Mean Charge States of Solar Energetic Particles in Impulsive Events

Details Mean Charge States of Solar Energetic Particles in Impulsive Events Mean Charge States of Solar Energetic Particles in Impulsive Events

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....8.3161r&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

Scientific paper

The calculation of the mean charge states of various ion stages of abundant elements is the first step in understanding and modelling the X-ray emission from hot astrophysical plasmas such as stellar coronae. Our model combines acceleration with energy loss and charge stripping low in the corona. Therefore we have taken into account explicitly the second-order Fermi-type stochastic acceleration under a magnetohydrodynamic turbulence. We have found that the mean ionic charge states depend sensitively on plasma parameters as source temperature or density and on acceleration parameters as efficiency or the timescales for acceleration.

Affiliated with

Also associated with

No associations

Rating

Mean Charge States of Solar Energetic Particles in Impulsive Events 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 Mean Charge States of Solar Energetic Particles in Impulsive Events, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Mean Charge States of Solar Energetic Particles in Impulsive Events will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-798488