Physics
Scientific paper
Nov 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981icar...48..167v&link_type=abstract
Icarus, vol. 48, Nov. 1981, p. 167-179.
Physics
6
Atmospheric Heating, Mercury (Planet), Planetary Atmospheres, Solar Radiation, Upper Atmosphere, Venus Atmosphere, Diurnal Variations, Incident Radiation, Insolation, Radiation Distribution, Thermal Absorption, Planets, Mercury (Planet), Venus, Solar Radiation, Atmosphere, Insolation, Distribution, Diurnal Variations, Seasonal Variations, Cycles, Obliquity, Parameters, Calculations, Latitude, Diagrams, Orbits, Polar Regions, Equatorial Regions, Periodicity, Eccentricity
Scientific paper
A formalism has been developed for the calculation of the insolation on the planets Mercury and Venus neglecting any atmospheric absorption. For Mercury, the instantaneous insolation curves are repeated in a 2-tropical-year cycle, the distribution of the solar radiation being perfectly symmetric between both hemispheres. In addition to latitudinal variations, one observes a longitudinal effect expressed by different instantaneous insolation distributions during the course of the time; on the equator, the relative diurnal insolation variability may attain a factor of three. The small obliquity of Venus results in a nearly symmetric solar radiation distribution with respect to the equator except at the poles, where an important seasonal effect has been found. It has to be noted that no longitudinal dependence exists. Finally, the insolation curves are repeated in a nearly half-year cycle.
van Hemelrijck E.
Vercheval J.
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