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|Title:||Solar plasma activated decametric radio emission of non-lo origin from Jupiter magnetosphere|
|Authors:||Bose, S K|
Bhattacharya, A B
|Abstract:||The interaction between solar plasma with Jovian magnetosphere has been highlighted by studying the correlation between decametric radio emission from the Jupiter with different solar plasma parameters and also with the interplanetary magnetic field feature and the he liospheric current sheet extent. Significance of the correlation is tested with usual statistical technique. Also the Chree-superposed-epoch analysis has been performed with lag-days correction for the observed solar plasma parameters at IAU, considering high values of occurrence probability of decametric radio-emission of non-lo origin from Jupiter as epoch days. The results of Chree analysis support the correlation study.|
|ISSN:||0975-105X (Online); 0367-8393 (Print)|
|Appears in Collections:||IJRSP Vol.32(1) [February 2003]|
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