Physical nature of the low-speed solar wind

Details Physical nature of the low-speed solar wind Physical nature of the low-speed solar wind

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..385...17g&link_type=abstract

Scientific basis for robotic exploration close to the sun. AIP Conference Proceedings, Volume 385, pp. 17-24 (1997).

Other

11

Particle Emission, Solar Wind, Neutrino, Muon, Pion, And Other Elementary Particles, Cosmic Rays

Scientific paper

In situ observations indicate that the low-speed wind is highly variable. It commonly originates on open field lines that thread coronal streamers in the vicinity of the magnetic equator, but transient ejections are also a source of low-speed flows on occasion. Close to the Sun a large flow shear probably is common at the interface between low- and high-speed flows. Near solar activity minimum low-speed flows are confined to a narrow band 40-45° wide centered roughly on the solar equator, but near solar maximum low-speed flows may dominate at all heliographic latitudes.

Affiliated with

Also associated with

No associations

Rating

Physical nature of the low-speed 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 Physical nature of the low-speed solar wind, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Physical nature of the low-speed solar wind will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1783364