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3. Structure of the Atmosphere of Venus up to 110 Kilometers: Preliminary Results from the Four Pioneer Venus Entry Probes. Seiff A; Kirk DB; Sommer SC; Young RE; Blanchard RC; Juergens DW; Lepetich JE; Intrieri PF; Findlay JT; Derr JS Science; 1979 Feb; 203(4382):787-90. PubMed ID: 17832998 [TBL] [Abstract][Full Text] [Related]
4. Venus winds are zonal and retrograde below the clouds. Counselman CC; Gourevitch SA; King RW; Loriot GB; Prinn RG Science; 1979 Jul; 205(4401):85-7. PubMed ID: 17778911 [TBL] [Abstract][Full Text] [Related]
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