Multiwavelength Aspects of Stellar Coronae

Details Multiwavelength Aspects of Stellar Coronae Multiwavelength Aspects of Stellar Coronae

2001-09-17

arxiv.org/abs/astro-ph/0109266v1

Astronomy and Astrophysics

Astrophysics

review paper to appear in 35th ESLAB Symposium "Stellar Coronae in the Chandra and XMM-Newton Era", eds. F. Favata & J.J. Drak

Scientific paper

Coronae express different facets of their energy release processes in different wavelength regions. While soft X-ray and EUV emission dominates the radiative losses of the thermal plasma, hard X-ray emission (>10 keV) can be produced from non-thermal high-energy particles accelerated as a consequence of flare processes, and radio emission is often emitted from mildly relativistic electrons trapped in magnetic fields. Combined measurements of all emissions are important to understand the ultimate mechanisms responsible for coronal energy release and heating. This presentation will summarize a number of aspects for which multi-wavelength studies are important, both for quiescent and flare emission.

Affiliated with

Also associated with

No associations

Rating

Multiwavelength Aspects of Stellar Coronae does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Multiwavelength Aspects of Stellar Coronae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Multiwavelength Aspects of Stellar Coronae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-132266