On the equivalence of the solar wind coupling parameter epsilon and the magnetospheric energy output parameter U(T) during intense geomagnetic storms

Details On the equivalence of the solar wind coupling parameter epsilon and the magnetospheric energy output parameter U(T) during intense geomagnetic storms On the equivalence of the solar wind coupling parameter epsilon and the magnetospheric energy output parameter U(T) during intense geomagnetic storms

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990p%26ss...38..341g&link_type=ejournal

Planetary and Space Science (ISSN 0032-0633), vol. 38, March 1990, p. 341, 342.

Physics

1

Earth Magnetosphere, Magnetic Storms, Solar Terrestrial Interactions, Solar Wind, Geomagnetism, Ring Currents

Scientific paper

Not Available

Affiliated with

Also associated with

No associations

Rating

On the equivalence of the solar wind coupling parameter epsilon and the magnetospheric energy output parameter U(T) during intense geomagnetic storms 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 On the equivalence of the solar wind coupling parameter epsilon and the magnetospheric energy output parameter U(T) during intense geomagnetic storms, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the equivalence of the solar wind coupling parameter epsilon and the magnetospheric energy output parameter U(T) during intense geomagnetic storms will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1250226