Publikationsdatum:
2019-08-13
Beschreibung:
Experimental measurements by ultraviolet photometers aboard Venera-9 and -10 are presented, discussed, and compared with various theoretical models of the ultraviolet structure of the atmosphere of Venus. The model in best agreement with observation provides for a finely dispersed, 8 km thick Rayleigh scattering layer above the primary cloud cover. Dark contrast details are considered to be breaks or areas of lower optical thickness in the upper scattering layer.
Schlagwort(e):
LUNAR AND PLANETARY EXPLORATION
Materialart:
NASA-TM-75543
,
PR-288
Format:
application/pdf
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