Observational constraints on solar wind acceleration mechanisms

Details Observational constraints on solar wind acceleration mechanisms Observational constraints on solar wind acceleration mechanisms

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nascp.2280.135n&link_type=abstract

In its Solar Wind Five p 135-146 (SEE N84-13067 03-92)

Computer Science

2

Flow Velocity, Magnetohydrodynamic Flow, Plasma Acceleration, Solar Wind, Boundary Layer Flow, Coronal Holes, Stellar Mass Ejection

Scientific paper

A complete theoretical understanding of the acceleration of the solar wind must account for at least three types of solar wind flow: high-speed streams associated with coronal holes, low-speed boundary layer flows associated with sector boundaries, and both high- and low-speed flows associated with impulsive ejections from the Sun. The properties of each type of flow are summarized.

Affiliated with

Also associated with

No associations

Rating

Observational constraints on solar wind acceleration mechanisms 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 Observational constraints on solar wind acceleration mechanisms, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observational constraints on solar wind acceleration mechanisms will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1487580