Changes in the geometry of the solar wind transition region with the level of solar activity

Details Changes in the geometry of the solar wind transition region with the level of solar activity Changes in the geometry of the solar wind transition region with the level of solar activity

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ge%26ae..26....6l&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 26, Jan.-Feb. 1986, p. 6-9. In Russian.

Computer Science

Anisotropic Media, Scintillation, Solar Activity, Solar Wind Velocity, Transition Points, Solar Cycles, Supersonic Flow

Scientific paper

The dynamics of the circumsolar medium is investigated in the complex supersonic transition region on the basis of scintillation observations. In particular, attention is given to the problem of separating two effects, i.e., heliolatitudinal anisotropy and radial changes of the medium parameters, which arises at the decline phase of the 11-yr solar cycle. It is found that the heliolatitudinal changes of the scintillation index in the transition region are substantially less than scintillation enhancement in this region.

Affiliated with

Also associated with

No associations

Rating

Changes in the geometry of the solar wind transition region with the level of solar activity 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 Changes in the geometry of the solar wind transition region with the level of solar activity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Changes in the geometry of the solar wind transition region with the level of solar activity will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1675557