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 <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">57174</article-id>
   <article-id pub-id-type="doi">10.2205/2023ES000871</article-id>
   <article-id pub-id-type="edn">ctviqu</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">Theoretical and Experimental Modeling of Local Scale CO2 Flushing of Hydrous Rhyolitic Magma</article-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Theoretical and Experimental Modeling of Local Scale CO2 Flushing of Hydrous Rhyolitic Magma</trans-title>
    </trans-title-group>
   </title-group>
   <contrib-group content-type="authors">
    <contrib contrib-type="author">
     <contrib-id contrib-id-type="orcid">https://orcid.org/0000-0002-6498-7188</contrib-id>
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Симакин</surname>
       <given-names>Александр Геннадьевич</given-names>
      </name>
      <name xml:lang="en">
       <surname>Simakin</surname>
       <given-names>Alexander Gennadievich</given-names>
      </name>
     </name-alternatives>
     <email>simakin@ifz.ru</email>
     <bio xml:lang="ru">
      <p>доктор физико-математических наук;</p>
     </bio>
     <bio xml:lang="en">
      <p>doctor of physical and mathematical sciences;</p>
     </bio>
     <xref ref-type="aff" rid="aff-1"/>
    </contrib>
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Девятова</surname>
       <given-names>Вера Николаевна</given-names>
      </name>
      <name xml:lang="en">
       <surname>Devyatova</surname>
       <given-names>Vera Nikolaevna</given-names>
      </name>
     </name-alternatives>
     <xref ref-type="aff" rid="aff-2"/>
    </contrib>
    <contrib contrib-type="author">
     <contrib-id contrib-id-type="orcid">https://orcid.org/0000-0002-2467-825X</contrib-id>
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Ширяев</surname>
       <given-names>Андрей Альбертович</given-names>
      </name>
      <name xml:lang="en">
       <surname>Shiryaev</surname>
       <given-names>Andrey Albertovich</given-names>
      </name>
     </name-alternatives>
     <xref ref-type="aff" rid="aff-3"/>
    </contrib>
   </contrib-group>
   <aff-alternatives id="aff-1">
    <aff>
     <institution xml:lang="ru">Институт Экспериментальной Минералогии, РАН</institution>
     <city>Черноголовка</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Institute of Experimental Mineralogy, RAS</institution>
     <city>Chernogolovka</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-2">
    <aff>
     <institution xml:lang="ru">Институт Экспериментальной Минералогии, РАН</institution>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Institute of Experimental Mineralogy, RAS</institution>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-3">
    <aff>
     <institution xml:lang="ru">Институт физической химии и электрохимии им. А.Н. Фрумкина РАН</institution>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Institute of Physical Chemistry and Electrochemistry named after. A.N. Frumkin RAS</institution>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <pub-date publication-format="print" date-type="pub" iso-8601-date="2023-12-30T00:00:00+03:00">
    <day>30</day>
    <month>12</month>
    <year>2023</year>
   </pub-date>
   <pub-date publication-format="electronic" date-type="pub" iso-8601-date="2023-12-30T00:00:00+03:00">
    <day>30</day>
    <month>12</month>
    <year>2023</year>
   </pub-date>
   <volume>23</volume>
   <issue>6</issue>
   <fpage>1</fpage>
   <lpage>24</lpage>
   <history>
    <date date-type="received" iso-8601-date="2024-03-23T00:00:00+03:00">
     <day>23</day>
     <month>03</month>
     <year>2024</year>
    </date>
    <date date-type="accepted" iso-8601-date="2023-09-21T00:00:00+03:00">
     <day>21</day>
     <month>09</month>
     <year>2023</year>
    </date>
   </history>
   <self-uri xlink:href="https://rjes.ru/en/nauka/article/57174/view">https://rjes.ru/en/nauka/article/57174/view</self-uri>
   <abstract xml:lang="ru">
    <p>Flushing of hydrous silicic magmas with crustal carbonic fluid may be an important factor controlling the dynamics of rhyolitic eruptions. We present combined theoretical and experimental study of the interaction of carbonic fluid with a hydrous silicic melt. The process of diffusional equilibration of a CO2 bubble with a silicic melt was simulated numerically in the spherical shell approximation. The rapid water transfer from the melt to the bubble is followed by a slower diffusion of CO2 into the melt. The water distribution in the melt becomes almost uniform over a period proportional to the diffusional unit of time 0.14τw, determined by the initial inter-bubble distance W equal the distance between neighbor bubbles centers and the water diffusion coefficient Dw in the melt (τw = W 2/Dw), while the CO2 distribution remains strongly contrasting and the melt remains undersaturated in CO2. This process was modelled experimentally with a hydrous albite melt at P = 200MPa and T = 950–1000 °C. In the first series of experiments at T = 950◦C, a glass powder was filled with pure CO2 at the beginning of the experiment, forming numerous bubbles at the run temperature. Micro-FTIR measurements showed that after 40 minutes the water content in the melt decreased from 4.9 down to 1.8 wt. % with the maximum CO2 content of 500 ppm (below saturation). After 4 hours, the crystallinity increased to 85%, and almost all of the fluid bubbles escaped. The second series of experiments CO2 interacted with a 2 mm high column of hydrous albite melt. Diffusion profiles in the quenched glass were measured using EMPA (H2O) and micro-FTIR (CO2 and H2O). The estimated diffusion coefficients in the melt for H2O (1.1 × 10−6 cm2 /s) and CO2 (1.5 × 10−7 cm2 /s) are consistent with published data. Scaling analysis predicts that in the nature, after the influx of CO2 bubbles a few millimeters in size, the maximum dehydration of rhyolitic magma with viscosity near 105 Pa s without a significant increase in CO2 content occurs after 1–30 days, i.e. a period compatible with the minimum duration of pre-eruption processes in the magma chamber.</p>
   </abstract>
   <trans-abstract xml:lang="en">
    <p>Flushing of hydrous silicic magmas with crustal carbonic fluid may be an important factor controlling the dynamics of rhyolitic eruptions. We present combined theoretical and experimental study of the interaction of carbonic fluid with a hydrous silicic melt. The process of diffusional equilibration of a CO2 bubble with a silicic melt was simulated numerically in the spherical shell approximation. The rapid water transfer from the melt to the bubble is followed by a slower diffusion of CO2 into the melt. The water distribution in the melt becomes almost uniform over a period proportional to the diffusional unit of time 0.14τw, determined by the initial inter-bubble distance W equal the distance between neighbor bubbles centers and the water diffusion coefficient Dw in the melt (τw = W 2/Dw), while the CO2 distribution remains strongly contrasting and the melt remains undersaturated in CO2. This process was modelled experimentally with a hydrous albite melt at P = 200MPa and T = 950–1000 °C. In the first series of experiments at T = 950◦C, a glass powder was filled with pure CO2 at the beginning of the experiment, forming numerous bubbles at the run temperature. Micro-FTIR measurements showed that after 40 minutes the water content in the melt decreased from 4.9 down to 1.8 wt. % with the maximum CO2 content of 500 ppm (below saturation). After 4 hours, the crystallinity increased to 85%, and almost all of the fluid bubbles escaped. The second series of experiments CO2 interacted with a 2 mm high column of hydrous albite melt. Diffusion profiles in the quenched glass were measured using EMPA (H2O) and micro-FTIR (CO2 and H2O). The estimated diffusion coefficients in the melt for H2O (1.1 × 10−6 cm2 /s) and CO2 (1.5 × 10−7 cm2 /s) are consistent with published data. Scaling analysis predicts that in the nature, after the influx of CO2 bubbles a few millimeters in size, the maximum dehydration of rhyolitic magma with viscosity near 105 Pa s without a significant increase in CO2 content occurs after 1–30 days, i.e. a period compatible with the minimum duration of pre-eruption processes in the magma chamber.</p>
   </trans-abstract>
   <kwd-group xml:lang="ru">
    <kwd>Carbon dioxide</kwd>
    <kwd>explosive volcanic eruption</kwd>
    <kwd>experiment in IHPV</kwd>
    <kwd>diffusion of CO2 and H2O</kwd>
    <kwd>magma flushing with CO2</kwd>
   </kwd-group>
   <kwd-group xml:lang="en">
    <kwd>Carbon dioxide</kwd>
    <kwd>explosive volcanic eruption</kwd>
    <kwd>experiment in IHPV</kwd>
    <kwd>diffusion of CO2 and H2O</kwd>
    <kwd>magma flushing with CO2</kwd>
   </kwd-group>
   <funding-group>
    <funding-statement xml:lang="ru">Authors thank for invaluable contribution of A.N. Nekrasov in EMPA analyses of our experimental samples and G. V. Bondarenko for assistance in the Raman investigation of the bubbles. The authors are also grateful to R. E. Botcharnikov and anonymous reviewer for critical comments that clarify the presentation of the results and significantly improve the MS</funding-statement>
    <funding-statement xml:lang="en">Authors thank for invaluable contribution of A.N. Nekrasov in EMPA analyses of our experimental samples and G. V. Bondarenko for assistance in the Raman investigation of the bubbles. The authors are also grateful to R. E. Botcharnikov and anonymous reviewer for critical comments that clarify the presentation of the results and significantly improve the MS</funding-statement>
   </funding-group>
  </article-meta>
 </front>
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