The heliolatitudinal dependence of the parameters of solar wind

Details The heliolatitudinal dependence of the parameters of solar wind The heliolatitudinal dependence of the parameters of solar wind

Jul 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975kosis..13..603e&link_type=abstract

Kosmicheskie Issledovaniia, vol. 13, July-Aug. 1975, p. 603-605. In Russian.

Physics

2

Latitude, Solar Activity Effects, Solar Wind, Long Term Effects, Nonuniform Plasmas, Scintillation, Solar Cycles

Scientific paper

Radio scintillation measurements conducted with a number of satellites throughout an 11-year solar cycle show a latitudinal dependence in the velocity of solar wind heterogeneities. Observations were limited to plus or minus 7 deg solar latitude. There is a tendency for solar wind velocity to increase with increasing latitude. No phasic changes in the character of this dependence are seen over the 11-year cycle, but the effect increases in periods of minimum solar activity and decreases with increasing solar activity, vanishing in the year of maximum activity.

Affiliated with

Also associated with

No associations

Rating

The heliolatitudinal dependence of the parameters of 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 The heliolatitudinal dependence of the parameters of solar wind, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The heliolatitudinal dependence of the parameters of solar wind will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1756719