Large‐scale patterns of eolian sediment transport on Venus: Predictions for Magellan
- 1 August 1990
- journal article
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 17 (9) , 1365-1368
- https://doi.org/10.1029/gl017i009p01365
Abstract
No abstract availableThis publication has 14 references indexed in Scilit:
- Surface characteristics of Venus derived from Pioneer Venus altimetry, roughness, and reflectivity measurementsJournal of Geophysical Research, 1985
- Transport of venusian rolling ‘stones’ by wind?Nature, 1985
- Windblown sand on Venus: Preliminary results of laboratory simulationsIcarus, 1984
- Atmospheric tides on VenusIcarus, 1983
- Venera 13 and Venera 14: Sedimentary Rocks on Venus?Science, 1983
- Venus: Global Surface Radar ReflectivityScience, 1982
- Venus: Chemical Weathering of Igneous Rocks and Buffering of Atmospheric CompositionScience, 1982
- Atmospheric tides and the rotation of Venus I. Tidal theory and the balance of torquesIcarus, 1980
- Venus Winds Are Zonal and Retrograde Below the CloudsScience, 1979
- Diurnal Tide in the Martian AtmosphereJournal of the Atmospheric Sciences, 1976