<?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>47</startPage>
    <endPage>50</endPage>
    <doi>jusps-B</doi>
    <publisherRecordId>1357</publisherRecordId>
    <documentType>article</documentType>
    <title language="eng">Spherical shock in heat radiating atmosphere</title>
    <authors>
      <author>
        <name>R.P. Yadav (rpyadav93physics@yahoo.co.in)</name>
        <affiliationId>1</affiliationId>
      </author>
      <author>
        <name>Ratnesh Kumar </name>
        <affiliationId>1</affiliationId>
      </author>
      <author>
        <name>Manoj Kumar Gangwar</name>
        <affiliationId>1</affiliationId>
      </author>
    </authors>
    <affiliationsList>
      <affiliationName affiliationId="1">Physics, Deptt., Govt., P.G. College, Bisalpur (Pillibhit) 262201 (INDIA)</affiliationName>
    </affiliationsList>
    <abstract language="eng">&lt;p style="text-align: justify;"&gt;Chester - Chesnell- Whitham method has been applied to study the propagation of strong spherical shock in the heat radiating atmosphere having uniform density distribution. Neglecting the effect of overtaking disturbances the analytical expressions for shock velocity, shock strength, particle velocity and pressure have been obtained using Bhowmick conditions. The results obtained here are compared with those for non-radiating heat atmosphere.&lt;br /&gt;&#xD;
&amp;nbsp;&lt;/p&gt;&#xD;
</abstract>
    <fullTextUrl format="html">https://ultraphysicalsciences.org/paper/1357/</fullTextUrl>
    <keywords>
      <keyword language="eng">Isothermal propagation</keyword>
    </keywords>
    <keywords>
      <keyword language="eng">Shock wave</keyword>
    </keywords>
    <keywords>
      <keyword language="eng"> Uniform density distribution</keyword>
    </keywords>
  </record>
</records>
