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

S. K. Mishra; Talwinder Singh; P. Kayshap; A. K. Srivastava

doi:10.1017/S1743921318002028

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

Solar and Stellar Astrophysics 2019-01-30 v1

Authors: 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.

Keywords

mrt instability plasma spikes prominence eruption interplanetary space stereo observations

Cite

@article{arxiv.1806.01213,
  title  = {Propagation of MRT Unstable Plasma Spikes in the Inter-planetary Space},
  author = {S. K. Mishra and Talwinder Singh and P. Kayshap and A. K. Srivastava},
  journal= {arXiv preprint arXiv:1806.01213},
  year   = {2019}
}

Comments

IAU 340 Proceedings Paper

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