A high time resolution study of the solar wind-magnetosphere energy coupling function

Details A high time resolution study of the solar wind-magnetosphere energy coupling function A high time resolution study of the solar wind-magnetosphere energy coupling function

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982p%26ss...30..537a&link_type=abstract

Planetary and Space Science, vol. 30, June 1982, p. 537-543

Physics

8

Earth Magnetosphere, Energy Dissipation, Solar Terrestrial Interactions, Solar Wind, Coupling, Magnetic Storms, Temporal Resolution

Scientific paper

A high time resolution study of the relationships between the solar wind-magnetosphere energy coupling function and the total energy dissipation rate of the magnetosphere is made using 5-min average values of solar wind data and of the geomagnetic indices AE and Dst. All the results are essentially the same as those obtained by the earlier studies which were based on the hourly average data set. Therefore, it is confirmed that the magnetosphere is primarily a driven system

Affiliated with

Also associated with

No associations

Rating

A high time resolution study of the solar wind-magnetosphere energy coupling function 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 A high time resolution study of the solar wind-magnetosphere energy coupling function, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A high time resolution study of the solar wind-magnetosphere energy coupling function will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1354983