Mars thermospheric general circulation model: Calculations for the arrival of Phobos at Mars
The NCAR thermospheric general circulation model (TGCM) for the Earth's thermosphere has been modified to examine the three‐dimensional structure and circulation of the upper mesosphere and thermosphere of Mars (MTGCM). The computational framework and major processes unique to a CO2 thermospher...
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| Veröffentlicht in: | Geophysical research letters 1988-12, Vol.15 (13), p.1511-1514 |
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| container_end_page | 1514 |
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| container_issue | 13 |
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| container_title | Geophysical research letters |
| container_volume | 15 |
| creator | Bougher, S. W. Dickinson, R. E. Roble, R. G. Ridley, E. C. |
| description | The NCAR thermospheric general circulation model (TGCM) for the Earth's thermosphere has been modified to examine the three‐dimensional structure and circulation of the upper mesosphere and thermosphere of Mars (MTGCM). The computational framework and major processes unique to a CO2 thermosphere are similar to those utilized in a recent Venus TGCM. Mean orbital, seasonal, and solar conditions are specified. An Equinox version of the MTGCM is used to predict the Mars solar driven global circulation and structure for a non‐dusty (quiet) lower atmosphere at the time of arrival of the two Phobos spacecraft. |
| doi_str_mv | 10.1029/GL015i013p01511 |
| format | Article |
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An Equinox version of the MTGCM is used to predict the Mars solar driven global circulation and structure for a non‐dusty (quiet) lower atmosphere at the time of arrival of the two Phobos spacecraft.</description><subject>Arrivals</subject><subject>Astronomy</subject><subject>Carbon dioxide</subject><subject>Circulation</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>Mars</subject><subject>Mesosphere</subject><subject>Phobos</subject><subject>Planets, their satellites and rings. 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C.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Mars thermospheric general circulation model: Calculations for the arrival of Phobos at Mars</atitle><jtitle>Geophysical research letters</jtitle><addtitle>Geophys. Res. Lett</addtitle><date>1988-12</date><risdate>1988</risdate><volume>15</volume><issue>13</issue><spage>1511</spage><epage>1514</epage><pages>1511-1514</pages><issn>0094-8276</issn><eissn>1944-8007</eissn><coden>GPRLAJ</coden><abstract>The NCAR thermospheric general circulation model (TGCM) for the Earth's thermosphere has been modified to examine the three‐dimensional structure and circulation of the upper mesosphere and thermosphere of Mars (MTGCM). The computational framework and major processes unique to a CO2 thermosphere are similar to those utilized in a recent Venus TGCM. Mean orbital, seasonal, and solar conditions are specified. 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| identifier | ISSN: 0094-8276 |
| ispartof | Geophysical research letters, 1988-12, Vol.15 (13), p.1511-1514 |
| issn | 0094-8276 1944-8007 |
| language | eng |
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| source | Access via Wiley Online Library |
| subjects | Arrivals Astronomy Carbon dioxide Circulation Earth, ocean, space Exact sciences and technology Mars Mesosphere Phobos Planets, their satellites and rings. Asteroids Solar system Thermosphere Three dimensional |
| title | Mars thermospheric general circulation model: Calculations for the arrival of Phobos at Mars |
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