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Propagation of MRT Unstable Plasma Spikes in the Inter-planetary Space

Published online by Cambridge University Press:  27 November 2018

Sudheer K. Mishra Open the ORCID record for Sudheer K. Mishra [Opens in a new window] ,
Talwinder Singh ,
P. Kayshap  and
A. K. Srivastava
Sudheer K. Mishra
Affiliation:
Department of Physics, Indian Institute of Technology (BHU), Varanasi-221005, India. email: sudheerkm.rs.phy16@itbhu.ac.in
Talwinder Singh
Affiliation:
Department of Space Science, University of Alabama in Huntsville, Huntsville, AL 35899, USA
P. Kayshap
Affiliation:
UMCS, Group of Astrophysics, UMCS, ul. Radziszewskiego 10, 20-031, Lublin, Poland
A. K. Srivastava
Affiliation:
Department of Physics, Indian Institute of Technology (BHU), Varanasi-221005, India. email: sudheerkm.rs.phy16@itbhu.ac.in
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Abstract

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We have used the Coronagraphic and Heliospheric Imaging data from Solar TErrestrial RElations Observatory (STEREO) to observe a prominence which is erupted on June 7th 2011. This prominence is subjected to the morphological evolution of MRT instability from the lower solar corona upto the inter-planetary space. The unstable structures are converted into the bunch of localized plasma spikes due to the turbulent mixing, and propagate in the inter-planetary space upto 1 A.U.

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