Physics
Scientific paper
Mar 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986jgr....91.3287h&link_type=abstract
Journal of Geophysical Research (ISSN 0148-0227), vol. 91, March 1, 1986, p. 3287-3293.
Physics
35
Earth Magnetosphere, Electron Precipitation, Interplanetary Magnetic Fields, Polar Caps, Electrojets, Energy Transfer, Magnetopause, Polar Substorms
Scientific paper
Magnetospheric substorm data assembled at the Sixth Coordinated Data Analysis Workshop were analyzed in an attempt to define an average energy model of open flux in the polar cap. The model is applied to the growth phase of substorm events recorded in terms of precipitating electron data obtained with instrumentation on the DMSP-F2 and P78-1 polar orbiting satellites during two substorms on March 27, 1979. Simultaneous data on the state of the IMF was obtained with the IMP and ISEE 3 spacecraft. The model calculations indicate that the magnetopause merged with the IMF to produce an average efficiency of flux input from the IMF of 0.16-0.22 during average solar wind conditions. A proportionality was observed between the westward electrojet current during the expansion and recovery phases of the substorms and the time rate of decrease of the polar cap flux due to the merging activity in the magnetotail. The average energy model is concluded useful for predicting regions of open flux (the polar cap boundary) during the substorm growth phase and in the magnetically disturbed times of the expansion and recovery phases of substorms.
Hardy David A.
Holzer Robert E.
McPherron Robert L.
No associations
LandOfFree
A quantitative empirical model of the magnetospheric flux transfer process 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 quantitative empirical model of the magnetospheric flux transfer process, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A quantitative empirical model of the magnetospheric flux transfer process will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1283166