Computer Science
Scientific paper
Aug 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ge%26ae..24..674z&link_type=abstract
Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 24, July-Aug. 1984, p. 674-676. In Russian.
Computer Science
Auroras, Geomagnetism, Ionospheric Conductivity, Magnetic Effects, Electron Precipitation, Latitude, Magnetic Disturbances
Scientific paper
A theoretical study is made of relative changes of certain auroral parameters with variations of the level of geomagnetic activity; the energy flux of auroral electrons, the ionospheric conductivity, and the frequency of occurrence of auroras are taken as the initial quantities. Attention is given to the relation between the latitudinal variation of the energy flux of precipitating electrons (0.2-27 keV) in magnetically disturbed conditions (AE greater than 300 nTl) and to the distribution for a quieter situation (AE less than 300 nTl). The results obtained reflect the latitudinal manifestation of the excess, super-background component of the quasi-viscous effect on the magnetosphere of the solar wind as well as a mechanism for the reconnection of the geomagnetic field and the IMF.
Gusev G. M.
Zaretskii N. S.
No associations
LandOfFree
Response in latitudinal distributions of auroral phenomena to variations of magnetic activity 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 Response in latitudinal distributions of auroral phenomena to variations of magnetic activity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Response in latitudinal distributions of auroral phenomena to variations of magnetic activity will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1675792