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arXiv · 1806.01213

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

S. K. Mishra·Talwinder Singh·P. Kayshap·A. K. Srivastava
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Abstract

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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S. K. Mishra, Talwinder Singh, P. Kayshap, A. K. Srivastava. 2018-06-04. Propagation of MRT Unstable Plasma Spikes in the Inter-planetary Space. https://doi.org/10.1017/s1743921318002028

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