Characteristics of the magnetospheric configuration in the case of stable convection activity

Details Characteristics of the magnetospheric configuration in the case of stable convection activity Characteristics of the magnetospheric configuration in the case of stable convection activity

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ge%26ae..31..722m&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 31, July-Aug. 1991, p. 722-725. In Russian.

Computer Science

Convection Currents, Geomagnetism, Magnetic Field Configurations, Magnetopause, Magnetospheric Instability, Polar Cusps, Goes Satellites, Nocturnal Variations, Remote Sensing

Scientific paper

Direct magnetic-field measurements are compared with T89 models for the stable convection period of 24 Nov. 1981. In the day sector, besides erosion of the daytime magnetopause in the magnetosphere, a strong depression of the Bz component (about 30 nTl) occurred, as a consequence of which the polar cusp in the Northern Hemisphere sank to the geeomagnetic latitude of 70 deg. In the nighttime magnetosphere at 6.6 earth radii, the magnetic configuration was characterized by a developed current sheet, and differed greatly from the model configuration.

Affiliated with

Also associated with

No associations

Rating

Characteristics of the magnetospheric configuration in the case of stable convection 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 Characteristics of the magnetospheric configuration in the case of stable convection activity, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Characteristics of the magnetospheric configuration in the case of stable convection activity will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1727156