Nonlinear processes involved in particle acceleration in solar flares

Details Nonlinear processes involved in particle acceleration in solar flares Nonlinear processes involved in particle acceleration in solar flares

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981phyd....2...87s&link_type=abstract

Physica D: Nonlinear Phenomena, Volume 2, Issue 1, p. 87-89.

Physics

Scientific paper

Requirements for nonrelativistic electron accelaration in solar flares are reviewed. Candidate mechanisms for the primary energy release in flares, steady-state reconnection and the tearing mode instability, are examined to see to what extent they can satisfy these requirements. By examining direct electric field acceleration and electron plasma wave acceleration into their nonlinear phases it is concluded that at most 0.1% of the flare energy can be deposited into nonthermal streaming electrons with the primary energy release mechanisms as they have been proposed and analyzed. Implications for hard X-ray emission models and ion acceleration are given.

Affiliated with

Also associated with

No associations

Rating

Nonlinear processes involved in particle acceleration in solar flares 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 Nonlinear processes involved in particle acceleration in solar flares, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Nonlinear processes involved in particle acceleration in solar flares will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1054213