High-energy particles at and from the Sun

Details High-energy particles at and from the Sun High-energy particles at and from the Sun

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007sf2a.conf....7k&link_type=abstract

SF2A-2007: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics held in Grenoble, France, July

Astronomy and Astrophysics

Astrophysics

Scientific paper

Non thermal particles up to relativistic energies contain a large fraction of the energy released during solar activity, especially flares and coronal mass ejections. The Sun gives us a unique opportunity to observe radiative signatures of these particles at time scales relevant to their acceleration, to measure in space those particles which escape from the Sun, and to image the environment where the particles are accelerated. Shock waves of coronal mass ejections and magnetic reconnection during flares are the most plausible origins of energetic particle populations. The paper outlines recent work with emphasis on the French Solar-Terrerstrial Physics community.

Affiliated with

Also associated with

No associations

Rating

High-energy particles at and from the Sun 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 High-energy particles at and from the Sun, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High-energy particles at and from the Sun will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-789685