Solar Cycle Dependence of High-Latitude Solar Wind

Details Solar Cycle Dependence of High-Latitude Solar Wind Solar Cycle Dependence of High-Latitude Solar Wind

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..679..141f&link_type=abstract

SOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conference. AIP Conference Proceedings, Volume 679, pp. 141-1

Physics

3

Particle Emission, Solar Wind, Solar Wind Plasma, Sources Of Solar Wind

Scientific paper

How has the high-latitude solar wind velocity changed over the solar activity cycle? We analyzed interplanetary scintillation data during the years 1985-2001 (excluding the few years around solar maximum) and obtained the following results: (1) the solar wind in the polar region did not change its speed even during the phases of rising and declining solar activity, (2) the N-S asymmetry of the high-latitude solar wind speed is a stable structure from 1987 to 1998, (3) the latitudinal velocity gradient at high latitude becomes steeper with increasing solar activity.

Affiliated with

Also associated with

No associations

Rating

Solar Cycle Dependence of High-Latitude 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 Solar Cycle Dependence of High-Latitude Solar Wind, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar Cycle Dependence of High-Latitude Solar Wind will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1148753