Radio occultation studies of the Venus atmosphere with the Magellan spaceraft. I - Experiemntal description and performance
The high effective isotropic radiated power (EIRP) from the Magellan spacecraft renders it an ideal transmitter for for radio occultation measurements of the Venus atmosphere's refractivity and absorptivity. A spacecraft tracking maneuver was designed to maintain the Magellan antenna pointing i...
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Veröffentlicht in: | Icarus (New York, N.Y. 1962) N.Y. 1962), 1994-07, Vol.110 (1), p.71-78 |
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Hauptverfasser: | , , , , , , |
Format: | Artikel |
Sprache: | eng |
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Zusammenfassung: | The high effective isotropic radiated power (EIRP) from the Magellan spacecraft renders it an ideal transmitter for for radio occultation measurements of the Venus atmosphere's refractivity and absorptivity. A spacecraft tracking maneuver was designed to maintain the Magellan antenna pointing in the direction of the refracted ray path back to Earth; this, together with the high EIRP of the Magellan transmitter has yielded 3.6 cm refractivity and absorptivity profiles. (AIAA) |
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ISSN: | 0019-1035 |