Probing the Properties and Effects of Coronal Shocks Using Modeling, Simulations and Observations
Abstract
We start with the 3D reconstruction of evolving shock waves based on remote-sensing observations that provide the shock's outermost extent, 3-D expansion speeds, geometry, Mach and a new technique to derive compression ratio. We compare the results of these reconstructions with other techniques. We then carried out case studies and surveys to study the link between these shock waves and electromagnetic emissions at radio, X-ray and gamma-ray frequencies. We focus on the onsets of radio type II bursts and exploit a new modeling framework that includes particle acceleration and transport effects to study the onset of a number of hard X-ray and gamma-ray events.
- Publication:
-
Solar Heliospheric and INterplanetary Environment (SHINE 2018)
- Pub Date:
- July 2018
- Bibcode:
- 2018shin.confE.140R