Paper:	Solar Coronal Shocks and Particle Acceleration as Deduced from EUV, Radio, and In-situ Observations
Volume:	456, The Fifth Hinode Science Meeting
Page:	151
Authors:	Kozarev, K. A.; Korreck, K. E.; Lobzin, V. V.; Schwadron, N. A.
Abstract:	We utilize the great angular resolution and unprecedented cadence of the Advanced Imaging Assembly instrument on the Solar Dynamics Observatory to characterize shocks forming in the low solar corona. We present recent observations of extreme ultraviolet (EUV) off-limb bright fronts and radio shock wave signatures. Our analysis shows that the EUV observations correspond to compressed plasma behind fast coronal shocks, but they do not uniformly accelerate electrons at their nose. We have attempted here to estimate the significance of magnetic geometry for accelerating energetic particles in a model coronal shock.

Astronomical Society of the Pacific
Conference Series

© Copyright 1988 - 2024 - Astronomical Society of the Pacific
No part of the material protected by this copyright may be reproduced or used in any form other than for personal use without written permission from the ASP.

Page generated in 0.039 seconds