Global structure of solar wind plasma flux output near the Sun.

Details Global structure of solar wind plasma flux output near the Sun. Global structure of solar wind plasma flux output near the Sun.

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994sccha..37..751w&link_type=abstract

Science in China, Series A, Vol. 37, No. 6, p. 751 - 760

Computer Science

Solar Wind: Plasma

Scientific paper

Based on the observational data for K-corona brightness, interplanetary scintillations and the photosphere's magnetic fields in the ten Carrington rotations, 1733 - 1742, in 1983, the average global structure of solar wind mass, momentum and energy flux outputs on the source surface (10 RS) near the Sun have been discussed and compared with those of the magnetic fields on the photosphere. The results imply that global structures of soplar plasma outputs near the Sun could be an important indicator for large scale global dynamical processes near the Sun.

Affiliated with

Also associated with

No associations

Rating

Global structure of solar wind plasma flux output near the Sun. 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 Global structure of solar wind plasma flux output near the Sun., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Global structure of solar wind plasma flux output near the Sun. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1508376