Observations of selected coronae from Venusian quadrangles V31 and V19

Details Observations of selected coronae from Venusian quadrangles V31 and V19 Observations of selected coronae from Venusian quadrangles V31 and V19

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..259c&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 259.

Mathematics

Logic

Venus Surface, Topography, Coronas, Satellite Imagery, Planetary Geology, Plains, Volcanoes

Scientific paper

Observations from FMAP images and topographic data reveal coronae within V31 and V19 to have a more complex, protracted history than previously recorded. Five coronae are studied here in detail: the Idem-Kuva and Nissaba coronae situated on the Western Eistla Rise and the Heng-o, Beten, and Silvia coronae contained with the Guinevere Lineated and Mottled Plains and Guinevere Regional Plains units. It is inferred that the amount of relief at any individual corona is more strongly controlled by the amount of uplift and/or volcanic construction which has taken place, and that not all coronae may go through a dome or plateau-shaped phase. It is also shown that coronae both pre- and post-date formation of the adjacent plains and can have a long, complex geologic history.

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