Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985kosis..23..248l&link_type=abstract
Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 23, Mar.-Apr. 1985, p. 248-258. In Russian.
Astronomy and Astrophysics
Astronomy
Brightness Temperature, Infrared Astronomy, Planetary Temperature, Spaceborne Experiments, Venera Satellites, Heat Flux, Latitude, Northern Hemisphere, Temperature Profiles
Scientific paper
Venera-15 infrared data were represented in the following ways: latitude dependence of brightness temperature for selected wave numbers; dependence of brightness temperature on date and solar time for selected latitudes; and analogous dependences for the spectrum ('flux') integral. A preliminary analysis shows the existence of three characteristic regions in the northern hemisphere of Venus: low latitudes (40-60 deg) where the brightness temperatures and fluxes are constant; a 'cold zone' (60-75 deg), with large variations; and a warm 'polar cap' (phi greater than 75 deg). It is also shown that thermal asymmetry is absent at latitudes below 60 deg, that hot spots may occur in pairs, and that the cold zone does not rotate together with the atmosphere.
Diachkov A. V.
Diubua R.
Doehler W.
Kerzhanovich Viktor V.
Linkin V. M.
No associations
LandOfFree
The Venera 15 and 16 infrared experiment. V - Preliminary analysis of fields of brightness temperatures and heat fluxes 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 The Venera 15 and 16 infrared experiment. V - Preliminary analysis of fields of brightness temperatures and heat fluxes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Venera 15 and 16 infrared experiment. V - Preliminary analysis of fields of brightness temperatures and heat fluxes will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-823710