Indication of a near surface cloud layer on Venus from reanalysis of Venera 13/14 spectrophotometer data

European Space Agency, (Special Publication) ESA SP

Volumn , Issue 544, 2004, Pages 63-70

  Grieger, B ^a   Ignatiev, N I ^b   Hoekzema, N M ^a   Keller, H U ^a  

^a MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^b Space Research Institute ^*  (Russian Federation)

Author keywords

Huygens; Titan; Venera; Venus

Indexed keywords

APPROXIMATION THEORY; CLOUDS; COMPUTATIONAL METHODS; DATA REDUCTION; EXTRATERRESTRIAL ATMOSPHERES; MATHEMATICAL MODELS; OPTICAL PROPERTIES; PLANETS; SCATTERING; SOLAR RADIATION; SPACE PROBES; SPACE RESEARCH; SPECTROPHOTOMETERS;

HUYGENS; TITAN; VENERA; VENUS;

PLANETARY SURFACE ANALYSIS;

EID: 1542306771     PISSN: 03796566     EISSN: None     Source Type: Conference Proceeding    
DOI: None     Document Type: Conference Paper

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