Propagation of MRT Unstable Plasma Spikes in the Inter-planetary Space
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.
- Publication:
-
Long-term Datasets for the Understanding of Solar and Stellar Magnetic Cycles
- Pub Date:
- February 2018
- DOI:
- 10.1017/S1743921318002028
- arXiv:
- arXiv:1806.01213
- Bibcode:
- 2018IAUS..340..237M
- Keywords:
-
- Astrophysics - Solar and Stellar Astrophysics
- E-Print:
- IAU 340 Proceedings Paper