Fundamental Physical Processes in Coronae: Waves, Turbulence, Reconnection, and Particle Acceleration

Details Fundamental Physical Processes in Coronae: Waves, Turbulence, Reconnection, and Particle Acceleration Fundamental Physical Processes in Coronae: Waves, Turbulence, Reconnection, and Particle Acceleration

2007-10-31

arxiv.org/abs/0711.0007v1

Astronomy and Astrophysics

Astrophysics

Proc. IAU Symp. 247, Waves and Oscillations in the Solar Atmosphere: Heating and Magneto-Seismology, (ed. R. Erdelyi)

Scientific paper

10.1017/S1743921308014956

Our understanding of fundamental processes in the solar corona has been greatly progressed based on the space observations of SMM, Yohkoh, Compton GRO, SOHO, TRACE, RHESSI, and STEREO. We observe now acoustic waves, MHD oscillations, turbulence-related line broadening, magnetic configurations related to reconnection processes, and radiation from high-energy particles on a routine basis. We review a number of key observations in EUV, soft X-rays, and hard X-rays that innovated our physical understanding of the solar corona, in terms of hydrodynamics, MHD, plasma heating, and particle acceleration processes.

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