Astronomy and Astrophysics – Astrophysics
Scientific paper
May 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004asthe..97..276s&link_type=abstract
The Astronomical Herald (ISSN 0374-2466), Vol. 97, No. 5, p. 276 - 286 (2004)
Astronomy and Astrophysics
Astrophysics
3
Astrophysical Plasmas, Clusters Of Galaxies, Solar Corona
Scientific paper
It is widely known that hot plasma is ubiquitous in various astrophysical objects from stars to galaxy clusters. I have worked on the wave dissipation which play a role in the momentum and energy transfer in the plasma. In this article, I firstly introduce our results on the wave heating and acceleration in the solar corona. I show that two kinds of the solar winds, the high-speed wind and low-speed wind, can be explained by the dissipation of different types of the waves. Then, we apply the wave dissipation to the heating in galaxy clusters in collaboration with Yutaka Fujita and Keiichi Wada (NAOJ). We show that the wave heating could be an effective process in reducing the cooling flow.
No associations
LandOfFree
Wave heating in astrophysical plasma - examples in the solar corona and in galaxy clusters 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 Wave heating in astrophysical plasma - examples in the solar corona and in galaxy clusters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Wave heating in astrophysical plasma - examples in the solar corona and in galaxy clusters will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1056972