<?xml version="1.0"?>
<!DOCTYPE article
PUBLIC "-//NLM//DTD JATS (Z39.96) Journal Publishing DTD v1.4 20190208//EN"
       "JATS-journalpublishing1.dtd">
<article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" article-type="research-article" dtd-version="1.4" xml:lang="en">
 <front>
  <journal-meta>
   <journal-id journal-id-type="publisher-id">Russian Journal of Earth Sciences</journal-id>
   <journal-title-group>
    <journal-title xml:lang="en">Russian Journal of Earth Sciences</journal-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Russian Journal of Earth Sciences</trans-title>
    </trans-title-group>
   </journal-title-group>
   <issn publication-format="online">1681-1208</issn>
  </journal-meta>
  <article-meta>
   <article-id pub-id-type="publisher-id">46990</article-id>
   <article-categories>
    <subj-group subj-group-type="toc-heading" xml:lang="ru">
     <subject>ОРИГИНАЛЬНЫЕ СТАТЬИ</subject>
    </subj-group>
    <subj-group subj-group-type="toc-heading" xml:lang="en">
     <subject>ORIGINAL ARTICLES</subject>
    </subj-group>
    <subj-group>
     <subject>ОРИГИНАЛЬНЫЕ СТАТЬИ</subject>
    </subj-group>
   </article-categories>
   <title-group>
    <article-title xml:lang="en">Magnetolithologic and Magnetomineralogical Characteristics of Deposits at the Mesozoic/Cenozoic Boundary: Gams Section Austria</article-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Magnetolithologic and Magnetomineralogical Characteristics of Deposits at the Mesozoic/Cenozoic Boundary: Gams Section Austria</trans-title>
    </trans-title-group>
   </title-group>
   <contrib-group content-type="authors">
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Pechersky</surname>
       <given-names>D M</given-names>
      </name>
      <name xml:lang="en">
       <surname>Pechersky</surname>
       <given-names>D M</given-names>
      </name>
     </name-alternatives>
     <xref ref-type="aff" rid="aff-1"/>
    </contrib>
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Grachev</surname>
       <given-names>A F</given-names>
      </name>
      <name xml:lang="en">
       <surname>Grachev</surname>
       <given-names>A F</given-names>
      </name>
     </name-alternatives>
     <xref ref-type="aff" rid="aff-2"/>
    </contrib>
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Nourgaliev</surname>
       <given-names>D K</given-names>
      </name>
      <name xml:lang="en">
       <surname>Nourgaliev</surname>
       <given-names>D K</given-names>
      </name>
     </name-alternatives>
     <xref ref-type="aff" rid="aff-3"/>
    </contrib>
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Tsel'movich</surname>
       <given-names>V A</given-names>
      </name>
      <name xml:lang="en">
       <surname>Tsel'movich</surname>
       <given-names>V A</given-names>
      </name>
     </name-alternatives>
     <xref ref-type="aff" rid="aff-4"/>
    </contrib>
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Sharonova</surname>
       <given-names>Z V</given-names>
      </name>
      <name xml:lang="en">
       <surname>Sharonova</surname>
       <given-names>Z V</given-names>
      </name>
     </name-alternatives>
     <xref ref-type="aff" rid="aff-5"/>
    </contrib>
   </contrib-group>
   <aff-alternatives id="aff-1">
    <aff>
     <institution xml:lang="ru">Institute of Physics of the Earth, Russian Academy of Sciences, Moscow, Russia</institution>
     <country>ru</country>
    </aff>
    <aff>
     <institution xml:lang="en">Institute of Physics of the Earth, Russian Academy of Sciences, Moscow, Russia</institution>
     <country>ru</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-2">
    <aff>
     <institution xml:lang="ru">Institute of Physics of the Earth, Russian Academy of Sciences, Moscow, Russia</institution>
     <country>ru</country>
    </aff>
    <aff>
     <institution xml:lang="en">Institute of Physics of the Earth, Russian Academy of Sciences, Moscow, Russia</institution>
     <country>ru</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-3">
    <aff>
     <institution xml:lang="ru">Kazan State University, Kazan, Russia</institution>
     <country>ru</country>
    </aff>
    <aff>
     <institution xml:lang="en">Kazan State University, Kazan, Russia</institution>
     <country>ru</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-4">
    <aff>
     <institution xml:lang="ru">Institute of Physics of the Earth, Russian Academy of Sciences, Moscow, Russia</institution>
     <country>ru</country>
    </aff>
    <aff>
     <institution xml:lang="en">Institute of Physics of the Earth, Russian Academy of Sciences, Moscow, Russia</institution>
     <country>ru</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-5">
    <aff>
     <institution xml:lang="ru">Institute of Physics of the Earth, Russian Academy of Sciences, Moscow, Russia</institution>
     <country>ru</country>
    </aff>
    <aff>
     <institution xml:lang="en">Institute of Physics of the Earth, Russian Academy of Sciences, Moscow, Russia</institution>
     <country>ru</country>
    </aff>
   </aff-alternatives>
   <volume>8</volume>
   <issue>3</issue>
   <fpage>1</fpage>
   <lpage>23</lpage>
   <history>
    <date date-type="received" iso-8601-date="2021-11-10T19:21:09+03:00">
     <day>10</day>
     <month>11</month>
     <year>2021</year>
    </date>
   </history>
   <self-uri xlink:href="https://rjes.ru/en/nauka/article/46990/view">https://rjes.ru/en/nauka/article/46990/view</self-uri>
   <abstract xml:lang="ru">
    <p>This paper continues a series of detailed magnetolithologic and magnetomineralogical investigations of epicontinental deposits at the Mesozoic/Cenozoic K/T boundary and is devoted to the study of a small segment of the Gams section Austria including the K/T. Thermomagnetic analysis revealed several magnetic phases; according to the curve MT, these are goethite nbsp;T C = 90-150o C, hemoilmenite nbsp;T C = 200-300o C, metallic nickel nbsp;T C = 350-360o C, magnetite and titanomagnetite nbsp;T C = 550-610o C, a Fe-Ni alloy nbsp;T C = 640-660o C, and metallic iron nbsp;T C = 740-770o C. Ensembles of magnetic grains has similar coercivity spectra in all samples and are characterized by a high coercivity. Against this background, the transition layer J with a maximum at 25-40nbsp;mT is identified, which is related to grains of metallic nickel and the Fe-Ni alloy. Numerous small single-domain and superparamagnetic grains of magnetic minerals present throughout the rock sequence contribute appreciably to the magnetic susceptibility of the rocks. With rare exceptions, the study deposits are anisotropic and have a mostly oblate magnetic fabric foliation, indicating a terrigenous origin of the magnetic minerals. Many samples of sandy-clayey sediments have inverse magnetic fabric. This is primarily related to the inverse magnetic fabric of needle goethite that is present among the iron hydroxides. Relative contributions of paramagnetic iron hydroxides, clays, and so on and diamagnetic carbonates and quartz components in the sediments are estimated from M s values near 800o C, where the contribution of magnetic minerals is absent. Results of these studies imply that the K/T boundary is distinguished by a sharp rise in the concentrations of iron hydroxides and paramagnetic Fe-bearing minerals it is at the K/T boundary, in the transition layer J, a sharp rise in the concentrations of magnetite and hemoilmenite occurs 4nbsp;cm above the K/T boundary. Lithologic control has no influence on the concentration of titanomagnetite, thereby reflecting the titanomagnetite dispersal at the time of eruptive activity that was most pronounced in the Maestrichtian. Metallic iron is distributed along the section rather uniformly, implying that it is most likely meteoritic dust. The occurrence of metallic nickel in the deposits is a unique phenomenon.</p>
   </abstract>
   <trans-abstract xml:lang="en">
    <p>This paper continues a series of detailed magnetolithologic and magnetomineralogical investigations of epicontinental deposits at the Mesozoic/Cenozoic K/T boundary and is devoted to the study of a small segment of the Gams section Austria including the K/T. Thermomagnetic analysis revealed several magnetic phases; according to the curve MT, these are goethite nbsp;T C = 90-150o C, hemoilmenite nbsp;T C = 200-300o C, metallic nickel nbsp;T C = 350-360o C, magnetite and titanomagnetite nbsp;T C = 550-610o C, a Fe-Ni alloy nbsp;T C = 640-660o C, and metallic iron nbsp;T C = 740-770o C. Ensembles of magnetic grains has similar coercivity spectra in all samples and are characterized by a high coercivity. Against this background, the transition layer J with a maximum at 25-40nbsp;mT is identified, which is related to grains of metallic nickel and the Fe-Ni alloy. Numerous small single-domain and superparamagnetic grains of magnetic minerals present throughout the rock sequence contribute appreciably to the magnetic susceptibility of the rocks. With rare exceptions, the study deposits are anisotropic and have a mostly oblate magnetic fabric foliation, indicating a terrigenous origin of the magnetic minerals. Many samples of sandy-clayey sediments have inverse magnetic fabric. This is primarily related to the inverse magnetic fabric of needle goethite that is present among the iron hydroxides. Relative contributions of paramagnetic iron hydroxides, clays, and so on and diamagnetic carbonates and quartz components in the sediments are estimated from M s values near 800o C, where the contribution of magnetic minerals is absent. Results of these studies imply that the K/T boundary is distinguished by a sharp rise in the concentrations of iron hydroxides and paramagnetic Fe-bearing minerals it is at the K/T boundary, in the transition layer J, a sharp rise in the concentrations of magnetite and hemoilmenite occurs 4nbsp;cm above the K/T boundary. Lithologic control has no influence on the concentration of titanomagnetite, thereby reflecting the titanomagnetite dispersal at the time of eruptive activity that was most pronounced in the Maestrichtian. Metallic iron is distributed along the section rather uniformly, implying that it is most likely meteoritic dust. The occurrence of metallic nickel in the deposits is a unique phenomenon.</p>
   </trans-abstract>
   <kwd-group xml:lang="ru">
    <kwd>Mesozoic/Cenozoic K/T boundary</kwd>
    <kwd>magnetomineralogy</kwd>
    <kwd>lithology</kwd>
    <kwd>magnetic minerals</kwd>
    <kwd>petromagnetology.</kwd>
   </kwd-group>
   <kwd-group xml:lang="en">
    <kwd>Mesozoic/Cenozoic K/T boundary</kwd>
    <kwd>magnetomineralogy</kwd>
    <kwd>lithology</kwd>
    <kwd>magnetic minerals</kwd>
    <kwd>petromagnetology.</kwd>
   </kwd-group>
  </article-meta>
 </front>
 <body>
  <p></p>
 </body>
 <back>
  <ref-list>
   <ref id="B1">
    <label>1.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Adamia, Geologica Carpatica, v. 23, no. 3, 1993.</mixed-citation>
     <mixed-citation xml:lang="en">Adamia, Geologica Carpatica, v. 23, no. 3, 1993.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B2">
    <label>2.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Alvarez, Science, v. 250, 1990.</mixed-citation>
     <mixed-citation xml:lang="en">Alvarez, Science, v. 250, 1990.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B3">
    <label>3.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Bagin, Magnetism of #x3B1;-Oxides and Hydroxides of Iron, 1988.</mixed-citation>
     <mixed-citation xml:lang="en">Bagin, Magnetism of #x3B1;-Oxides and Hydroxides of Iron, 1988.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B4">
    <label>4.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Bagin, Izv. Acad. Sci. USSR Phys. Solid Earth, v. 12, no. 9, 1976.</mixed-citation>
     <mixed-citation xml:lang="en">Bagin, Izv. Acad. Sci. USSR Phys. Solid Earth, v. 12, no. 9, 1976.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B5">
    <label>5.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Bagin, Izv. Acad. Sci. USSR Phys. Solid Earth, v. 13, no. 2, 1977.</mixed-citation>
     <mixed-citation xml:lang="en">Bagin, Izv. Acad. Sci. USSR Phys. Solid Earth, v. 13, no. 2, 1977.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B6">
    <label>6.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Baulus, Earth Planet. Sci. Lett., v. 182, 2000., doi: 10.1016/S0012-821X0000245-4</mixed-citation>
     <mixed-citation xml:lang="en">Baulus, Earth Planet. Sci. Lett., v. 182, 2000., doi: 10.1016/S0012-821X0000245-4</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B7">
    <label>7.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Burov, Paleomagnetic Analysis, 1986.</mixed-citation>
     <mixed-citation xml:lang="en">Burov, Paleomagnetic Analysis, 1986.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B8">
    <label>8.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Day, Phys. Earth Planet. Inter., v. 13, 1977., doi: 10.1016/0031-92017790108-X</mixed-citation>
     <mixed-citation xml:lang="en">Day, Phys. Earth Planet. Inter., v. 13, 1977., doi: 10.1016/0031-92017790108-X</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B9">
    <label>9.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Dunlop, J. Geophys. Res., v. 107, no. B3, 2002., doi: 10.1029/2001JB000486</mixed-citation>
     <mixed-citation xml:lang="en">Dunlop, J. Geophys. Res., v. 107, no. B3, 2002., doi: 10.1029/2001JB000486</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B10">
    <label>10.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Dunlop, J. Geophys. Res., v. 107, no. B3, 2002., doi: 10.1029/2001JB000487</mixed-citation>
     <mixed-citation xml:lang="en">Dunlop, J. Geophys. Res., v. 107, no. B3, 2002., doi: 10.1029/2001JB000487</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B11">
    <label>11.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Egli, J. Geophys. Res., v. 108, no. B2, 2003., doi: 10.1029/2002JB002023</mixed-citation>
     <mixed-citation xml:lang="en">Egli, J. Geophys. Res., v. 108, no. B2, 2003., doi: 10.1029/2002JB002023</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B12">
    <label>12.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Ellwood, Earth Planet. Sci. Lett., v. 206, 2003., doi: 10.1016/S0012-821X0201124-X</mixed-citation>
     <mixed-citation xml:lang="en">Ellwood, Earth Planet. Sci. Lett., v. 206, 2003., doi: 10.1016/S0012-821X0201124-X</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B13">
    <label>13.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Ernst, Annu. Rev. Earth Planet. Sci., v. 31, 2003., doi: 10.1146/annurev.earth.31.100901.145500</mixed-citation>
     <mixed-citation xml:lang="en">Ernst, Annu. Rev. Earth Planet. Sci., v. 31, 2003., doi: 10.1146/annurev.earth.31.100901.145500</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B14">
    <label>14.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Gapeev, Izv. Acad. Sci. USSR Phys. Solid Earth, v. 24, no. 10, 1988.</mixed-citation>
     <mixed-citation xml:lang="en">Gapeev, Izv. Acad. Sci. USSR Phys. Solid Earth, v. 24, no. 10, 1988.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B15">
    <label>15.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Grachev, Izv. Phys. Solid Earth, v. 36, 2000.</mixed-citation>
     <mixed-citation xml:lang="en">Grachev, Izv. Phys. Solid Earth, v. 36, 2000.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B16">
    <label>16.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Grachev, Russian J. Earth Sci., v. 7, 2005., doi: 10.2205/2005ES000189</mixed-citation>
     <mixed-citation xml:lang="en">Grachev, Russian J. Earth Sci., v. 7, 2005., doi: 10.2205/2005ES000189</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B17">
    <label>17.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Lahodynsky, Riv. Espanola de Paleontologia, no. extraordinario, 1988.</mixed-citation>
     <mixed-citation xml:lang="en">Lahodynsky, Riv. Espanola de Paleontologia, no. extraordinario, 1988.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B18">
    <label>18.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Montanari, Planet. Space Sci., v. 46, 1998., doi: 10.1016/S0032-06339700130-X</mixed-citation>
     <mixed-citation xml:lang="en">Montanari, Planet. Space Sci., v. 46, 1998., doi: 10.1016/S0032-06339700130-X</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B19">
    <label>19.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Morner, 27 IGC Session, Abstracts, vol. 9, 1984.</mixed-citation>
     <mixed-citation xml:lang="en">Morner, 27 IGC Session, Abstracts, vol. 9, 1984.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B20">
    <label>20.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Nagata, Rock-Magnetism, 1961.</mixed-citation>
     <mixed-citation xml:lang="en">Nagata, Rock-Magnetism, 1961.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B21">
    <label>21.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Nazarov, Byull. MOIP, Otd. Geol., v. 68, no. 3, 1993.</mixed-citation>
     <mixed-citation xml:lang="en">Nazarov, Byull. MOIP, Otd. Geol., v. 68, no. 3, 1993.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B22">
    <label>22.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Pechersky, Russian J. Earth Sci., v. 7, no. 2, 2005.</mixed-citation>
     <mixed-citation xml:lang="en">Pechersky, Russian J. Earth Sci., v. 7, no. 2, 2005.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B23">
    <label>23.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Pechersky, Izv. Phys. Solid Earth, v. 42, no. 10, 2006.</mixed-citation>
     <mixed-citation xml:lang="en">Pechersky, Izv. Phys. Solid Earth, v. 42, no. 10, 2006.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B24">
    <label>24.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Richter, Phys. Earth Planet. Int., v. 82, 1994.</mixed-citation>
     <mixed-citation xml:lang="en">Richter, Phys. Earth Planet. Int., v. 82, 1994.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B25">
    <label>25.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Robertson, Phys. Earth Planet. Inter., v. 82, 1994., doi: 10.1016/0031-92019490074-4</mixed-citation>
     <mixed-citation xml:lang="en">Robertson, Phys. Earth Planet. Inter., v. 82, 1994., doi: 10.1016/0031-92019490074-4</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B26">
    <label>26.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Rocchia, Earth Planet. Sci. Lett., v. 99, 1990., doi: 10.1016/0012-821X9090111-A</mixed-citation>
     <mixed-citation xml:lang="en">Rocchia, Earth Planet. Sci. Lett., v. 99, 1990., doi: 10.1016/0012-821X9090111-A</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B27">
    <label>27.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Rochette, Rev. Geophys., v. 30, 1992.</mixed-citation>
     <mixed-citation xml:lang="en">Rochette, Rev. Geophys., v. 30, 1992.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B28">
    <label>28.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Sholpo, Rock Magnetism Applications to Geological Problems, 1977.</mixed-citation>
     <mixed-citation xml:lang="en">Sholpo, Rock Magnetism Applications to Geological Problems, 1977.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B29">
    <label>29.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Veimarn, Global Catastrophic Events and Their Implications for Stratigraphic Correlations of Sedimentary Basins of Various Types, 1998.</mixed-citation>
     <mixed-citation xml:lang="en">Veimarn, Global Catastrophic Events and Their Implications for Stratigraphic Correlations of Sedimentary Basins of Various Types, 1998.</mixed-citation>
    </citation-alternatives>
   </ref>
   <ref id="B30">
    <label>30.</label>
    <citation-alternatives>
     <mixed-citation xml:lang="ru">Yasonov, Geologica Carpathica, v. 49, no. 3, 1998.</mixed-citation>
     <mixed-citation xml:lang="en">Yasonov, Geologica Carpathica, v. 49, no. 3, 1998.</mixed-citation>
    </citation-alternatives>
   </ref>
  </ref-list>
 </back>
</article>
