Physics
Scientific paper
Sep 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975jatp...37.1245s&link_type=abstract
Journal of Atmospheric and Terrestrial Physics, vol. 37, Sept. 1975, p. 1245-1253.
Physics
2
Atmospheric Density, Atmospheric Heating, Atmospheric Models, Atmospheric Temperature, Solar Radiation, Thermosphere, Wind Profiles, Atmospheric Attenuation, Density Distribution, Diurnal Variations, Far Ultraviolet Radiation, Incident Radiation, Temperature Distribution, Upper Atmosphere
Scientific paper
This paper discusses the extension of the numerical model of the earth's upper atmosphere described by Creekmore et al. (1975) to treat global wind, density and temperature fields generated by absorption of solar extreme ultraviolet (EUV) radiation. The equations of mass, momentum and energy conservation are solved in a spherical shell between the altitudes of 120 and 500 km. Comparisons of the calculated wind, density and temperature fields with those resulting from previous theoretical and observational studies are made. The phases of the density and temperature fields agree quite well with those given by empirical models. However, further comparisons indicate the necessity of a heat source at high latitudes, even during geomagnetically quiet times.
Ching B. K.
Chiu Yam T.
Creekmore S. P.
Harris Richard M.
Straus J. M.
No associations
LandOfFree
A global model of thermospheric dynamics. II - Wind, density, and temperature fields generated by EUV heating 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 global model of thermospheric dynamics. II - Wind, density, and temperature fields generated by EUV heating, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A global model of thermospheric dynamics. II - Wind, density, and temperature fields generated by EUV heating will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-911624