<?xml version="1.0" encoding="UTF-8"?>
<collection xmlns="http://www.loc.gov/MARC21/slim">
 <record>
  <leader>     caa a22        4500</leader>
  <controlfield tag="001">445815981</controlfield>
  <controlfield tag="003">CHVBK</controlfield>
  <controlfield tag="005">20180317145228.0</controlfield>
  <controlfield tag="007">cr unu---uuuuu</controlfield>
  <controlfield tag="008">170323e20110701xx      s     000 0 eng  </controlfield>
  <datafield tag="024" ind1="7" ind2="0">
   <subfield code="a">10.1007/s11214-010-9737-9</subfield>
   <subfield code="2">doi</subfield>
  </datafield>
  <datafield tag="035" ind1=" " ind2=" ">
   <subfield code="a">(NATIONALLICENCE)springer-10.1007/s11214-010-9737-9</subfield>
  </datafield>
  <datafield tag="245" ind1="0" ind2="0">
   <subfield code="a">MHD Waves and Instabilities in Space Plasma Flows</subfield>
   <subfield code="h">[Elektronische Daten]</subfield>
   <subfield code="c">[Y. Taroyan, M. Ruderman]</subfield>
  </datafield>
  <datafield tag="520" ind1="3" ind2=" ">
   <subfield code="a">Shear flow instabilities are an important aspect of hydrodynamic studies. The present review article discusses the role of an ambient magnetic field which both modifies the Kelvin-Helmholtz instability and may introduce new types of magnetohydrodynamic waves and instabilities. A brief overview of magnetospheric pulsations is presented with an emphasis on the long-period resonant Alfvén waves associated with the high speed solar wind. The spatio-temporal evolution of magnetically modified shear flow instabilities in various space plasma structures is addressed. A distinction between convective and absolute instabilities is necessary for proper understanding of theory and correct interpretation of the observations. Finally, it is shown how incompressible Alfvénic disturbances may become unstable in a compressible flow in the absence of any shear. An application to coronal loops is presented.</subfield>
  </datafield>
  <datafield tag="540" ind1=" " ind2=" ">
   <subfield code="a">Springer Science+Business Media B.V., 2011</subfield>
  </datafield>
  <datafield tag="690" ind1=" " ind2="7">
   <subfield code="a">Space plasmas</subfield>
   <subfield code="2">nationallicence</subfield>
  </datafield>
  <datafield tag="690" ind1=" " ind2="7">
   <subfield code="a">MHD waves</subfield>
   <subfield code="2">nationallicence</subfield>
  </datafield>
  <datafield tag="690" ind1=" " ind2="7">
   <subfield code="a">Shear flow instabilities</subfield>
   <subfield code="2">nationallicence</subfield>
  </datafield>
  <datafield tag="690" ind1=" " ind2="7">
   <subfield code="a">Convective and absolute instabilities</subfield>
   <subfield code="2">nationallicence</subfield>
  </datafield>
  <datafield tag="690" ind1=" " ind2="7">
   <subfield code="a">Compressible flows</subfield>
   <subfield code="2">nationallicence</subfield>
  </datafield>
  <datafield tag="700" ind1="1" ind2=" ">
   <subfield code="a">Taroyan</subfield>
   <subfield code="D">Y.</subfield>
   <subfield code="u">Solar Physics &amp; Space Plasma Research Centre (SP²RC), Department of Applied Mathematics, University of Sheffield, S3 7RH, Sheffield, UK</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="700" ind1="1" ind2=" ">
   <subfield code="a">Ruderman</subfield>
   <subfield code="D">M.</subfield>
   <subfield code="u">Solar Physics &amp; Space Plasma Research Centre (SP²RC), Department of Applied Mathematics, University of Sheffield, S3 7RH, Sheffield, UK</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="773" ind1="0" ind2=" ">
   <subfield code="t">Space Science Reviews</subfield>
   <subfield code="d">Springer Netherlands</subfield>
   <subfield code="g">158/2-4(2011-07-01), 505-523</subfield>
   <subfield code="x">0038-6308</subfield>
   <subfield code="q">158:2-4&lt;505</subfield>
   <subfield code="1">2011</subfield>
   <subfield code="2">158</subfield>
   <subfield code="o">11214</subfield>
  </datafield>
  <datafield tag="856" ind1="4" ind2="0">
   <subfield code="u">https://doi.org/10.1007/s11214-010-9737-9</subfield>
   <subfield code="q">text/html</subfield>
   <subfield code="z">Onlinezugriff via DOI</subfield>
  </datafield>
  <datafield tag="908" ind1=" " ind2=" ">
   <subfield code="D">1</subfield>
   <subfield code="a">research-article</subfield>
   <subfield code="2">jats</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">856</subfield>
   <subfield code="E">40</subfield>
   <subfield code="u">https://doi.org/10.1007/s11214-010-9737-9</subfield>
   <subfield code="q">text/html</subfield>
   <subfield code="z">Onlinezugriff via DOI</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">700</subfield>
   <subfield code="E">1-</subfield>
   <subfield code="a">Taroyan</subfield>
   <subfield code="D">Y.</subfield>
   <subfield code="u">Solar Physics &amp; Space Plasma Research Centre (SP²RC), Department of Applied Mathematics, University of Sheffield, S3 7RH, Sheffield, UK</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">700</subfield>
   <subfield code="E">1-</subfield>
   <subfield code="a">Ruderman</subfield>
   <subfield code="D">M.</subfield>
   <subfield code="u">Solar Physics &amp; Space Plasma Research Centre (SP²RC), Department of Applied Mathematics, University of Sheffield, S3 7RH, Sheffield, UK</subfield>
   <subfield code="4">aut</subfield>
  </datafield>
  <datafield tag="950" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="P">773</subfield>
   <subfield code="E">0-</subfield>
   <subfield code="t">Space Science Reviews</subfield>
   <subfield code="d">Springer Netherlands</subfield>
   <subfield code="g">158/2-4(2011-07-01), 505-523</subfield>
   <subfield code="x">0038-6308</subfield>
   <subfield code="q">158:2-4&lt;505</subfield>
   <subfield code="1">2011</subfield>
   <subfield code="2">158</subfield>
   <subfield code="o">11214</subfield>
  </datafield>
  <datafield tag="900" ind1=" " ind2="7">
   <subfield code="a">Metadata rights reserved</subfield>
   <subfield code="b">Springer special CC-BY-NC licence</subfield>
   <subfield code="2">nationallicence</subfield>
  </datafield>
  <datafield tag="898" ind1=" " ind2=" ">
   <subfield code="a">BK010053</subfield>
   <subfield code="b">XK010053</subfield>
   <subfield code="c">XK010000</subfield>
  </datafield>
  <datafield tag="949" ind1=" " ind2=" ">
   <subfield code="B">NATIONALLICENCE</subfield>
   <subfield code="F">NATIONALLICENCE</subfield>
   <subfield code="b">NL-springer</subfield>
  </datafield>
 </record>
</collection>
