Zobrazeno 1 - 10
of 128
pro vyhledávání: '"D. L. Bindschadler"'
Publikováno v:
Acta Astronautica. 53:329-352
After a six-year odyssey, Galileo has completed its survey of the large moons of Jupiter. In the four years since the end of the primary mission, Galileo provided new insights into the fundamental questions concerning Jupiter and its moons and magnet
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::825e5ee39ea55535bca81d7b5c118c64
https://doi.org/10.1016/s0094-5765(03)00152-8
https://doi.org/10.1016/s0094-5765(03)00152-8
Publikováno v:
Acta Astronautica. 53:85-122
Galileo has completed the long awaited Io flybys of the Galileo Europa Mission and the Galileo Millennium Mission, and is now pumping up its apojove in each succeeding orbit in preparation for the chance to perform a dual spacecraft observation of th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9a0e37b429eeb268dcdd04e53fa4fe0a
https://doi.org/10.1016/s0094-5765(02)00276-x
https://doi.org/10.1016/s0094-5765(02)00276-x
Publikováno v:
Icarus. 111:417-432
Magellan altimetry data reveal that the center of figure (CF) of Venus is displaced approximately 280 m from its center of mass (CM) toward 4.4 deg S, 135.8 deg E, a location in Aphrodite Terra. This offset is smaller than those of other terrestrial
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5dcc15600eb8f000a4e0f1f12a7822b5
https://doi.org/10.1006/icar.1994.1153
https://doi.org/10.1006/icar.1994.1153
Autor:
D. L. Bindschadler, Richard E. Young, Howard Houben, Gerald Schubert, Leonhard Pfister, Richard L. Walterscheid
Publikováno v:
Journal of the Atmospheric Sciences. 51:1857-1875
This paper extends the study of stationary gravity waves generated near the surface of Venus reported previously by Young et al. to include finite amplitude effects associated with large amplitude waves. Waves are forced near the surface of Venus by
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::42f8510fd7ef4614ee6dbb98f8e0b149
https://doi.org/10.1175/1520-0469(1994)051<1857:cofasg>2.0.co
https://doi.org/10.1175/1520-0469(1994)051<1857:cofasg>2.0.co
Autor:
D. L. Bindschadler, Jeffrey E. Moersch, Gerald Schubert, Donald L. Turcotte, E. R. Stofan, Steven W. Squyres, Daniel M. Janes
Publikováno v:
Geophysical Research Letters. 20:2965-2968
Coronae are large quasi-circular geologica features that are common on Venus. They appear to be the surface tectonic and volcanic expressions of mantle diapirs that have impinged on the underside of the venusian lithosphere. We have investigated the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fa3ef6eb9c01aae046faee327369579c
https://doi.org/10.1029/93gl00866
https://doi.org/10.1029/93gl00866
Publikováno v:
Geophysical Research Letters. 18:2209-2212
The origin and evolution of Ishtar Terra is modeled using numerical simulations of crust/mantle interaction on Venus. Based on our modeling, we favor a two phase evolutionary sequence for Ishtar. The first phase is driven by bulk mantle flow due to t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9f6ba01390af72c8aed5ea9d130c5a3e
https://doi.org/10.1029/91gl02734
https://doi.org/10.1029/91gl02734
Publikováno v:
Geophysical Research Letters. 17:1345-1348
It is proposed that western Ishtar Terra formed due to compression and crustal thickening above a cylindrical mantle downwelling. A model for crustal deformation due to downwelling successfully reproduces many observed characteristics of western Isht
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0f8ab9232ebc55dd0a3cbddc45232459
https://doi.org/10.1029/gl017i009p01345
https://doi.org/10.1029/gl017i009p01345
Autor:
Yu. G. Shkuratov, Alexander T. Basilevsky, James W. Head, Mikhail A. Ivanov, Mikhail A. Kreslavsky, D. L. Bindschadler
Publikováno v:
Geophysical Research Letters. 17:171-174
Tessera terrain is the dominant tectonic unit in the northern hemisphere of Venus and is characterized by complex sets of intersecting structural trends and distinctive radar properties due to a high degree of meter and sub-meter scale (5 cm to 10 m)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::83879e1756990335d6903449408325e8
https://doi.org/10.1029/gl017i002p00171
https://doi.org/10.1029/gl017i002p00171
Publikováno v:
54th International Astronautical Congress of the International Astronautical Federation, the International Academy of Astronautics, and the International Institute of Space Law.
A summary of spacecraft performance in the harsh jovian environment and a report of final subsystem and instrument status are provided.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::882c8a1e17eb31b8fc745b881c9376f4
https://doi.org/10.2514/6.iac-03-q.2.01
https://doi.org/10.2514/6.iac-03-q.2.01