Computer Science
Scientific paper
Dec 1977
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977ge%26ae..17.1122d&link_type=abstract
Geomagnetizm i Aeronomiia, vol. 17, Nov.-Dec. 1977, p. 1122-1124. In Russian.
Computer Science
Atmospheric Attenuation, Ionospheric Propagation, Magnetohydrodynamic Waves, Solar Activity Effects, Upper Atmosphere, Atmospheric Heating, Flux Density, Geomagnetism, Solar Wind
Scientific paper
MHD waves are generated in the interaction of the solar wind with the geomagnetic field. In the present paper, a theoretical analysis is presented of the upper-atmospheric absorption of MHD waves, propagating perpendicular to an external uniform magnetic field, and the efficiency of MHD-wave absorption as a heating mechanism for the neutral component of the upper atmosphere is evaluated. It is determined that, in the ionospheric height range of 100-200 km, MHD-wave heating of the atmosphere is comparable to solar-UV heating.
Diogenova T. V.
Khazanov George V.
Koen Mikhail A.
Konnikov Iu. V.
No associations
LandOfFree
Absorption of MHD waves in the upper atmosphere 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 Absorption of MHD waves in the upper atmosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Absorption of MHD waves in the upper atmosphere will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1418366