Dynamics of daytime auroras depending on the IMF and magnetic activity

Details Dynamics of daytime auroras depending on the IMF and magnetic activity Dynamics of daytime auroras depending on the IMF and magnetic activity

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ge%26ae..28..251v&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 28, Mar.-Apr. 1988, p. 251-255. In Russian.

Computer Science

3

Auroras, Interplanetary Magnetic Fields, Magnetic Disturbances, Daytime, Magnetoactivity, Solar Terrestrial Interactions, Solar Wind

Scientific paper

The paper examines the effect of the Bz component of the IMF and the geomagnetic disturbance intensity on the position of discrete auroras in the daytime sector of the auroral oval. It is shown that, in the case of a weakly varying level of magnetic activity, the dynamics of the auroral glow band in the daytime sector is determined by Bz variations in the solar wind in earth orbit. As the magnetic disturbance region is intensified, the glow region is shifted toward the equator, and Bz-dependent variations of daytime aurora position occur at lower latitudes.

Affiliated with

Also associated with

No associations

Rating

Dynamics of daytime auroras depending on the IMF and 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 Dynamics of daytime auroras depending on the IMF and magnetic activity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dynamics of daytime auroras depending on the IMF and magnetic activity will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-848821