Geometry of the transition region of the solar wind in the 11-year solar cycle

Details Geometry of the transition region of the solar wind in the 11-year solar cycle Geometry of the transition region of the solar wind in the 11-year solar cycle

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ge%26ae..26..488l&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 26, May-June 1986, p. 488-490. In Russian.

Physics

Interplanetary Medium, Morphology, Plasma Dynamics, Solar Cycles, Solar Wind Velocity, Transition Points, Geomagnetism, Solar Terrestrial Interactions

Scientific paper

The geometry of the transition region of the solar wind and its dynamics during the 11-year solar cycle are investigated on the basis of data for 1972-1982; shapes representing the heliolatitudinal geometry of the transition region are presented. The existence of a correlation between the location of the transition-region boundaries and the Kp index makes it possible to use observations of the transition region to predict geomagnetic activity over a period longer than that allowed by the use of conventional scintillation observations.

Affiliated with

Also associated with

No associations

Rating

Geometry of the transition region of the solar wind in the 11-year solar cycle 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 Geometry of the transition region of the solar wind in the 11-year solar cycle, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Geometry of the transition region of the solar wind in the 11-year solar cycle will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1832184