Zobrazeno 1 - 10
of 47
pro vyhledávání: '"Stephen S. Stahara"'
Autor:
Stephen S. Stahara
Publikováno v:
Planetary and Space Science. 50:421-442
A review is given of the author's two decades of magnetosheath modeling work with John Spreiter Beginning in the early 1970s, a sequence of computational magnetosheath submodels that extended and refined John's basic model were developed and successf
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a272d5c5a2bd321d5d693131e776ade9
https://doi.org/10.1016/s0032-0633(02)00023-5
https://doi.org/10.1016/s0032-0633(02)00023-5
Autor:
Stephen S. Stahara, Tamas I. Gombosi, Christopher T. Russell, John R. Spreiter, Paul Song, Xun‐Xie Zhang
Publikováno v:
Journal of Geophysical Research: Space Physics. 104:22357-22373
We test a new scheme to study the magnetosheath. The scheme uses the solar wind measurements as the input into the gasdynamic convected field model, and the model output is compared with magnetosheath observations. In our four test cases there is a s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::bd3fa3b44e883485636e096679268f57
https://doi.org/10.1029/1999ja900246
https://doi.org/10.1029/1999ja900246
Autor:
Stephen S. Stahara, Paul Song, Christopher T. Russell, Tamas I. Gombosi, Xiaoxin Zhang, John R. Spreiter
Publikováno v:
Journal of Geophysical Research: Space Physics. 104:22345-22355
We propose a new method to study the structure of the magnetosheath and thereby determine the underlying processes that create this structure. This method provides a systematic means of separating perturbations due to the solar wind variations from t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::57bfc87fd2eeddc5befa7a3fcc6dfbe1
https://doi.org/10.1029/1999ja900247
https://doi.org/10.1029/1999ja900247
Autor:
Stephen S. Stahara, John R. Spreiter
Publikováno v:
Venus and Mars: Atmospheres, Ionospheres, and Solar Wind Interactions
The fundamental ideas, successes, and shortcomings of fluid models based on MHD theory for the interaction of the solar wind and a planetary magnetic field and/or atmosphere are reviewed, with special attention to applications to Venus and Mars. An a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ff35e76ab933872a1b42923c5f0a7634
https://doi.org/10.1029/gm066p0345
https://doi.org/10.1029/gm066p0345
Publikováno v:
Journal of Geophysical Research: Space Physics. 101:27483-27497
Large-scale fluctuations in the solar wind plasma upstream of the heliospheric termination shock (TS) will cause inward and outward motions of the shock. Using numerical techniques, we extend an earlier strictly one-dimensional (planar) analytic gas
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ed405fe115280e37a6105a44457239c2
https://doi.org/10.1029/96ja02233
https://doi.org/10.1029/96ja02233
Autor:
John R. Spreiter, Joel A. Fedder, Stephen S. Stahara, Zerefsan Kaymaz, Janet G. Luhmann, John G. Lyon
Publikováno v:
Journal of Geophysical Research: Space Physics. 101:13321-13326
Fedder and Lyon [1995] recently showed the results from a global three-dimensional magnetohydrodynamic (MHD) model of the solar wind interaction with the Earth's magnetic field for northward interplanetary magnetic field (IMF) that exhibited a “tad
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::919583cdcc2d75ebb3aa4ccb06a1dc6a
https://doi.org/10.1029/96ja00509
https://doi.org/10.1029/96ja00509
Autor:
John R. Spreiter, Stephen S. Stahara, Paul Song, X. X. Zhang, Christopher T. Russell, Guan Le
Publikováno v:
Geophysical Research Letters. 23:105-108
Observations of the solar wind and the interplanetary magnetic field from ISEE-3 are used as input to the gasdynamic convected field model, as implemented in a new space weather forecast model. Then the model output, for three case studies, is compar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::80d1079d268ee0635c3c54eaf0184dec
https://doi.org/10.1029/95gl03503
https://doi.org/10.1029/95gl03503
Publikováno v:
Geophysical Research Letters. 20:751-754
In the past the global solar wind interaction with Venus has been treated principally with gas dynamic models. While this gas dynamic treatment has proven successful in modeling some of the global characteristics of the interaction, this model does n
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e29ca63344070b64ba07ae99f55fb28c
https://doi.org/10.1029/93gl00484
https://doi.org/10.1029/93gl00484
Publikováno v:
Journal of Geophysical Research: Planets. 98:3311-3318
Oxygen ion production rates above the ionopauses of Venus and Mars are calculated for photoionization, charge exchange, and solar wind electron impact ionization processes. The latter two require the use of the Spreiter and Stahara (1980) gas dynamic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7af0977d33c57b48c6df70aeaf21599a
https://doi.org/10.1029/92je02229
https://doi.org/10.1029/92je02229
Autor:
Stephen S. Stahara, John R. Spreiter
Publikováno v:
Discovery of the Magnetosphere ISBN: 087590288X
Discovery of the Magnetosphere
Discovery of the Magnetosphere
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a36f9e14fb52eebd7b75b441e109917f
https://doi.org/10.1029/hg007p0193
https://doi.org/10.1029/hg007p0193