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

  • Sudheer K. Mishra (a1), Talwinder Singh (a2), P. Kayshap (a3) and A. K. Srivastava (a1)


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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