Formation of SCR Energy Spectra during Stochastic Acceleration with Allowance for Coulomb Losses

Details Formation of SCR Energy Spectra during Stochastic Acceleration with Allowance for Coulomb Losses Formation of SCR Energy Spectra during Stochastic Acceleration with Allowance for Coulomb Losses

Feb 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000astl...26..122o&link_type=abstract

Astronomy Letters, vol. 26, p. 122-128 (2000)

Astronomy and Astrophysics

Astronomy

6

Scientific paper

The stochastic acceleration of heavy ions by Alfven turbulence is considered with allowance for Coulomb losses. The pattern of energy dependence of these losses gives rise to characteristic features in the energy spectra of the accelerated particles at energies of the order of several MeV per nucleon. The manifestation of these features in the spectra is sensitive to the temperature and density of the medium, which can serve as a basis for plasma diagnostics in the flare region. Some impulsive solar energetic particle events during which features in the spectra of He-3 and He-4 were observed are considered as an example.

Affiliated with

Also associated with

No associations

Rating

Formation of SCR Energy Spectra during Stochastic Acceleration with Allowance for Coulomb Losses 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 Formation of SCR Energy Spectra during Stochastic Acceleration with Allowance for Coulomb Losses, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Formation of SCR Energy Spectra during Stochastic Acceleration with Allowance for Coulomb Losses will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1492631