205pt}?><graphic xlink:href="https://jm.copernicus.org/articles/38/1/2019/jm-38-1-2019-f02.png"/>

        </fig>

      <?pagebreak page3?><p id="d1e174">In this work, we have addressed the similarities and differences observed in
the paleodepositional and paleovegetational conditions from the Cambay, Kutch and
Barmer basins during the tropical climate of the Early and Middle Eocene. For
this, we have used an integrated approach by quantitatively analyzing various
microfossil groups like foraminifera, pollen and spores, dinoflagellates and
fungi. A holistic approach has made it possible to better determine the
paleoenvironmental conditions from a restricted marine setting which depicts
transitional environments and is comprised of various groups of microfossils
belonging to both continental and open marine ecosystems. For our present
study, we have chosen four lignite mine sections: (1) Surkha lignite mine
section (Cambay Basin), (2) Giral lignite mine section (Barmer Basin),
(3) Matanomadh (Kutch Basin) and (4) Panandhro lignite mine section (Kutch
Basin).</p>
</sec>
<sec id="Ch1.S1.SS2">
  <title>Eocene lignites from western Indian basins</title>
      <p id="d1e183">The mineable lignite deposits of Eocene age are found along the three
sedimentary basins of western India viz. Barmer, Kutch and Cambay. Various
well-preserved vertebrate fossils belonging to perissodactyls, artiodactyls,
insectivores, proteutherians, apatotherians, marsupials, rodents and
microfossils like dinoflagellates, pollen and spores, and foraminifera have been
discovered from these lignite mine sections, rendering them essential from a
stratigraphic point of view (Bajpai et al., 2005; Khanolkar and Saraswati,
2015; Garg et al., 2008).</p>
<sec id="Ch1.S1.SS2.SSS1">
  <title>Rajasthan Basin</title>
      <p id="d1e191">The Rajasthan Basin consists of a geological record from Archean to recent times.
Within the Rajasthan Basin, three sub-basins, namely the Barmer, Jaisalmer and
Bikaner–Nagaur (K. Kumar et al., 2007), exist and cover an area of
approximately 120 000 km<inline-formula><mml:math id="M2" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>. The Barmer Basin is comprised of sediments
from Precambrian to Middle Miocene age. The Jagmal Group, which is of Eocene
age, lies unconformably over the Mallinath Group of Late Cretaceous–Late
Paleocene age. The Jagmal Group is comprised of shales, lignites and sandstones.
The Giral lignite mine belongs to the Dharvi Dungar Formation within the
Jagmal Group and is of Early Eocene age (Fig. 2). The subsurface stratigraphy
has established that there is a second and younger level of lignite (Akli
Formation) of Middle Eocene age in the basin that is seismically well
separated (Dolson et al., 2015).</p>
</sec>
<sec id="Ch1.S1.SS2.SSS2">
  <title>Cambay Basin</title>
      <p id="d1e209">The Cambay Basin is comprised of Paleogene sediments overlain by Quaternary
alluvium. The Paleogene sequence rests unconformably over the Deccan flood
basalts, ranges in age from Paleocene to Plio-Pleistocene and has been
deposited by various transgressive–regressive cycles. The oldest Paleogene
rocks are comprised of the Olpad Formation, which is unconformably overlain by the Cambay
Formation (Paleocene–Early Eocene) (Fig. 2) (Chandra and Chowdhary, 1969).
The Cambay Formation is best exposed along the open-cast lignite mines and
has yielded rich and diverse fauna of various fossil groups. The lignite
mine sections of Vastan and Valia have reported the presence of hyperthermal
events including PETM and EECO (Samanta et al., 2013; Clementz et al., 2011).
The Surkha lignite mine section is examined in this study.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><caption><p id="d1e214">Percentage distribution of palynomorphs in the Giral lignite mine
section, Barmer Basin.</p></caption>
            <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://jm.copernicus.org/articles/38/1/2019/jm-38-1-2019-f03.jpg"/>

          </fig>

</sec>
<sec id="Ch1.S1.SS2.SSS3">
  <title>Kutch Basin</title>
      <p id="d1e229">The Kutch Basin is a pericratonic rift basin trending laterally beside the
western margin of India and developed during the separation of India from
Gondwanaland in the Late Triassic (Biswas, 1992). A complete stratigraphic
succession from Paleogene to Quaternary, with records of marine transgression
and several stratigraphic breaks, was recorded in the basin (Biswas, 1992). A
significant part of the Tertiary sequence is observed in the offshore region
of the Kutch<?pagebreak page4?> Basin, whereas on land, these Tertiary sections are restricted
to the western part. The Eocene sections mainly constitute shales, claystones
and limestones deposited in lagoonal to shallow marine environments. These
Eocene sediments have preserved large groups of faunal assemblages including
foraminifera, dinocysts, pollen and spores (Khanolkar and Saraswati, 2015;
Sharma and Saraswati, 2015; Garg et al., 2008). The Paleogene succession of
the Kutch is comprised of five formations. These include Matanomadh
Formation, Naredi Formation, Harudi Formation, Fulra limestone and Maniyara
Fort Formation) (Fig. 2) (Biswas, 1992; Saraswati et al., 2018).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><caption><p id="d1e234">Percentage distribution of palynomorphs in the Surkha lignite mine
section, Cambay Basin.</p></caption>
            <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://jm.copernicus.org/articles/38/1/2019/jm-38-1-2019-f04.jpg"/>

          </fig>

</sec>
</sec>
<sec id="Ch1.S1.SS3">
  <title>Previous stratigraphic works</title>
      <p id="d1e250">The Cambay, Kutch and Rajasthan basins have been previously investigated by
various workers to decipher the age of the mine sections.</p>
<sec id="Ch1.S1.SS3.SSS1">
  <title>Rajasthan Basin</title>
      <p id="d1e258">Dolson et al. (2015) updated the stratigraphy of the Barmer Basin in
Rajasthan using the data acquired from 420 wells, 4 km of conventional core
and 2-D and 3-D seismic mapping techniques. The age of the lignite mine section
of the Giral was earlier thought to be of Late Paleocene–Early Eocene (Rana et
al., 2005). However, the recent work by Dolson et al. (2015) has updated it
to be of Early Eocene age.</p>
</sec>
<sec id="Ch1.S1.SS3.SSS2">
  <title>Cambay Basin</title>
      <p id="d1e267">The Early Eocene (Ypresian) palynomorph taxa from the Surkha mine consist of
<italic>Polysphaeridium subtile, Homotryblium pallidum, Retipollenites confusus, Arengapollenites achinatus</italic> and <italic>Tribrevicolporites eocenicus</italic> reported from lignite mine sections of Rajpardi and Vastan from
the Cambay Basin (Kumar, 1994; Samant and Phadtare, 1997; Mandal and Guleria,
2006; Tripathi and Srivastava, 2012; Rao et al., 2013). This evidence further
corroborates the existence of coeval deposition and analogous
paleoenvironment. The age of the Vastan mine section is inferred to be
Early Eocene, given the presence of <italic>Nummulites burdigalensis burdigalensis</italic>
(Punekar and Saraswati, 2010).</p>
</sec>
<sec id="Ch1.S1.SS3.SSS3">
  <title>Kutch Basin</title>
      <p id="d1e285">The age of lignites from the Kutch Basin was earlier thought to be Early Eocene
(Biswas, 1992). However, recent work has revised the stratigraphy of the Kutch Basin,
and the current understanding states that the lignites belong to Middle Eocene age (Saraswati et al., 2018, 2014). In a marginal
marine environment, it is essential to infer the age of the<?pagebreak page5?> sequence using an
integrated approach which involves the study of various group of microfossils
like palynomorphs and foraminifera (Sharma and Saraswati, 2015). The shales
deposited above the lignite seams of the Panandhro and Matanomadh mines consists
of foraminifera such as <italic>Nummulites spectabilis, Linderina kutchensis</italic> and
<italic>Halkyardia minima</italic>, which are typically found in the Middle Eocene in
other sections of the Kutch Basin and correspond to Bartonian age (SBZ 17). There
is no break in sedimentation or unconformity observed between the lignites
and the overlying shales of Bartonian age. It can thus be stated that the
lignites are of Bartonian age or could have ranged down to latest Lutetian.</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S2">
  <title>Materials and methods</title>
<sec id="Ch1.S2.SS1">
  <title>Materials</title>
      <p id="d1e307">The field area is comprised of lignite mine sections from three different
sedimentary basins (Cambay, Kutch and Rajasthan) alongside the western margin
of India (Fig. 1; Sect. S1 in the Supplement).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><caption><p id="d1e312">Percentage distribution of palynomorphs in the Matanomadh lignite mine
section, Kutch Basin.</p></caption>
          <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://jm.copernicus.org/articles/38/1/2019/jm-38-1-2019-f05.jpg"/>

        </fig>

<sec id="Ch1.S2.SS1.SSS1">
  <title>Rajasthan Basin</title>
      <p id="d1e326">For the current study, we collected 33 samples from 26 m exposure
of the open-cast lignite mine of the Giral from the Barmer sub-basin. The profile
constitutes alternations of shale and lignite beds. The sample positions are
marked in the lithocolumn illustrated in Fig. 3 (refer to Sect. S1 in the Supplement).</p><?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S2.SS1.SSS2">
  <title>Cambay Basin</title>
      <p id="d1e336">The Surkha lignite mine section is equivalent to the subsurface Cambay Shale
Formation and belongs to Early Eocene. We have collected eight samples from
the bottom to top of the mine section, and their positions are marked within the
lithocolumn (Fig. 4; Sect. S1 in the Supplement). The mine section is comprised mainly of
lignites and shales. Around 5 m thick brown colored friable lignite horizon
is overlain by marine shale, which gradually grades into silty shale at the
top. The whole lignite-bearing sequence is covered by 20 m thick bentonite clay.</p>

      <?xmltex \floatpos{p}?><?pagebreak page7?><fig id="Ch1.F6" specific-use="star"><caption><p id="d1e341">The palynomorph
assemblage from Early Eocene sections: panels <bold>(1)</bold> and
<bold>(2)</bold> are <italic>Longapertites retipilatus</italic>. Panels <bold>(3)</bold>,
<bold>(4)</bold> and <bold>(5)</bold> are <italic>Spinizonocolpites prominatus</italic>.
Panels <bold>(6)</bold> and <bold>(7)</bold> are <italic>Spinizonocolpites bulbospinosus</italic>. <bold>(8)</bold> <italic>Proxapertites microreticulatus</italic>.
<bold>(9)</bold> <italic>Longapertites retipilatus</italic>.
<bold>(10)</bold> <italic>Acanthotricolpites bulbospinosus</italic>.
<bold>(11)</bold> <italic>Kapurdipollenites gemmatus</italic>.
<bold>(12)</bold> <italic>Spinizonocolpites baculatus</italic>.
<bold>(13)</bold> <italic>Spinizonocolpites brevispinosus</italic>.
<bold>(14)</bold> <italic>Apectodinium quinquelatum</italic>.
<bold>(15)</bold> <italic>Apectodinium paniculatum</italic>.
<bold>(16)</bold> <italic>Apectodinium paniculatum</italic>.
<bold>(17)</bold> <italic>Arengapollenites achinatus</italic>.
<bold>(18)</bold> <italic>Acanthotricolpites kutchensis</italic>.
Panels <bold>(19)</bold> and <bold>(20)</bold> are fungal elements.</p></caption>
            <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://jm.copernicus.org/articles/38/1/2019/jm-38-1-2019-p01.jpg"/>
            <?xmltex \hack{\def\figurename{Plate}\setcounter{figure}{0}}?>

          </fig>

      <?xmltex \floatpos{p}?><?pagebreak page8?><fig id="Ch1.F7" specific-use="star"><caption><p id="d1e461">The palynomorph
assemblage from Middle Eocene lignite mine sections of the Panandhro and
Matanomadh: panel <bold>(1)</bold> is <italic>Achomosphaera</italic> sp. Panels <bold>(2)</bold> and
<bold>(3)</bold> are <italic>Cordosphaeridium exilimurum</italic>. Panels <bold>(4)</bold>, <bold>(5)</bold>
and <bold>(6)</bold> are <italic>Homotryblium floripes</italic>.
<bold>(6)</bold> <italic>Glaphyrocysta exuberans</italic>.
<bold>(7)</bold> <italic>Cordosphaeridium cantharellus</italic>.
<bold>(8)</bold> <italic>Glaphyrocysta exuberans</italic>.
<bold>(9)</bold> <italic>Spiniferites ramosus</italic>.
<bold>(10)</bold> <italic>Kenleyia</italic> sp.
Panels <bold>(11)</bold> and <bold>(12)</bold> are <italic>Operculodinium centrocarpum</italic>.
<bold>(13)</bold> <italic>Thalassiphora pelagica</italic>.
<bold>(14)</bold> <italic>Polysphaeridium subtile</italic>.
<bold>(15)</bold> <italic>Thalassiphora fenestrata</italic>.
<bold>(16)</bold> <italic>Thalassiphora pelagica</italic>.
<bold>(17)</bold> <italic>Dipterocarpuspollenites retipilatus</italic>. Panels <bold>(18)</bold> and
<bold>(19)</bold> are <italic>Albertipollenites crassireticulatus</italic>.
<bold>(20)</bold> <italic>Tricolpites</italic> sp.</p></caption>
            <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://jm.copernicus.org/articles/38/1/2019/jm-38-1-2019-p02.jpg"/>
            <?xmltex \hack{\def\figurename{Plate}\setcounter{figure}{1}}?>

          </fig>

</sec>
<sec id="Ch1.S2.SS1.SSS3">
  <title>Kutch Basin</title>
      <p id="d1e596">From the Kutch Basin, we have collected samples from the Matanomadh mine section
(23 samples from 10 m exposure of lignites, shales and
mudstones; Fig. 5; Sect. S1 in the Supplement) and Panandhro lignite mine (47
samples from 55 m exposure of lignite and shale sections;
Fig. 6; Sect. S1 in the Supplement).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><caption><p id="d1e601">The
foraminiferal assemblage from the Panandhro and Matanomadh lignite mines.
<bold>(1)</bold> <italic>Jenkinsina columbiana</italic>.
<bold>(2)</bold> <italic>Streptochilus martini</italic>.
<bold>(3)</bold> <italic>Orbulinoides beckmanni</italic>.
<bold>(4)</bold> <italic>Acarinina topilensis</italic>.
<bold>(5)</bold> <italic>Nummulites obtusus</italic>.
<bold>(6)</bold> <italic>Linderina kutchiensis</italic>.
<bold>(7)</bold> <italic>Halkyardia minima</italic>.
<bold>(8)</bold> <italic>Textularia halkyardia</italic>.
<bold>(9)</bold> <italic>Miliammina</italic> sp.
<bold>(10)</bold> <italic>Trifarina advena rajasthanensis</italic>.
<bold>(11)</bold> <italic>Brizalina</italic> sp.
<bold>(12)</bold> <italic>Reusella</italic> sp.
<bold>(13)</bold> <italic>Triloculina architectura</italic>.
<bold>(14)</bold> <italic>Robulus</italic> sp.
<bold>(15)</bold> <italic>Cibicides punjabensis</italic>.
<bold>(16)</bold> <italic>Cibicides</italic> sp.
<bold>(17)</bold> <italic>Florilus</italic> sp.
<bold>(18)</bold> <italic>Pijpersia coronaeformis</italic>.
<bold>(19)</bold> <italic>Eponides</italic> sp.
<bold>(20)</bold> <italic>Glabratella ubiqua</italic>.</p></caption>
            <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://jm.copernicus.org/articles/38/1/2019/jm-38-1-2019-p03.jpg"/>
            <?xmltex \hack{\def\figurename{Plate}\setcounter{figure}{2}}?>

          </fig>

<?xmltex \hack{\setcounter{figure}{5}}?><?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><caption><p id="d1e741">Percentage distribution of palynomorphs in the Panandhro lignite mine
section, Kutch Basin.</p></caption>
            <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://jm.copernicus.org/articles/38/1/2019/jm-38-1-2019-f06.jpg"/>

          </fig>

</sec>
</sec>
<sec id="Ch1.S2.SS2">
  <title>Methodology</title>
<sec id="Ch1.S2.SS2.SSS1">
  <title>Palynomorphs separation and slide preparation</title>
      <p id="d1e762">For palynomorph analysis, we processed samples from all four mine sections.
Initially, we treated 20 g of the dry sample with dilute HCl (30 %) for
removal of carbonates. The residue left was consecutively treated with
hydrofluoric (HF) acid (38 %) for removal of silica and <inline-formula><mml:math id="M3" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">HNO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> for removal of
sulfides and sulfates. Deionized water was utilized to neutralize the samples
which were wet sieved (10–250 <inline-formula><mml:math id="M4" display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m sieve<?pagebreak page6?> size). We used Safranin O
to stain the residue. Polyvinyl alcohol and Canada balsam were used for the
preparation and mounting of the slides. From each sample which contained of
palynomorphs, we have counted at least 200 palynomorphs, which we considered
as the total count. Figures 3–6 exhibit plots of percentage variation of
palynomorphs (refer to Sect. S2 in the Supplement). We have also grouped
various categories of palynomorphs and their distributions in Figs. 7–10.
The palynomorph distribution diagrams have been further divided into zones by
stratigraphically constrained cluster analysis using CONISS (Grimm, 2004)
available in Tilia TG View 2.0.2 software (Grimm, 2004) in conjugation with
the changes in the percentage of some important taxa. Plates 1–2 illustrate
the representative palynomorph taxa. The ecological preferences for
palynomorph taxa are given in Sect. S3 in the Supplement.</p>
</sec>
<sec id="Ch1.S2.SS2.SSS2">
  <title>Foraminiferal analysis</title>
      <p id="d1e789">We have used around 20 g of sample (shales and mudstones) for processing.
The sample was treated with <inline-formula><mml:math id="M5" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> initially for removal of any
organic material. The residue left was then mixed with water and heated after
adding <inline-formula><mml:math id="M6" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">Na</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> to it for half an hour, following which the
residue was washed over a <inline-formula><mml:math id="M7" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">63</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M8" display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m sieve. The washed residue was dried
at 60 <inline-formula><mml:math id="M9" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C temperature in an oven. From each representative sample
obtained by using a microsplitter, a minimum of 300 foraminifera were picked
and represented as the “total foraminifera number”. We have used the
TILIA 2.0.2 software by Grimm (2004) to plot the percentage distribution data of each
species. The foraminifera percentage distribution data for the sections are
provided in Fig. 11. The identification of foraminifera was carried out by
following the works of Murray and Wright (1974), Singh and Kalia (1970),
Kalia (1978), Loeblich Jr. and Tappan (2015) and Pearson et al. (2005). The
paleoenvironment and paleodepositional analysis has been carried out by using
foraminiferal morphogroups (Nagy, 1992; Preece et al., 1999; Nigam et al.,
2007; Reolid et al., 2008; Singh et al., 2015). Using their technique to
record the foraminiferal morphogroups, we have divided the smaller benthic
foraminifera further into the rectilinear benthic foraminifer (RBF)
morphogroup, consisting of foraminifera with uniserial, biserial or triserial chamber
arrangements, and its percentage is used to indicate benthic oxygenation
conditions. The illustration of significant foraminifera taxa is shown in
Plate 3.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10" specific-use="star"><caption><p id="d1e852">Distribution of a group of palynomorph taxa in the Giral lignite mine,
Barmer Basin.</p></caption>
            <?xmltex \igopts{width=327.206693pt}?><graphic xlink:href="https://jm.copernicus.org/articles/38/1/2019/jm-38-1-2019-f07.jpg"/>

          </fig>

</sec>
</sec>
</sec>
<sec id="Ch1.S3">
  <title>Results</title>
<sec id="Ch1.S3.SS1">
  <title>Biostratigraphy of the study areas</title>
      <p id="d1e874">The age of lignite mines of the Surkha (Cambay), Panandhro and Matanomadh
(Kutch) has already been established earlier. However, the age of the Giral
mine section of the Barmer Basin was determined in this study using
palynomorphs.</p>
      <?pagebreak page9?><p id="d1e877">For the Rajasthan Basin, the palynological analysis of the Giral mine section (Barmer
Basin) indicates an Early Eocene age. Dinocysts are present in a few shale
layers within the Giral lignite section. The dinocyst assemblage is comprised of
<italic>Apectodinium homomorphum, Adnatosphaeridium</italic> sp.,
<italic>Glaphyrocysta exuberans, Kenleyia</italic> sp. and <italic>Thalassiphora pelagica</italic>. Although most of the genera recovered in the analysis are
long-ranging, the presence of rich and diverse <italic>Apectodinium</italic>
assemblages all along the profile suggests that the lignites were deposited
during the Ypresian (Garg et al., 2008; Crouch et al., 2003). This matches with
the age given by Dolson et al. (2015) of the Giral lignite mine section and is
thus reconfirmed to be the Early Eocene.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11"><caption><p id="d1e894">Distribution of a group of palynomorph taxa in the Surkha lignite mine,
Cambay Basin.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://jm.copernicus.org/articles/38/1/2019/jm-38-1-2019-f08.jpg"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12" specific-use="star"><caption><p id="d1e906">Distribution of a group of palynomorph taxa in the Matanomadh lignite
mine, Kutch Basin.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://jm.copernicus.org/articles/38/1/2019/jm-38-1-2019-f09.jpg"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS2">
  <title>Stratigraphic variation in percentage of palynomorphs in individual
mine sections</title>
<sec id="Ch1.S3.SS2.SSS1">
  <title>Giral mine</title>
      <p id="d1e926">Overall, 33 samples from the Giral lignite mine were processed and studied for
the palynomorph assemblage (Fig. 3). The mine section is rich in both
terrestrial and marine flora. Some of the palynoflora recovered are
<italic>Spinizonocolpites baculatus, Dandotiaspora telonata, Palmaepollenites plicatus, Longapertites retipilatus</italic> and <italic>Acanthotricolpites</italic>. Based on the
distribution and abundance of palynomorphs, the<?pagebreak page10?> studied succession of the Giral
lignite mine has been divided into three cenozones.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F13" specific-use="star"><caption><p id="d1e937">Distribution of a group of palynomorph taxa in the Panandhro lignite mine,
Kutch Basin.</p></caption>
            <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://jm.copernicus.org/articles/38/1/2019/jm-38-1-2019-f10.png"/>

          </fig>

      <p id="d1e946">In the stratigraphic order, they are
<list list-type="custom"><list-item><label> </label>
      <p id="d1e951"><italic>Spinizonocolpites </italic>spp. cenozone.</p></list-item></list></p>
</sec>
<sec id="Ch1.S3.SS2.SSSx1" specific-use="unnumbered">
  <title>Lithology</title>
      <p id="d1e962">The lowermost lignite and intervening shale units. Thickness is about 7 m.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx2" specific-use="unnumbered">
  <title>Position</title>
      <p id="d1e971">From sample no. RG-12/1 to RG-12/10.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx3" specific-use="unnumbered">
  <title>Important taxa</title>
      <p id="d1e980">In relation to the overlying assemblage, the litho-unit of this cenozone is
poor in pollen yield. All the samples were studied but only sample number
RG-12/1 yielded enough palynomorphs for quantification.
<italic>Spinizonocolpites</italic> and <italic>Proxapertites</italic> mark their appearance
in this cenozone; however, these taxa could not be quantified due to their
low abundance. The cenozone is named after the presence of
<italic>Spinizonocolpites </italic>pollen grain which was represented throughout the
cenozone. The other essential taxa recovered are <italic>Spinizonocolpites baculatus, S. bulbospinosus, Proxapertites microreticulatus, P. crassimurus, Acanthotricolpites brevispinosus</italic>, <italic>Arengapollenites achinatus, Longapertites retipilatus</italic>, etc.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx4" specific-use="unnumbered">
  <title>Lower limit</title>
      <p id="d1e1005">The lower limit is not traceable.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx5" specific-use="unnumbered">
  <title>Upper limit</title>
      <p id="d1e1014">The upper contact is the overlying 70 cm thick shale bed.</p>
      <p id="d1e1017"><list list-type="custom">
              <list-item><label> </label>

      <p id="d1e1022"><italic>Apectodinium homomorphum </italic>cenozone</p>
              </list-item>
            </list></p>
</sec>
<sec id="Ch1.S3.SS2.SSSx6" specific-use="unnumbered">
  <title>Lithology</title>
      <p id="d1e1035">Lignite- and marine-fossil-bearing shale unit. Thickness is about 8 m.</p>
</sec>
<?pagebreak page11?><sec id="Ch1.S3.SS2.SSSx7" specific-use="unnumbered">
  <title>Position</title>
      <p id="d1e1044">From sample no. RG-12/11 to RG-12/22.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F14" specific-use="star"><caption><p id="d1e1049">Percentage distribution, diversity indices and RBF morphogroup of
foraminifera in samples from the <bold>(a)</bold> Panandhro lignite mine and
<bold>(b)</bold> Matanomadh lignite mine section in the Kutch Basin of western
India.</p></caption>
            <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://jm.copernicus.org/articles/38/1/2019/jm-38-1-2019-f11.png"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS2.SSSx8" specific-use="unnumbered">
  <title>Important taxa</title>
      <p id="d1e1070">This cenozone is comprised of marine and terrestrial palynomorphs. The
cenozone is named after the first occurrence of stratigraphically important
dinocyst <italic>Apectodinium homomorphum</italic>. The characteristic feature of
this cenozone is the high percentage of <italic>Spinizonocolpites echinatus, S. baculatus, S. bulbospinosus, Proxapertites microreticulatus, P. crassimurus, Acanthotricolpites brevispinosus</italic> and <italic>A. bulbospinosus</italic>.
The other essential taxa recovered are <italic>Arengapollenites achinatus, Longapertites retipilatus, Dandotiaspora telonata, Lygodiumsporites</italic> sp.,
<italic>Todisorites major</italic>. <italic>Kapurdipollenites gemmatus</italic> made its
first appearance along with dinocysts (<italic>Apectodinium paniculatum, Kenleyia</italic> spp<italic>., Thalassiphora pelagica</italic> and <italic>Glaphyrocysta exuberans, Adnatosphaeridium</italic> sp.) in this zone.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx9" specific-use="unnumbered">
  <title>Lower limit</title>
      <p id="d1e1107">First appearance of <italic>Kapurdipollenites</italic> and <italic>Apectodinium homomorphum</italic>.</p><?xmltex \hack{\newpage}?>
</sec>
<?pagebreak page12?><sec id="Ch1.S3.SS2.SSSx10" specific-use="unnumbered">
  <title>Upper limit</title>
      <p id="d1e1124">Significant increase in the percentage of <italic>Acanthotricolpites </italic>spp.</p>
      <p id="d1e1130"><list list-type="custom">
              <list-item><label> </label>

      <p id="d1e1135"><italic>Acanthotricolpites </italic>spp. cenozone</p>
              </list-item>
            </list></p>
</sec>
<sec id="Ch1.S3.SS2.SSSx11" specific-use="unnumbered">
  <title>Lithology</title>
      <p id="d1e1148">Alternate lignite and shale beds. Thickness is about 10 m.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx12" specific-use="unnumbered">
  <title>Position</title>
      <p id="d1e1157">From sample no. RG-12/22 to RG-12/33.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx13" specific-use="unnumbered">
  <title>Important taxa</title>
      <p id="d1e1166">This cenozone is comprised of a high percentage of different species of
<italic>Acanthotricolpites</italic>, along with pollen grains of
<italic>Spinizonocolpites</italic> and <italic>Proxapertites</italic>. It is similar to the
<italic>Apectodinium homomorphum</italic> cenozone in the distribution of
palynomorphs with a reduction in marine taxa and an increment in the number
of <italic>Acanthotricolpites </italic>spp. The cenozone is named after the rise in
the percentage of various species of <italic>Acanthotricolpites</italic> genera. The
other essential taxa are <italic>Spinizonocolpites echinatus, S. brevispinosus, S. baculatus, S. bulbospinosus, Proxapertites cursus, P. microreticulatus, P. crassimurus, Acanthotricolpites brevispinosus, A. robustus, A. bulbospinosus, Arengapollenites achinatus, Longapertites retipilatus</italic> and  <italic>Kapurdipollenites gemmatus</italic>. The percentage of dinocysts is
decreasing compared to the earlier zone.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx14" specific-use="unnumbered">
  <title>Lower limit</title>
      <p id="d1e1200">Lignite seam above the marine-fossil-bearing shale unit.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx15" specific-use="unnumbered">
  <title>Upper limit</title>
      <p id="d1e1209">The overlying bentonite just above the last lignite seam in the exposure.</p>
</sec>
<sec id="Ch1.S3.SS2.SSS2">
  <title>Surkha mine</title>
      <p id="d1e1219">Out of the eight samples, only samples from five horizons yielded
palynomorphs. Palynomorphs ascribed as pteridophytic spores have been
assigned to six genera and eight species, while 12 genera and 22 species have
been identified as angiosperm pollen. Spores, hyphae and microthyraceous
fruiting bodies constitute the fungal remains. The angiosperms dominate the
assemblage with a low percentage of pteridophytes. The gymnospermous pollen
grains are absent in the assemblage. The assemblage has been divided into two
cenozones viz. (i) <italic>Retipollenites borrasodendrii<?pagebreak page13?></italic> cenozone and
(ii) <italic>Spinizonocolpites</italic> spp. cenozone. The lowermost part of the
section is comprised of tropical rainforest elements, whereas mangrove
elements dominate the section towards the upper part. The angiosperm pollen
of the <italic>Arecaceae</italic> family is dominant over all the other groups of
palynomorphs. The cenozones in the Surkha mine are demarcated in Fig. 4.</p>
      <p id="d1e1231"><list list-type="custom">
              <list-item><label> </label>

      <p id="d1e1236"><italic>Retipollenites borrasodendrii</italic> cenozone</p>
              </list-item>
            </list></p>
</sec>
<sec id="Ch1.S3.SS2.SSSx16" specific-use="unnumbered">
  <title>Lithology</title>
      <p id="d1e1249">Lignite with shale intercalations at 3 m from the base. Thickness is about
4 m.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx17" specific-use="unnumbered">
  <title>Position</title>
      <p id="d1e1258">From sample no. BN 12/1 to BN 12/3.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx18" specific-use="unnumbered">
  <title>Important taxa</title>
      <p id="d1e1267">This cenozone is marked by a high percentage of <italic>Retipollenites borrasodendrii</italic> (up to 91 %) and <italic>Retipollenites confuses</italic> which
does not occur in the younger zone. Other significant taxa represented in the
cenozone are <italic>Tribrevicolporites eocenicus, Lakiapollis ovatus, Arengapollenites achinatus, Retistephanocolpites</italic> spp.,
<italic>Acanthotricolpites kutchensis</italic> and <italic>Todisporites minor</italic>.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx19" specific-use="unnumbered">
  <title>Lower limit</title>
      <p id="d1e1291">The lower limit is not traceable.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx20" specific-use="unnumbered">
  <title>Upper limit</title>
      <p id="d1e1300">Significant decrease in the percentage of <italic>Retipollenites</italic>.</p>
      <p id="d1e1306"><list list-type="custom">
              <list-item><label> </label>

      <p id="d1e1311"><italic>Spinizonocolpites</italic> spp. cenozone</p>
              </list-item>
            </list></p>
</sec>
<sec id="Ch1.S3.SS2.SSSx21" specific-use="unnumbered">
  <title>Lithology</title>
      <p id="d1e1325">Comprised of carbonaceous shales. Thickness is about 4 m.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx22" specific-use="unnumbered">
  <title>Position</title>
      <p id="d1e1334">From sample no. BN 12/5 to BN 12/7.</p>
      <p id="d1e1337">This cenozone is marked by an appreciable decrease in the percentage of
<italic>Retipollenites</italic> spp. (from 91 % to 2 %), the first appearance
of <italic>Spinizonocolpites echinatus</italic> and dinocysts.<?pagebreak page14?> The cenozone is
comprised of arecaceous pollen <italic>Spinizonocolpites, Proxapertites, Neocouperipollis, Retimonosulcites</italic> and <italic>Acanthotricolpites</italic>. The
pollen ascribed to <italic>Spinizonocolpites</italic> (about 21 %) dominates the
assemblage; hence, the cenozone is named after it. Some of the other taxa
found are <italic>Arengapollenites achinatus, Tribrevicolporites eocenicus, Longapertites</italic> sp., <italic>Retipollenites</italic> spp.,
<italic>Kutchiathyrites</italic> spp. and <italic>Phragmothyrites</italic> spp.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx23" specific-use="unnumbered">
  <title>Lower limit</title>
      <p id="d1e1374">Appearance of dinoflagellates.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx24" specific-use="unnumbered">
  <title>Upper limit</title>
      <p id="d1e1383">Bentonite layer.</p>
</sec>
<sec id="Ch1.S3.SS2.SSS3">
  <title>Matanomadh mine</title>
      <p id="d1e1392">Palynological analysis of 23 samples from the Matanomadh mine section
was accomplished. The lower part of the mine section includes pollen and
spores with sparse dinocysts. Well-preserved and abundant dinocysts
characterize the top part of the section. The entire lithocolumn is dominated
by dinocysts, followed by the pollen of the <italic>Arecaceae</italic> family
(<italic>Spinizonocolpites, Acanthotricolpites, Proxapertites</italic>). Based on
variations in the percentage of the different species, three cenozones were
identified (Fig. 5) in the assemblage as follows:</p>
      <p id="d1e1401"><list list-type="custom">
              <list-item><label> </label>

      <p id="d1e1406"><italic>Spinizonocolpites spp.</italic> cenozone</p>
              </list-item>
            </list></p>
</sec>
<sec id="Ch1.S3.SS2.SSSx25" specific-use="unnumbered">
  <title>Lithology</title>
      <p id="d1e1419">The lowermost lignite and intervening shale unit. Thickness is about 8 m.</p>
</sec>
<?pagebreak page15?><sec id="Ch1.S3.SS2.SSSx26" specific-use="unnumbered">
  <title>Position</title>
      <p id="d1e1429">From sample no. KM-12/19 to KM-12/23.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx27" specific-use="unnumbered">
  <title>Important taxa</title>
      <p id="d1e1438">In relation to the overlying assemblage, the litho-unit of this cenozone is
poor in pollen yield. All the samples were studied but the pollen diagram
shows the presence of palynomorphs only at sample number KM-12/23, as the
yield was not enough for quantitative analysis from other samples. In the
samples at other depths, <italic>Spinizonocolpites echinatus</italic> and
<italic>Polysphaeridium subtile</italic> mark their appearance, but the low percentage
was a constraint for the quantification at these depths. The cenozone is
named after the presence of <italic>Spinizonocolpites echinatus</italic> present
throughout the cenozone. The lower part of lignite consists of terrestrial
palynomorphs, belonging to <italic>Arecaceae</italic>. The other essential taxa
recovered are <italic>Spinizonocolpites bulbospinosus, Proxapertites cursus, Acanthotricolpites kutchensis</italic> and <italic>Albertipollenites crassireticulatus</italic>. The
dinocysts which make their appearance in this zone are <italic>Achomosphaera</italic>
sp., <italic>Eocladopyxis peniculata, Homotryblium</italic> sp., <italic>Kenleyia </italic>sp<italic>., Spiniferites ramosus, Glaphyrocysta exuberans</italic> and
<italic>Polysphaeridium subtile</italic>. The dinocyst assemblage is comprised of
<italic>Cordosphaeridium exilimurum, Eocladopyxis peniculata, Glaphyrocysta exuberans, Homotryblium</italic> sp., <italic>Hystrichostrogylon membraniphorum, Polysphaeridium subtile, Spiniferites ramosus</italic> and <italic>Thalassiphora pelagica</italic>. The assemblage of dinocysts is dominated by the genera
<italic>Polysphaeridium subtile</italic>, <italic>Glaphyrocysta exuberans</italic> and
<italic>Cordosphaeridium exilimurum</italic>. They are observed throughout the
section.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx28" specific-use="unnumbered">
  <title>Lower limit</title>
      <p id="d1e1500">The lower limit is not traceable.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx29" specific-use="unnumbered">
  <title>Upper limit</title>
      <p id="d1e1509">The upper contact is the overlying green shale bed.</p>
      <p id="d1e1512"><list list-type="custom">
              <list-item><label> </label>

      <p id="d1e1517"><italic>Homotryblium floripes</italic> cenozone</p>
              </list-item>
            </list></p>
</sec>
<sec id="Ch1.S3.SS2.SSSx30" specific-use="unnumbered">
  <title>Lithology</title>
      <p id="d1e1530">Green shales just above the second lignite seam. Thickness is about 3 m.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx31" specific-use="unnumbered">
  <title>Position</title>
      <p id="d1e1539">From sample no. KM-12/17 to KM-12/7.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx32" specific-use="unnumbered">
  <title>Important taxa</title>
      <p id="d1e1549">The cenozone is characterized by the absolute dominance of dinocysts with the
presence of <italic>Albertipollenites crassireticulatus</italic> only at one level.
The cenozone is named after the first occurrence of the <italic>Homotryblium floripes</italic> dinocyst, which is an age marker taxon. The important taxa from the
shale beds are <italic>Achomosphaera</italic> spp., <italic>Cordosphaeridium cantharellum, C. exilimurum, Glaphyrocysta exuberans, Homotryblium floripes, Hystricholpoma cinctum, Pentadinium</italic> sp., <italic>Kenleyia</italic> spp.,
<italic>Operculodinium divergence, Polysphaeridium subtile, Spiniferites ramosus</italic> and <italic>Thalassiphora</italic> <italic>pelagica</italic>. A reduction in
<italic>Polysphaeridium subtile</italic> and <italic>Thalassiphora pelagica</italic> species
is observed from the bottom to the top of the section. The assemblage is dominated by
<italic>Spiniferites</italic> sp. and <italic>Operculodinium</italic> spp.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx33" specific-use="unnumbered">
  <title>Lower limit</title>
      <p id="d1e1596">The second lignite seam.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx34" specific-use="unnumbered">
  <title>Upper limit</title>
      <p id="d1e1605">The upper contact is the overlying calcareous mudstone.</p>
      <p id="d1e1608"><list list-type="custom">
              <list-item><label> </label>

      <p id="d1e1613"><italic>Glaphyrocysta exuberans</italic> cenozone</p>
              </list-item>
            </list></p>
</sec>
<sec id="Ch1.S3.SS2.SSSx35" specific-use="unnumbered">
  <title>Lithology</title>
      <p id="d1e1626">Calcareous mudstone. Thickness is about 4 m.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx36" specific-use="unnumbered">
  <title>Position</title>
      <p id="d1e1635">From sample no. KM-12/11 to KM-12/16.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx37" specific-use="unnumbered">
  <title>Important taxa</title>
      <p id="d1e1644">This cenozone lies above the green shale layer.
Here, mangrove pollen, <italic>Spinizonocolpites echinatus</italic> and
<italic>Albertipollenites crassireticulatus</italic> mark its presence. The dinocysts
which were present in <italic>Homotryblium floripes</italic> cenozone also extended
to this zone but their percentage decreases. A drastic reduction in the
percentage of <italic>Polysphaeridium subtile, Spiniferites ramosus</italic> and
<italic>Operculodinium centrocarpum</italic> is observed. <italic>Wilsonidium</italic>
<italic>tabulatum</italic>, in comparison, appears for the first time in this cenozone.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx38" specific-use="unnumbered">
  <title>Lower limit</title>
      <p id="d1e1676">The unfossiliferous zone just above the green shales.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx39" specific-use="unnumbered">
  <title>Upper limit</title>
      <p id="d1e1685">The upper contact is not discernible.</p>
</sec>
<sec id="Ch1.S3.SS2.SSS4">
  <title>Panandhro mine</title>
      <p id="d1e1694">We have analyzed a total of 16 samples; however, only few yielded good
results. The overall assemblage consists of angiosperms, pteridophytes,
dinocysts and fungal remains.<?pagebreak page16?> Only one or two specimens of dinoflagellate
<italic>Polysphaeridium subtile</italic> were discovered from the basal lignitic seam.</p>
      <p id="d1e1700">The profile has been divided into three cenozones for the convenience of
study (Fig. 6). The cenozones are as follows:
<list list-type="custom"><list-item><label> </label>
      <p id="d1e1705"><italic>Spinizonocolpites echinatus</italic> cenozone</p></list-item></list></p>
</sec>
<sec id="Ch1.S3.SS2.SSSx40" specific-use="unnumbered">
  <title>Lithology</title>
      <p id="d1e1716">Lower lignite is having a thickness of about 8 m.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx41" specific-use="unnumbered">
  <title>Position</title>
      <p id="d1e1725">From sample no. KP-12/1 to KP-12/8.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx42" specific-use="unnumbered">
  <title>Important taxa</title>
      <p id="d1e1734">This cenozone is poorly fossiliferous. The cenozone is named after the
occurrence and abundance of <italic>Spinizonocolpites echinatus</italic>, which marks
its presence at all levels within the cenozone. The pollen spectra are
constructed only for sample number KP-12/5 due to the low percentage of
pollen grains at other depths. <italic>Spinizonocolpites echinatus, Acanthotricolpites kutchensis</italic> and fungal remains were the only palynomorphs
constituting the assemblage.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx43" specific-use="unnumbered">
  <title>Lower limit</title>
      <p id="d1e1750">The basement is not exposed.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx44" specific-use="unnumbered">
  <title>Upper limit</title>
      <p id="d1e1759">The upper contact is <italic>Meliapollis ramanujamii</italic> cenozone.</p>
      <p id="d1e1765"><list list-type="custom">
              <list-item><label> </label>

      <p id="d1e1770"><italic>Meliapollis ramanujamii</italic> cenozone</p>
              </list-item>
            </list></p>
</sec>
<sec id="Ch1.S3.SS2.SSSx45" specific-use="unnumbered">
  <title>Lithology</title>
      <p id="d1e1783">Lignite and overlying highly carbonaceous shale thickness of about 12 m.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx46" specific-use="unnumbered">
  <title>Position</title>
      <p id="d1e1792">From sample no. KP-12/10 to KP-12/18.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx47" specific-use="unnumbered">
  <title>Important taxa</title>
      <p id="d1e1801">The angiosperm pollen predominantly present in the assemblage is comprised of
<italic>Acanthotricolpites, Albertipollenites crassireticulatus, Ctenolophonidites costatus</italic>, <italic>Dipterocarpuspollenites retipilatus, Incrotonipollis neyveli, Meliapollis ramanujamii, Paleosantalaceaepites</italic> <italic>distinctus, Proxapertites, Spinizonocolpites echinatus, Spinizonocolpites bulbospinosus, Spinomonosulcites, Spinulotetradites juxtatus, Tribrevicolporites sp.</italic>
<italic>Meliapollis ramanujamii and Incrotonipollis neyveli</italic> are restricted to this zone only.</p>
      <p id="d1e1816">Pteridophytes and fungal fruiting bodies were also observed in this
cenozone.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx48" specific-use="unnumbered">
  <title>Lower limit</title>
      <p id="d1e1825">This zone lies above the thin band of dark grey carbonaceous shale.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx49" specific-use="unnumbered">
  <title>Upper limit</title>
      <p id="d1e1835">The upper contact is the overlying carbonaceous shale bed with sand lenses.</p>
      <p id="d1e1838"><list list-type="custom">
              <list-item><label> </label>

      <p id="d1e1843"><italic>Kenleyia</italic> spp. cenozone</p>
              </list-item>
            </list></p>
</sec>
<sec id="Ch1.S3.SS2.SSSx50" specific-use="unnumbered">
  <title>Lithology</title>
      <p id="d1e1856">Carbonaceous shales and calcareous green shale, about 15 m thickness.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx51" specific-use="unnumbered">
  <title>Position</title>
      <p id="d1e1865">From sample no. KP-12/20 to KP-12/31.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx52" specific-use="unnumbered">
  <title>Important taxa</title>
      <p id="d1e1874">The cenozone is characterized by the presence of both terrestrial and marine
palynomorphs. The assemblage is comprised of the taxa <italic>Thalassiphora fenestrata, T. patula, Kenleyia</italic> sp., <italic>Glaphyrocysta exuberans, Homotryblium floripes</italic> and <italic>Polysphaeridium subtile</italic>. The cenozone is
named after the dominance of dinocysts ascribed to <italic>Kenleyia</italic> genera.
The angiosperms are the second most dominant group in the assemblage
characterized by the pollen grains of <italic>Albertipollenites crassireticulatus, Ctenolophonidites costatus, Dipterocarpuspollenites retipilatus, Proxapertites cursus, Spinizonocolpites echinatus, S.bulbospinosus</italic> and <italic>Spinomonosulcites echinatus.</italic> The other essential
palynomorphs are <italic>Arengapollenites achinatus, Longapertites</italic> sp.,
<italic>Palmaepollenites ovatus, Lakiapollis ovatus, Retipollenites echinulatus, Incrotonipollis neyveli, Spinulotetradites juxtatus</italic> and
<italic>Margocolporites venkatachalae</italic>, <italic>Tribrevicolporites eocenicus</italic> and <italic>Tricolpites</italic> sp.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx53" specific-use="unnumbered">
  <title>Lower limit</title>
      <p id="d1e1917">The carbonaceous shale with sand lenses. Dinocysts were found from this
level.</p>
</sec>
<sec id="Ch1.S3.SS2.SSSx54" specific-use="unnumbered">
  <title>Upper limit</title>
      <p id="d1e1926">The upper contact is not discernible.</p>
</sec>
</sec>
<?pagebreak page17?><sec id="Ch1.S3.SS3">
  <title>Foraminiferal analysis</title>
      <p id="d1e1936">The lignite mine sections of the Giral and Surkha are devoid of foraminifera.
However, the Matanomadh and Panandhro mine sections are comprised of remarkably
well-preserved foraminifera. The characteristics of foraminifera from these
marginal marine settings are described below.</p>
<sec id="Ch1.S3.SS3.SSS1">
  <title>Bloom of triserial planktic</title>
      <p id="d1e1944">A bloom of planktic foraminifera <italic>Jenkinsina columbiana</italic> (<inline-formula><mml:math id="M10" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> %) is found (40 % of abundance observed at <inline-formula><mml:math id="M11" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">4.5</mml:mn></mml:mrow></mml:math></inline-formula> m and
<inline-formula><mml:math id="M12" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">15</mml:mn></mml:mrow></mml:math></inline-formula> % of abundance at <inline-formula><mml:math id="M13" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">18</mml:mn></mml:mrow></mml:math></inline-formula> m depth) in the Panandhro
lignite mine (Fig. 11a). The triserial planktic foraminifera are usually
observed in the top portion of the seawater along the continental margins,
and its percentage increases near the shelf edge, indicating eutrophic
conditions (Kroon and Nederbragt, 1990).</p>
</sec>
<sec id="Ch1.S3.SS3.SSS2">
  <title>Low-diversity assemblages</title>
      <p id="d1e1996">The diversity of foraminifera (planktic plus benthic) remains low in
the Matanomadh (Fig. 11b; Fisher alpha: <inline-formula><mml:math id="M14" display="inline"><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">1.5</mml:mn></mml:mrow></mml:math></inline-formula> to 7 and
Shannon–Weaver indices: <inline-formula><mml:math id="M15" display="inline"><mml:mrow><mml:mi>H</mml:mi><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">1.3</mml:mn></mml:mrow></mml:math></inline-formula> to 2.4) and Panandhro mine sections.
However, towards the top of the Panandhro section, there is a drastic increase in
the diversity (Fig. 11a: from <inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:math></inline-formula> to 47; <inline-formula><mml:math id="M17" display="inline"><mml:mrow><mml:mi>H</mml:mi><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">1.5</mml:mn></mml:mrow></mml:math></inline-formula>
to 3.6) and abundance of foraminifera.</p>
</sec>
<sec id="Ch1.S3.SS3.SSS3">
  <title>High abundance of rectilinear benthic foraminifera</title>
      <p id="d1e2053">The RBF percentage in the Matanomadh mine section is quite high throughout (<inline-formula><mml:math id="M18" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">40</mml:mn></mml:mrow></mml:math></inline-formula> %). <italic>Brizalina</italic> sp. (<inline-formula><mml:math id="M19" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> % to 45 %) and
<italic>Trifarina advena rajasthanensis</italic> (<inline-formula><mml:math id="M20" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">20</mml:mn></mml:mrow></mml:math></inline-formula> %–45 %) species
belonging to the RBF morphogroup are abundant in the Matanomadh section
(Fig. 11b). In the Panandhro section, the RBF percentage varies between <inline-formula><mml:math id="M21" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> % and 20 %. <italic>Brizalina</italic> sp. (<inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> % to 10 %)
belonging to RBF morphogroups are common in the Panandhro section (Fig. 11a).</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S4">
  <title>Discussion</title>
      <p id="d1e2125">The Indian subcontinent began its northward journey after its separation from
the Gondwanaland around the Cretaceous (P. Kumar et al., 2007). The
subcontinent carried flora and fauna from Africa to Asia. The Deccan
volcanism covered the western and central portions of the subcontinent with
basaltic lava flows, rendering it inhospitable for the growth of flora and
fauna on the mainland. Following this, during the Late Paleocene, extensive
weathering occurred, which gave rise to the soil cover in the subcontinent.
The phase of sediment deposition occurred around the Early Eocene, coinciding
with the marine transgression along the Kutch, Cambay and Rajasthan basins.
Major parts of the mainland were covered with marine sediments ranging from
glauconitic shales to limestones; however, some restricted marine areas along
the coast gave rise to lignite deposits comprised dominantly of angiosperms
(Sarkar et al., 2012; Saraswati et al., 2012).</p>
<sec id="Ch1.S4.SS1">
  <title>Paleoenvironment in the Early Eocene in western India</title>
      <p id="d1e2133">In the Early Eocene, India was positioned at the Equator (Ocean Drilling
Stratigraphic Network, 2004), and the tropical climate enhanced the
production of mangrove forests along the western coast of India (Fig. 1a).
The modern analog of these are the Sunderbans
mangrove forests, along the Ganges–Brahmaputra Delta on the eastern coast of
India. The Early Eocene sections of the Surkha and Giral mines consist of
palynofloral assemblage belonging to the <italic>Arecaceae, Cyatheaceae, Lycopodiaceae, Matoniaceae, Osmundaceae, Schizaeaceae, Ctenolophonaceae, Sapotaceae, Alangiaceae</italic> and <italic>Bombacaceae</italic> families which relate to
subtropical–tropical climate in their present-day distribution (Sect. S3 in
the Supplement).</p>
      <p id="d1e2142">The lignite seams from both the Giral and Surkha mines are dominant in tropical
rainforest elements (<italic>Retipollenites, Arengapollenites, Longapertites</italic>), which declines gradually towards the top of the section
(Figs. 3 and 4). The basal zone consisting of the tropical rainforest gets
steadily replaced by an ecosystem in which mangroves form the majority
(mangroves <inline-formula><mml:math id="M23" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">55</mml:mn></mml:mrow></mml:math></inline-formula> %–100 % in all samples in the Giral mine; Fig. 7;
<inline-formula><mml:math id="M24" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">20</mml:mn></mml:mrow></mml:math></inline-formula> %–80 % in most samples of the Surkha mine; Fig. 8). The
abundance of mangrove elements (<italic>Nypa</italic>), along with the appearance of
dinoflagellates, increases in the shales deposited above the lignite seam (in
the Surkha mine, dinoflagellate abundance reaches 45 %; Fig. 8; in the
Giral mine, it reaches 25 % above the lignite; Fig. 7). Different species of mangrove
elements (<italic>Nypa</italic>) like <italic>Proxapertites, Palmaepollenites, Spinizonocolpites</italic> and   <italic>Acanthotricolpites</italic> were observed towards the top of the
Giral and Surkha mine sections, which indicate the proximity of the site of
deposition to the coastal area. The size of <italic>Nypa</italic> pollen is quite
large and hence cannot be transported to more considerable distances, and thus
its abundance indicates that the source and depositional site were not
entirely far off (Chaloner, 1968). <italic>Lakiapollis ovatus,</italic> which is
observed in the basal part (<inline-formula><mml:math id="M25" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">8</mml:mn></mml:mrow></mml:math></inline-formula> m depth; Fig. 4) of the Surkha mine
section, exhibits affinity with the modern plant <italic>Durio</italic>, which is
currently found in Indo-Malayan tropics. The taxa <italic>Lakiapollis ovatus</italic> (<italic>Todisporites major</italic>, <italic>T. minor</italic>),
<italic>Laevigatosporites cognatus, Polypodiisporites repandus</italic> and
<italic>Lycopodiumsporites</italic> are found in the lowermost part of the Surkha mine
section constituting tropical rainforest vegetation and were gradually
replaced by mangroves (Figs. 4 and 8) towards the top. A warm, humid climatic
condition with high precipitation is indicated by the presence of
microthyriaceous fungal fruiting bodies (Dilcher, 1965; Selkirk, 1975) in the
<italic>Apectodinium homomorphum</italic> cenozone of the Giral mine section (Fig. 3).
The dominance of mangroves towards the top of the section in both the Giral and
Surkha mines is indicative of the increase of coastal<?pagebreak page18?> water influence on the
mainland (Figs. 3 and 4). The dinoflagellates which are commonly found in the
Cambay and Giral mine sections consist of <italic>Kenleyia</italic> sp.,
<italic>Cordosphaeridium</italic> sp. and <italic>Apectodinium homomorphum</italic>,
respectively. The first occurrence of <italic>Apectodinium homomorphum</italic> is
observed in the middle part of the Giral mine (<inline-formula><mml:math id="M26" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">7</mml:mn></mml:mrow></mml:math></inline-formula> m depth; Fig. 3), which
indicates deposition at high temperatures (Frieling and Sluijs, 2018),
especially during the PETM. In the Surkha section, the thermophilic
dinoflagellates <italic>Cordosphaeridium</italic> sp. and <italic>Achomosphaera</italic> sp.
are found, which also indicates deposition at high temperatures.</p>

<?xmltex \floatpos{p}?><table-wrap id="Ch1.T1" specific-use="star" orientation="landscape"><caption><p id="d1e2252">Similarities and differences between the Early and Middle Eocene
lignites from western India based on diversity, abundance of various groups
of palynomorphs and foraminifera.</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.80}[.80]?><oasis:tgroup cols="12">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:colspec colnum="4" colname="col4" align="left"/>
     <oasis:colspec colnum="5" colname="col5" align="left"/>
     <oasis:colspec colnum="6" colname="col6" align="left"/>
     <oasis:colspec colnum="7" colname="col7" align="left"/>
     <oasis:colspec colnum="8" colname="col8" align="left" colsep="1"/>
     <oasis:colspec colnum="9" colname="col9" align="left"/>
     <oasis:colspec colnum="10" colname="col10" align="left"/>
     <oasis:colspec colnum="11" colname="col11" align="left"/>
     <oasis:colspec colnum="12" colname="col12" align="justify" colwidth="142.26378pt"/>
     <oasis:thead>
       <oasis:row>

         <oasis:entry colname="col1">Age</oasis:entry>

         <oasis:entry namest="col2" nameend="col3" align="center">Area of </oasis:entry>

         <oasis:entry colname="col4">Lithology</oasis:entry>

         <oasis:entry namest="col5" nameend="col8" align="center" colsep="1">Characteristics of  </oasis:entry>

         <oasis:entry namest="col9" nameend="col11" align="center">Characteristics of </oasis:entry>

         <oasis:entry colname="col12">Paleoenvironment</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1"/>

         <oasis:entry namest="col2" nameend="col3" align="center">study </oasis:entry>

         <oasis:entry colname="col4"/>

         <oasis:entry rowsep="1" namest="col5" nameend="col8" align="center" colsep="1">palynomorph assemblages </oasis:entry>

         <oasis:entry rowsep="1" namest="col9" nameend="col11" align="center">foraminiferal assemblages </oasis:entry>

         <oasis:entry colname="col12"/>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1"/>

         <oasis:entry colname="col2"/>

         <oasis:entry colname="col3"/>

         <oasis:entry colname="col4"/>

         <oasis:entry colname="col5">Mangrove</oasis:entry>

         <oasis:entry colname="col6">Rainforest</oasis:entry>

         <oasis:entry colname="col7">Percentage of dinoflag-</oasis:entry>

         <oasis:entry colname="col8">Thermophilic</oasis:entry>

         <oasis:entry colname="col9">Fisher</oasis:entry>

         <oasis:entry colname="col10">RBF %</oasis:entry>

         <oasis:entry colname="col11">Biserial and</oasis:entry>

         <oasis:entry colname="col12"/>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1"/>

         <oasis:entry colname="col2"/>

         <oasis:entry colname="col3"/>

         <oasis:entry colname="col4"/>

         <oasis:entry colname="col5">elements</oasis:entry>

         <oasis:entry colname="col6">elements</oasis:entry>

         <oasis:entry colname="col7">ellates</oasis:entry>

         <oasis:entry colname="col8">dinoflag-</oasis:entry>

         <oasis:entry colname="col9">alpha</oasis:entry>

         <oasis:entry colname="col10"/>

         <oasis:entry colname="col11">triserial</oasis:entry>

         <oasis:entry colname="col12"/>

       </oasis:row>
       <oasis:row rowsep="1">

         <oasis:entry colname="col1"/>

         <oasis:entry colname="col2"/>

         <oasis:entry colname="col3"/>

         <oasis:entry colname="col4"/>

         <oasis:entry colname="col5"/>

         <oasis:entry colname="col6"/>

         <oasis:entry colname="col7"/>

         <oasis:entry colname="col8">ellates</oasis:entry>

         <oasis:entry colname="col9"/>

         <oasis:entry colname="col10"/>

         <oasis:entry colname="col11">planktic %</oasis:entry>

         <oasis:entry colname="col12"/>

       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>

         <oasis:entry colname="col1">Middle</oasis:entry>

         <oasis:entry colname="col2">Kutch</oasis:entry>

         <oasis:entry colname="col3">Matanomadh</oasis:entry>

         <oasis:entry colname="col4">Lignite</oasis:entry>

         <oasis:entry colname="col5"><inline-formula><mml:math id="M27" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">28</mml:mn></mml:mrow></mml:math></inline-formula> %</oasis:entry>

         <oasis:entry colname="col6"><italic>Albertipollenites</italic></oasis:entry>

         <oasis:entry colname="col7"><inline-formula><mml:math id="M28" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">45</mml:mn></mml:mrow></mml:math></inline-formula> %–</oasis:entry>

         <oasis:entry colname="col8"><italic>Cordosphaeridium</italic></oasis:entry>

         <oasis:entry colname="col9">1.5–7</oasis:entry>

         <oasis:entry colname="col10">7 %–</oasis:entry>

         <oasis:entry colname="col11">–</oasis:entry>

         <?xmltex \mrwidth{142.26378pt}?><oasis:entry rowsep="1" colname="col12" morerows="11">Eutrophic, high runoff,<?xmltex \hack{\break}?> upwelling conditions are observed in<?xmltex \hack{\break}?> the basal to middle part of the mine sections. The switch to oligotrophic conditions as observed by the increase in abundance of planktic foraminifera and dinoflagellates towards the topmost part of the mine section corresponds to Kirthar–Wilson Bluff transgression, probably caused as an aftermath of the MECO warming event.</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1">Eocene</oasis:entry>

         <oasis:entry colname="col2">Basin</oasis:entry>

         <oasis:entry colname="col3">lignite</oasis:entry>

         <oasis:entry colname="col4">shale</oasis:entry>

         <oasis:entry colname="col5"/>

         <oasis:entry colname="col6"><italic>crassireticulatus</italic></oasis:entry>

         <oasis:entry colname="col7">98 %</oasis:entry>

         <oasis:entry colname="col8">sp.</oasis:entry>

         <oasis:entry colname="col9"/>

         <oasis:entry colname="col10">24 %</oasis:entry>

         <oasis:entry colname="col11"/>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1"/>

         <oasis:entry colname="col2"/>

         <oasis:entry rowsep="1" colname="col3">mine</oasis:entry>

         <oasis:entry rowsep="1" colname="col4">mudstone</oasis:entry>

         <oasis:entry rowsep="1" colname="col5"/>

         <oasis:entry rowsep="1" colname="col6"/>

         <oasis:entry rowsep="1" colname="col7"/>

         <oasis:entry rowsep="1" colname="col8"/>

         <oasis:entry rowsep="1" colname="col9"/>

         <oasis:entry rowsep="1" colname="col10"/>

         <oasis:entry rowsep="1" colname="col11"/>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1"/>

         <oasis:entry colname="col2"/>

         <oasis:entry colname="col3">Panandhro</oasis:entry>

         <oasis:entry colname="col4">Lignite,</oasis:entry>

         <oasis:entry colname="col5"><inline-formula><mml:math id="M29" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">20</mml:mn></mml:mrow></mml:math></inline-formula> %–40 %</oasis:entry>

         <oasis:entry colname="col6"><italic>Albertipollenites</italic></oasis:entry>

         <oasis:entry colname="col7"><inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">80</mml:mn></mml:mrow></mml:math></inline-formula> %</oasis:entry>

         <oasis:entry colname="col8"><italic>Kenleyia</italic> sp.</oasis:entry>

         <oasis:entry colname="col9"><inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:math></inline-formula> in</oasis:entry>

         <oasis:entry colname="col10">25 %–</oasis:entry>

         <oasis:entry colname="col11"><inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">15</mml:mn></mml:mrow></mml:math></inline-formula> %–</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1"/>

         <oasis:entry colname="col2"/>

         <oasis:entry colname="col3">lignite</oasis:entry>

         <oasis:entry colname="col4">shale,</oasis:entry>

         <oasis:entry colname="col5">in upper part</oasis:entry>

         <oasis:entry colname="col6"><italic>crassireticulatus</italic>,</oasis:entry>

         <oasis:entry colname="col7"/>

         <oasis:entry colname="col8"/>

         <oasis:entry colname="col9">basal and</oasis:entry>

         <oasis:entry colname="col10">43 %</oasis:entry>

         <oasis:entry colname="col11">40 %</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1"/>

         <oasis:entry colname="col2"/>

         <oasis:entry colname="col3">mine</oasis:entry>

         <oasis:entry colname="col4">limestone</oasis:entry>

         <oasis:entry colname="col5">and 90 % in</oasis:entry>

         <oasis:entry colname="col6"><italic>Meliapollis</italic></oasis:entry>

         <oasis:entry colname="col7"/>

         <oasis:entry colname="col8"/>

         <oasis:entry colname="col9">middle</oasis:entry>

         <oasis:entry colname="col10"/>

         <oasis:entry colname="col11"/>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1"/>

         <oasis:entry colname="col2"/>

         <oasis:entry colname="col3"/>

         <oasis:entry colname="col4"/>

         <oasis:entry colname="col5">basal part</oasis:entry>

         <oasis:entry colname="col6"><italic>ramanujamii</italic>,</oasis:entry>

         <oasis:entry colname="col7"/>

         <oasis:entry colname="col8"/>

         <oasis:entry colname="col9">levels</oasis:entry>

         <oasis:entry colname="col10"/>

         <oasis:entry colname="col11"/>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1"/>

         <oasis:entry colname="col2"/>

         <oasis:entry colname="col3"/>

         <oasis:entry colname="col4"/>

         <oasis:entry colname="col5"/>

         <oasis:entry colname="col6"><italic>Incrotonipollis</italic></oasis:entry>

         <oasis:entry colname="col7"/>

         <oasis:entry colname="col8"/>

         <oasis:entry colname="col9">and 47</oasis:entry>

         <oasis:entry colname="col10"/>

         <oasis:entry colname="col11"/>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1"/>

         <oasis:entry colname="col2"/>

         <oasis:entry colname="col3"/>

         <oasis:entry colname="col4"/>

         <oasis:entry colname="col5"/>

         <oasis:entry colname="col6"><italic>neyveli</italic></oasis:entry>

         <oasis:entry colname="col7"/>

         <oasis:entry colname="col8"/>

         <oasis:entry colname="col9">at the</oasis:entry>

         <oasis:entry colname="col10"/>

         <oasis:entry colname="col11"/>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1"/>

         <oasis:entry colname="col2"/>

         <oasis:entry colname="col3"/>

         <oasis:entry colname="col4"/>

         <oasis:entry colname="col5"/>

         <oasis:entry colname="col6"/>

         <oasis:entry colname="col7"/>

         <oasis:entry colname="col8"/>

         <oasis:entry colname="col9">top</oasis:entry>

         <oasis:entry colname="col10"/>

         <oasis:entry colname="col11"/>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1"/>

         <oasis:entry colname="col2"/>

         <oasis:entry colname="col3"/>

         <oasis:entry colname="col4"/>

         <oasis:entry colname="col5"/>

         <oasis:entry colname="col6"/>

         <oasis:entry colname="col7"/>

         <oasis:entry colname="col8"/>

         <oasis:entry colname="col9"/>

         <oasis:entry colname="col10"/>

         <oasis:entry colname="col11"/>

       </oasis:row>
       <oasis:row rowsep="1">

         <oasis:entry colname="col1"/>

         <oasis:entry colname="col2"/>

         <oasis:entry colname="col3"/>

         <oasis:entry colname="col4"/>

         <oasis:entry colname="col5"/>

         <oasis:entry colname="col6"/>

         <oasis:entry colname="col7"/>

         <oasis:entry colname="col8"/>

         <oasis:entry colname="col9"/>

         <oasis:entry colname="col10"/>

         <oasis:entry colname="col11"/>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1">Early</oasis:entry>

         <oasis:entry namest="col2" nameend="col3" align="center">Cambay Basin </oasis:entry>

         <oasis:entry colname="col4">Lignite,</oasis:entry>

         <oasis:entry colname="col5">20 %–80 %</oasis:entry>

         <oasis:entry colname="col6"><italic>Lakiapollis ovatus</italic>,</oasis:entry>

         <oasis:entry colname="col7"><inline-formula><mml:math id="M33" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">45</mml:mn></mml:mrow></mml:math></inline-formula> %</oasis:entry>

         <oasis:entry colname="col8"><italic>Achomosphaera</italic> sp.,</oasis:entry>

         <oasis:entry namest="col9" nameend="col11" align="center">Foraminifera were not </oasis:entry>

         <?xmltex \mrwidth{5cm}?><oasis:entry colname="col12" morerows="12">The percentage of thermophilic <italic>Nypa</italic> pollen is quite high compared to that of Middle Eocene sections of the Matanomadh and Panandhro mines.  The existence of high abundance of rainforest elements indicate the presence of thick vegetation. The percentage of dinoflagellates is lower compared to Middle Eocene sections, indicating deposition in less depth. The presence of thermophilic dinoflagellates indicates high temperatures during the Early Eocene.</oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1">Eocene</oasis:entry>

         <oasis:entry namest="col2" nameend="col3" align="center">(Surkha lignite </oasis:entry>

         <oasis:entry colname="col4">shale</oasis:entry>

         <oasis:entry colname="col5"/>

         <oasis:entry colname="col6"><italic>Laevigatosporites</italic></oasis:entry>

         <oasis:entry colname="col7"/>

         <oasis:entry colname="col8"><italic>Cordosphaeridium</italic> sp.</oasis:entry>

         <oasis:entry namest="col9" nameend="col11" align="center">present in the samples </oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1"/>

         <oasis:entry namest="col2" nameend="col3" align="center">mine) </oasis:entry>

         <oasis:entry colname="col4"/>

         <oasis:entry colname="col5"/>

         <oasis:entry colname="col6"><italic>cognatus</italic>,</oasis:entry>

         <oasis:entry colname="col7"/>

         <oasis:entry colname="col8"><italic>Cordosphaeridium</italic> sp.</oasis:entry>

         <oasis:entry namest="col9" nameend="col11" align="center">of these mine sections </oasis:entry>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1"/>

         <oasis:entry colname="col2"/>

         <oasis:entry colname="col3"/>

         <oasis:entry colname="col4"/>

         <oasis:entry colname="col5"/>

         <oasis:entry colname="col6"><italic>Polypodiisporites</italic></oasis:entry>

         <oasis:entry colname="col7"/>

         <oasis:entry colname="col8"/>

         <oasis:entry colname="col9"/>

         <oasis:entry colname="col10"/>

         <oasis:entry colname="col11"/>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1"/>

         <oasis:entry colname="col2"/>

         <oasis:entry colname="col3"/>

         <oasis:entry colname="col4"/>

         <oasis:entry colname="col5"/>

         <oasis:entry colname="col6"><italic>repandus</italic>,</oasis:entry>

         <oasis:entry colname="col7"/>

         <oasis:entry colname="col8"/>

         <oasis:entry colname="col9"/>

         <oasis:entry colname="col10"/>

         <oasis:entry colname="col11"/>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1"/>

         <oasis:entry rowsep="1" colname="col2"/>

         <oasis:entry rowsep="1" colname="col3"/>

         <oasis:entry colname="col4"/>

         <oasis:entry rowsep="1" colname="col5"/>

         <oasis:entry rowsep="1" colname="col6"><italic>Lycopodiumsporites</italic></oasis:entry>

         <oasis:entry rowsep="1" colname="col7"/>

         <oasis:entry rowsep="1" colname="col8"/>

         <oasis:entry colname="col9"/>

         <oasis:entry colname="col10"/>

         <oasis:entry colname="col11"/>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1"/>

         <oasis:entry namest="col2" nameend="col3" align="center">Barmer Basin </oasis:entry>

         <oasis:entry colname="col4"/>

         <oasis:entry colname="col5">55 %–100 %</oasis:entry>

         <oasis:entry colname="col6"><italic>Longapertites</italic>,</oasis:entry>

         <oasis:entry colname="col7"><inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">25</mml:mn></mml:mrow></mml:math></inline-formula> %</oasis:entry>

         <oasis:entry colname="col8"><italic>Apectodinium</italic></oasis:entry>

         <oasis:entry colname="col9"/>

         <oasis:entry colname="col10"/>

         <oasis:entry colname="col11"/>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1"/>

         <oasis:entry namest="col2" nameend="col3" align="center">(Giral lignite </oasis:entry>

         <oasis:entry colname="col4"/>

         <oasis:entry colname="col5"/>

         <oasis:entry colname="col6"><italic>Arengapollenites</italic>,</oasis:entry>

         <oasis:entry colname="col7"/>

         <oasis:entry colname="col8"><italic>homomorphum</italic>,</oasis:entry>

         <oasis:entry colname="col9"/>

         <oasis:entry colname="col10"/>

         <oasis:entry colname="col11"/>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1"/>

         <oasis:entry namest="col2" nameend="col3" align="center">mine) </oasis:entry>

         <oasis:entry colname="col4"/>

         <oasis:entry colname="col5"/>

         <oasis:entry colname="col6"><italic>Retipollenites</italic></oasis:entry>

         <oasis:entry colname="col7"/>

         <oasis:entry colname="col8"><italic>Kenleyia</italic> sp.</oasis:entry>

         <oasis:entry colname="col9"/>

         <oasis:entry colname="col10"/>

         <oasis:entry colname="col11"/>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1"/>

         <oasis:entry colname="col2"/>

         <oasis:entry colname="col3"/>

         <oasis:entry colname="col4"/>

         <oasis:entry colname="col5"/>

         <oasis:entry colname="col6"/>

         <oasis:entry colname="col7"/>

         <oasis:entry colname="col8"/>

         <oasis:entry colname="col9"/>

         <oasis:entry colname="col10"/>

         <oasis:entry colname="col11"/>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1"/>

         <oasis:entry colname="col2"/>

         <oasis:entry colname="col3"/>

         <oasis:entry colname="col4"/>

         <oasis:entry colname="col5"/>

         <oasis:entry colname="col6"/>

         <oasis:entry colname="col7"/>

         <oasis:entry colname="col8"/>

         <oasis:entry colname="col9"/>

         <oasis:entry colname="col10"/>

         <oasis:entry colname="col11"/>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1"/>

         <oasis:entry colname="col2"/>

         <oasis:entry colname="col3"/>

         <oasis:entry colname="col4"/>

         <oasis:entry colname="col5"/>

         <oasis:entry colname="col6"/>

         <oasis:entry colname="col7"/>

         <oasis:entry colname="col8"/>

         <oasis:entry colname="col9"/>

         <oasis:entry colname="col10"/>

         <oasis:entry colname="col11"/>

       </oasis:row>
       <oasis:row>

         <oasis:entry colname="col1"/>

         <oasis:entry colname="col2"/>

         <oasis:entry colname="col3"/>

         <oasis:entry colname="col4"/>

         <oasis:entry colname="col5"/>

         <oasis:entry colname="col6"/>

         <oasis:entry colname="col7"/>

         <oasis:entry colname="col8"/>

         <oasis:entry colname="col9"/>

         <oasis:entry colname="col10"/>

         <oasis:entry colname="col11"/>

       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table></table-wrap>

</sec>
<sec id="Ch1.S4.SS2">
  <title>Paleoenvironment during the Middle Eocene in western India</title>
      <?pagebreak page20?><p id="d1e3277">The Indian continent was placed within the tropical belt during the Middle Eocene
(Fig. 1b). The basal part consisting of lignites in both mine
sections of the Kutch Basin exhibits a dominance of <italic>Albertipollenites</italic> and
<italic>Meliapollis ramanujamii</italic>, and <italic>Dipterocarpuspollenites</italic> and
<italic>Incrotonipollis</italic> belonging to family <italic>Euphorbiaceae</italic>. The
dominance of <italic>Euphorbiaceae</italic> is indicative of the prevalence of rainforests
in subtropical to tropical climate (Langenheim, 1995; Dutta et al., 2011).
Even though the vegetation was predominantly angiosperm rich, the percentage
of mangrove forests (particularly the <italic>Nypa</italic> pollen) decreased and
the percentage of dinoflagellates increased (Figs. 9 and 10) in the Middle Eocene
compared to the Early Eocene in western India. The pteridophyte percentage is
also considerably low in the Middle Eocene (<inline-formula><mml:math id="M35" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">25</mml:mn></mml:mrow></mml:math></inline-formula> %), as observed in
both mine sections. The percentage of mangrove elements is very low (<inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">28</mml:mn></mml:mrow></mml:math></inline-formula> %) in the Matanomadh mine section; however, in the Panandhro section, there
is a drastic decrease in percentage of mangrove elements from <inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">90</mml:mn></mml:mrow></mml:math></inline-formula> %
in the basal part to <inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">20</mml:mn></mml:mrow></mml:math></inline-formula> %–40 % in the upper levels. On the
contrary, the dinocysts became quite abundant (<inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">45</mml:mn></mml:mrow></mml:math></inline-formula> %–98 % in
most samples in the Matanomadh section and <inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">80</mml:mn></mml:mrow></mml:math></inline-formula> % at few levels in
the Panandhro section) as compared to Early Eocene sections in the Cambay and Barmer basins.
The abundance of dinoflagellate <italic>Spiniferites</italic> increased towards the
top in both mine sections (<inline-formula><mml:math id="M41" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> % at 9.8 m to <inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">25</mml:mn></mml:mrow></mml:math></inline-formula> %–60 %
between 2 and 6.5 m in the Matanomadh section; refer to
Fig. 5; first appearance at <inline-formula><mml:math id="M43" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">21</mml:mn></mml:mrow></mml:math></inline-formula> m in the top part of the Panandhro
section; refer to Fig. 6), indicating deposition in low-nutrient, low-TOC
(total organic content) and open marine conditions (inner neritic to outer
neritic) (Frieling and Sluijs, 2018; Brinkhuis, 1994) towards the upper
portion of the mine sections. Species of <italic>Operculodinium</italic> are generally
abundant in restricted marine conditions, as observed by Brinkhuis (1994), from
the Late Eocene–Oligocene section of northeast Italy. The abundance of
<italic>Operculodinium</italic> decreases from the bottom to the top within the shale unit
deposited above the lignite seam in the Matanomadh mine (decrease in percentage
from <inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">40</mml:mn></mml:mrow></mml:math></inline-formula> % at 6.8 m within the <italic>Homotryblium floripes</italic>
cenozone to 10 % at 2.8 m within the <italic>Glaphyrocysta exuberans</italic>
cenozone; refer to Fig. 5), indicating a change from restricted marine to an open
marine environment. A high abundance of <italic>Thalassiphora pelagica</italic> is
observed in the carbonaceous shale deposited between two lignite seams (<inline-formula><mml:math id="M45" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">20</mml:mn></mml:mrow></mml:math></inline-formula> % at 9.8 m; refer to Fig. 5) from the Matanomadh mine section, representing
an increase in productivity of surface waters as well as anaerobic bottom
water conditions (Pross, 2001). Similar conditions are observed in the Late
Eocene hemipelagic–pelagic sediments of central Italy (Pross and Schmiedl,
2002; Sluijs et al., 2005). <italic>T. pelagica</italic> in not observed in the upper
portion of the Matanomadh mine section; however, the abundance of
<italic>Homotryblium</italic> increases towards the top (Fig. 5).
<italic>Homotryblium</italic> does not have any extant representatives and is
dominantly found in low-latitude warm climates, especially in restricted
marine settings with increased salinity (Brinkhuis, 1994; Sluijs et al.,
2005), while <italic>T. pelagica</italic> is observed in relatively reduced salinity
conditions. The alternation of abundance between <italic>Homotryblium</italic>
(highest percentage of <inline-formula><mml:math id="M46" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">40</mml:mn></mml:mrow></mml:math></inline-formula> at 6.8 m in the section; Fig. 5) and
<italic>T. pelagica</italic> (highest percentage <inline-formula><mml:math id="M47" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">100</mml:mn></mml:mrow></mml:math></inline-formula> at 9.8 m in the section;
Fig. 5) corresponds to the increase and decrease in salinity conditions,
respectively (Sluijs et al., 2005), in the Matanomadh mine section. The
presence of <italic>Cordosphaeridium </italic>in the green shale (percentage <inline-formula><mml:math id="M48" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula>
to 15 between 2.5 to 6.8 m; refer to Fig. 5) in the Matanomadh mine section
corresponds to high temperature and open marine conditions (Frieling and
Sluijs, 2018) possibly coinciding with MECO warming event in the Bartonian
(Khanolkar et al., 2017). A drastic increase in diversity and abundance of
both planktic and benthic foraminifera is observed at the top part (<inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula> m depth; Fig. 11a) of the Panandhro section, which is also observed across
all sedimentary basins in western India (Saraswati et al., 2018). The sea
level increased on the western margin of India due to the Kirthar
transgression event in the E12 zone, probably related to an aftermath of MECO
(Saraswati et al., 2018). The expression of this event is the deposition of
marine shales above the lignite seams in both the Panandhro and Matanomadh mines
(Fig. 11a and b; Sect. S1 in the Supplement). These marine shales consisted of typical
Bartonian foraminifera like <italic>Acarinina rohri, Acarinina topilensis, Turborotalia frontosa, Nummulites spectabilis, Linderina kutchensis</italic> and
<italic>Halkyardia minima</italic>, and the relative percentage and diversity of foraminifera
and dinoflagellates increased from the Early to Middle Eocene (Khanolkar et al.,
2017; Sharma and Saraswati, 2015). The bloom of triserial planktic
foraminifer <italic>Jenkinsina columbiana</italic> in the glauconitic shale levels
(40 % of abundance observed at <inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">4.5</mml:mn></mml:mrow></mml:math></inline-formula> m and <inline-formula><mml:math id="M51" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">15</mml:mn></mml:mrow></mml:math></inline-formula> % of
abundance at <inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">18</mml:mn></mml:mrow></mml:math></inline-formula> m depth; Fig. 11a) in the Panandhro mine section is
suggestive of dysoxic and upwelling conditions. Concomitantly, a dominance of
rectilinear benthic foraminifera like <italic>Brizalina, Trifarina advena rajasthanensis, Buliminella pupa</italic> and <italic>Buliminella pulchra</italic> (<inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">40</mml:mn></mml:mrow></mml:math></inline-formula> %) from
shales in the Matanomadh mine (especially between 3.5 and 5.5 m depth;
Fig. 11b) is observed, which indicates deposition in low-oxygen and upwelling
conditions (Khanolkar and Saraswati, 2013). The agglutinated foraminifera
like <italic>Miliammina</italic>, <italic>Textularia, Valvulina</italic> and  <italic>Coskinolina</italic> appear
in shale layers above the lignite seam, indicating deposition in marsh and
sheltered conditions (<italic>Coskinolina</italic> and <italic>Valvulina</italic> are
observed between 6 and 6.5 m in shale layers in the  Matanomadh section
(Fig. 11b), while <italic>Miliammina</italic> and <italic>Textularia</italic> are observed between
depths of 1 and 3 m in the mudstone layers of the Panandhro section; Fig. 11a)
(Murray, 2006). The presence of atypical planktic foraminifera from the
Matanomadh section also indicates the stressed condition of deposition in the
restricted marine setting, probably caused by the MECO warming event
(Fig. 11b) (Khanolkar and Saraswati, 2016). A sharp increase in diversity and
abundance of foraminifera is observed at the topmost shale layer within the
Panandhro lignite mine section, which corresponds to the Kirthar transgression
event recorded within the Kutch Basin (Saraswati et al., 2018).</p>
</sec>
<sec id="Ch1.S4.SS3">
  <title>Correlation with global events and stratigraphic implications</title>
      <p id="d1e3580">The Early Eocene sections from Tasmania, Tanzania, Africa and Egypt have
exhibited a tropical mangrove forest domination (Contreras et al., 2014).
Similarly, the Early Eocene sections of the Cambay and Barmer basins in India
also indicate an overall domination of mangrove vegetation
(<italic>Arecaceae, Bombacaceae</italic> groups; refer to Figs. 3, 4, 7 and 8). The
pollen flora belonging to the <italic>Arecaceae</italic> group have also been
discovered in the Arctic–Siberian and Antarctic regions, indicating the
prevalence of tropical to subtropical vegetation belts even at higher
latitudes in the Early Eocene (Suan et al., 2017; Contreras et al., 2013).
The first appearance of the thermophilic <italic>Apectodinium</italic> in the Early
Eocene lignite is observed in the Giral lignite section of the Barmer Basin
(Fig. 3). The percentage of <italic>Apectodinium</italic> in the Giral section
remains low (<inline-formula><mml:math id="M54" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> to 10; Fig. 3). A high abundance of
<italic>Apectodinium</italic> is reported from other low-latitude sections of
Pakistan, the US Gulf Coast and north Africa throughout the Early Eocene,
along with the thermophilic <italic>Kenleyia</italic>, which follows an autotrophic
lifestyle (Harrington, 2001; Crouch et al., 2003). The presence of
<italic>Apectodinium</italic> is common before the PETM from low-latitude sites
(Frieling et al., 2018); however, usually, its first appearance and first
acme are correlated with the PETM. Recent reports from the high-latitude site
of the Otway Basin in Australia, however, suggested that the acme of
<italic>Apectodinium</italic> predates the PETM by <inline-formula><mml:math id="M55" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula>–500 kyr in the basin
(Frieling and Sluijs, 2018). In the Cambay Basin, Clementz et al. (2011)
established the presence of EECO, which may have led to the abundance of
thermophilic <italic>Nypa</italic> and <italic>Kenleyia</italic>. However,
<italic>Apectodinium</italic> is not yet reported from the Cambay Basin, and its
abundance in the Giral section remains low.</p>
      <p id="d1e3638">A gap in sedimentation exists from the late Early Eocene to late Middle
Eocene and is observed across basins in India, Pakistan and Australia,
referred to as the Lutetian gap, and is also recorded in the Kutch Basin
(McGowran et al., 2004; Saraswati et al., 2018; Fig. 2). The mangroves
continued to flourish in the tropics in the Middle Eocene; however, in the
high latitudes, the tropical vegetation which prevailed in the Early Eocene
was replaced by temperate flora, e.g., the growth of temperate
<italic>Nothofagus</italic> trees on Wilkes Island, Antarctica (Contreras et al.,
2013). <italic>Nypa</italic> mangroves from the Middle Eocene of Texas were dominated
by <italic>Spinizonocolpites</italic> genera like those observed in the Matanomadh
and Panandhro lignite sections of the Kutch Basin and thus may have had
similar paleodepositional conditions (Rull, 1998; Westgate and Gee, 1990).
Further, the earliest record of marine snake <italic>Pterosphenus</italic> was
reported from the Middle Eocene of Texas and its morphologically advanced
form, <italic>Pterosphenus</italic> <italic>kutchensis</italic>, which thrived in
mangrove-dominated brackish waters, was recorded from the Panandhro lignite
mine by Rage et al. (2003). The sediments that have been deposited above the
Lutetian gap were recorded in the Panandhro and Matanomadh mine sections of
the Kutch Basin (P12-P13 zone) during the Bartonian transgression caused by
MECO (Khanolkar et al., 2017) and are comprised of lignites, shales and
limestones composed dominantly of dinoflagellates and foraminifera. The
increase in percentage of dinoflagellates can be observed in the Middle
Eocene compared to the Early Eocene sections of western India. The increase
in abundance of planktic foraminifera <italic>Acarinina</italic> is indicative of
warm surface waters and is reported from the MECO warming event of Italy and
towards the top of the Panandhro section (Luciani et al., 2010; Khanolkar et
al., 2017). This sharp increase in the foraminiferal abundance corresponds to
the Kirthar transgression which flooded the sedimentary basins of India and
Pakistan (Nagappa, 1959) and is isochronous to the Wilson Bluff transgression
in Australia (McGowran, 1977, 1979) along the upper part of E11 planktic
foraminiferal zone in the Bartonian.</p>
</sec>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <title>Conclusions</title>
      <p id="d1e3670">The Early and Middle Eocene palynomorph assemblages from lignite mines in
western India represent an overall tropical vegetation pattern; however, our
current study further pointed out the following similarities and differences
in terms of paleovegetation and paleodepositional conditions (Table 1).
During the Early Eocene, angiosperms like <italic>Arengapollenites achinatus, Longapertites retipilatus</italic> and  <italic>Longapertites</italic> sp. constituted the rainforest
elements and along with mangrove vegetation gave rise to the thick lignite
deposits in the marginal marine setting of the Cambay and Barmer basins. An
increase in abundance and diversity of <italic>Nypa</italic> species
(<italic>Acanthotricolpites robustus</italic>, <italic>A. bulbospinosus, A. brevispinosus, A. tiruchirapalliensis, Arengapollenites achinatus, Spinizonocolpites baculatus</italic>, <italic>S. bulbospinosus, S. echinatus, S. adamanteus, S. prominatus, Spinomonosulcites echinatus</italic>) characterized the
Early Eocene lignites. The<?pagebreak page21?> percentage and diversity of dinoflagellates was
low in both sections, indicating low depth. The first occurrence of the
thermophilic dinoflagellates <italic>Apectodinium homomorphum</italic> and
<italic>Kenleyia</italic> sp. within the carbonaceous shales of the Barmer Basin
indicates the prevalence of hot climate across the Early Eocene. In the
Cambay Basin, the presence of dinoflagellates <italic>Achomosphaera</italic> sp. and
<italic>Cordosphaeridium</italic> sp. was recorded within the shales and is also
indicative of high temperatures. The lignites of the Early Eocene were deposited
in hot and humid marginal marine conditions. The Middle Eocene vegetation was
characterized by rainforest elements (<italic>Longapertites retipilatus, Palmaepollenites ovatus, Lakiapollis ovatus, Tribrevicolporites</italic> sp.,
<italic>Meliapollis ramanujamii, Dipterocarpuspollenites retipilatus, Paleosantalaceaepites distinctus</italic>), along with mangrove elements
(<italic>Spinizonocolpites echinatus</italic>, <italic>S. bulbospinosus, Acanthotricolpites kutchensis, Albertipollenites crassireticulatus</italic>) which
gave rise to significant organic detritus to form the lignite deposits in the
Kutch Basin. The abundance and diversity of <italic>Nypa</italic> had been reduced, while
those of dinoflagellates increased significantly compared to Early Eocene
lignites. The characteristics of foraminiferal assemblage recorded from the
Kutch mine sections including bloom in triserial planktics and RBFs, low
diversity and the presence of atypical planktic foraminifera are indicative of
eutrophic and stressed conditions of deposition. However, there was a drastic
increment in percentage and diversity of foraminifera observed at the
uppermost portion of the Panandhro mine section which exhibited a change in trophic
regime from eutrophic to oligotrophic and deposition in open marine
conditions. This rise in sea level, which can be correlated with the Kirthar–Wilson
Bluff transgression, may have been linked with the MECO hyperthermal event
in the Bartonian.</p>
</sec>

      
      </body>
    <back><notes notes-type="dataavailability">

      <p id="d1e3724">The data is provided in Sect. 2 of the Supplement;
the micropaleontological slides comprising the foraminifera are
in the microscopy lab, Department of Earth Sciences, Indian Institute of
Technology Kanpur; the palynomorph slides are housed in the Department
of Geology, K. J. Somaiya College of Science and Commerce, University of
Mumbai.</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e3727">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/jm-38-1-2019-supplement" xlink:title="zip">https://doi.org/10.5194/jm-38-1-2019-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution">

      <p id="d1e3736">SK wrote the manuscript and carried out foraminiferal
analysis. JS carried out palynomorph analysis.</p>
  </notes><notes notes-type="competinginterests">

      <p id="d1e3742">The authors declare that they have no conflict of
interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e3748">Sonal Khanolkar and Jyoti Sharma thank the Department of Science and
Technology, India (project nos. DST/INSPIRE/04/2016/002525 and DST-WOSA
PSR/WOS A/ES_31/2011) for providing the funding for carrying out this
research work. Jyoti Sharma and Sonal Khanolkar are grateful to the Indian
Institute of Technology Bombay and Indian Institute of Technology Kanpur for
providing the facilities to carry out this work. We are thankful to the two
anonymous reviewers and the handling editor Francesca Sangiorgi for the
constructive comments which helped us improve the manuscript. We would like
to dedicate this paper to Pratul Kumar Saraswati , IIT Bombay, who has been a
motivation for our work and has played an important role in revising the
Paleogene biostratigraphy of western India. Sonal Khanolkar would like to
thank Manudeo Singh for help with the preparation of figures.<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?> Edited by: Francesca Sangiorgi<?xmltex \hack{\newline}?> Reviewed by:
two anonymous referees</p></ack><ref-list>
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<abstract-html><p>Various Eocene hyperthermal events have been recorded from lignite sections
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Bloom of triserial planktic (<i>Jenkinsina columbiana</i>) and rectilinear
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Lutetian–Early Bartonian in the lignite sections of the Kutch Basin which later changed
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mines of the Kutch Basin which may be correlated with the Kirthar–Wilson Bluff
transgression event in the Bartonian observed across  basins in India, Pakistan and
Australia potentially linked to sea level rise around the Middle
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