Solar coronal heating by high-frequency dispersive Alfvén waves

Details Solar coronal heating by high-frequency dispersive Alfvén waves Solar coronal heating by high-frequency dispersive Alfvén waves

May 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999soph..186...61s&link_type=abstract

Solar Physics, v. 186, Issue 1/2, p. 61-66 (1999).

Physics

19

Scientific paper

It is shown that high-frequency dispersive kinetic Alfvén waves
can cause significant electron heating in the solar corona. The heating
is produced by collisionless electron Landau dissipation of the parallel
electron current associated with high-frequency dispersive kinetic
Alfvén waves, which have a parallel electric field.

Affiliated with

Also associated with

No associations

Rating

Solar coronal heating by high-frequency dispersive Alfvén waves 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 Solar coronal heating by high-frequency dispersive Alfvén waves, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar coronal heating by high-frequency dispersive Alfvén waves will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1193963