Results 121 to 130 of about 31,830 (272)
This study addresses the challenge of utilizing incomplete long-term discharge data when using gridded precipitation datasets and data-driven modeling in Iran’s Karkheh basin.
Reza Morovati, Ozgur Kisi
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Geology of the Venus equatorial region from Pioneer Venus radar imaging [PDF]
The surface characteristics and morphology of the equatorial region of Venus were first described by Masursky et al. who showed this part of the planet to be characterized by two topographic provinces, rolling plains and highlands, and more recently by ...
Head, James W., Senske, D. A.
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Changing Extreme Precipitation Patterns in Nepal Over 1971–2015
This paper provides a comprehensive and comparative analysis of extreme precipitation patterns from 1971 to 2015 in Nepal, a data scarce, but “hot spot” region in global climate change.
Yinxue Luo +4 more
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Letter to Aphrodite Mamoulides from H.B. Stenzel on 1968-04-10
H.B. Stenzel
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Capitolo V – Nuovi aspetti di Apollo e di Aphrodite a Olbia
Benedetto Bravo
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Tessera terrain: Characteristics and models of origin [PDF]
Tessera terrain consists of complexly deformed regions characterized by sets of ridges and valleys that intersect at angles ranging from orthogonal to oblique, and were first viewed in Venera 15/16 SAR data. Tesserae cover more area (approx.
Bindschadler, D. L., Head, James W.
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Evidence for retrograde lithospheric subduction on Venus [PDF]
Though there is no plate tectonics per se on Venus, recent Magellan radar images and topographic profiles of the planet suggest the occurrence of the plate tectonic processes of lithospheric subduction and back-arc spreading.
Sandwell, David T., Schubert, Gerald
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Long-term variations in abundance and distribution of sulfuric acid vapor in the Venus atmosphere inferred from Pioneer Venus and Magellan radio occultation studies [PDF]
Radio occultation experiments have been used to study various properties of planetary atmospheres, including pressure and temperature profiles, and the abundance profiles of absorbing constituents in those planetary atmospheres. However, the reduction of
Jenkins, J. M., Steffes, P. G.
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