Self-Consistent MHD Modeling of Solar Wind

Details Self-Consistent MHD Modeling of Solar Wind Self-Consistent MHD Modeling of Solar Wind

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..369..557s&link_type=abstract

New Solar Physics with Solar-B Mission ASP Conference Series, Vol. 369, proceedings of the conference held 8-11 November, 2005 a

Physics

Scientific paper

We study solar winds driven by low-frequency Alfven waves from the photosphere in coronal holes by using time-dependent numerical simulations. As shown in Suzuki & Inutsuka (2005; 2006) Alfven waves effectively dissipate through compressive-wave generation and wave reflection to heat up and accelerate the solar wind plasma. We also investigate photosphere-corona/solar wind connections which can be directly compared with future observations by Solar-B. By simulations in various coronal holes we analyse how physical properties of the corona and solar wind depend on Alfven wave parameters at the photosphere. We discuss some characteristic relations inferred from the nonlinear dissipation of the low-frequency Alfven waves in the light of Solar-B observations.

Affiliated with

Also associated with

No associations

Rating

Self-Consistent MHD Modeling of Solar Wind 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 Self-Consistent MHD Modeling of Solar Wind, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Self-Consistent MHD Modeling of Solar Wind will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-952406