<?xml version="1.0"?>
<records>
  <record>
    <language>eng</language>
    <publisher>Ansari Education and Research Society</publisher>
    <journalTitle>Journal of Ultra Scientist of Physical Sciences</journalTitle>
    <issn/>
    <eissn/>
    <publicationDate>April 2008</publicationDate>
    <volume>20</volume>
    <issue>1</issue>
    <startPage>27</startPage>
    <endPage>34</endPage>
    <doi>jusps-B</doi>
    <publisherRecordId>1355</publisherRecordId>
    <documentType>article</documentType>
    <title language="eng">Study of MHD modes of Oscillations in Solar Coronal arcades</title>
    <authors>
      <author>
        <name>Seema Pande</name>
        <affiliationId>1</affiliationId>
      </author>
      <author>
        <name>Bimal Pande</name>
        <affiliationId>1</affiliationId>
      </author>
      <author>
        <name>Kavita Pandey</name>
        <affiliationId>1</affiliationId>
      </author>
    </authors>
    <affiliationsList>
      <affiliationName affiliationId="1">Department of Physics, Kumaun Universiry, Nainital (INDIA)</affiliationName>
    </affiliationsList>
    <abstract language="eng">&lt;p style="text-align: justify;"&gt;We have made an attempt to study magnetohydrodynamic (MHD) disturbances inside the coronal arcades by solving a pair of second-order two dimensional partial differential equations. MHD modes of oscillations of coronal arcades are investigated. It has been shown that the factors responsible for oscillatory modes give rise to the propagation of MHD waves.&lt;/p&gt;&#xD;
</abstract>
    <fullTextUrl format="html">https://ultraphysicalsciences.org/paper/1355/</fullTextUrl>
    <keywords>
      <keyword language="eng">modes</keyword>
    </keywords>
    <keywords>
      <keyword language="eng">Oscillations</keyword>
    </keywords>
    <keywords>
      <keyword language="eng">Solar Coronal </keyword>
    </keywords>
  </record>
</records>
