Temperature response of Mars to Milankovitch cycles
latitude varies predominately with precession and is not closely related to annual mean insolation. Based on the last few million years of orbital history, the precession cycle dominates in a narrow latitude range 54°–65°, in which the margins of the two ice-rich permafrost layers in each hemisphere...
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2008
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| Online Access: | http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.366.4045 http://www.ifa.hawaii.edu/~norb1/Papers/2008-milank.pdf |
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.366.4045 2023-05-15T16:37:28+02:00 Temperature response of Mars to Milankovitch cycles Norbert Schorghofer The Pennsylvania State University CiteSeerX Archives 2008 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.366.4045 http://www.ifa.hawaii.edu/~norb1/Papers/2008-milank.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.366.4045 http://www.ifa.hawaii.edu/~norb1/Papers/2008-milank.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://www.ifa.hawaii.edu/~norb1/Papers/2008-milank.pdf text 2008 ftciteseerx 2016-01-08T01:04:00Z latitude varies predominately with precession and is not closely related to annual mean insolation. Based on the last few million years of orbital history, the precession cycle dominates in a narrow latitude range 54°–65°, in which the margins of the two ice-rich permafrost layers in each hemisphere happen to lie, while mean annual temperature at other latitudes is controlled by the obliquity cycle. The phenomenon already exists on an airless uniform body in Mars orbit, where this latitude range shifts to 62°–74 ° on both hemispheres, and is closely related to temperature amplitude dependent reradiation Text Ice permafrost Unknown |
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Open Polar |
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Unknown |
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ftciteseerx |
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English |
| description |
latitude varies predominately with precession and is not closely related to annual mean insolation. Based on the last few million years of orbital history, the precession cycle dominates in a narrow latitude range 54°–65°, in which the margins of the two ice-rich permafrost layers in each hemisphere happen to lie, while mean annual temperature at other latitudes is controlled by the obliquity cycle. The phenomenon already exists on an airless uniform body in Mars orbit, where this latitude range shifts to 62°–74 ° on both hemispheres, and is closely related to temperature amplitude dependent reradiation |
| author2 |
The Pennsylvania State University CiteSeerX Archives |
| format |
Text |
| author |
Norbert Schorghofer |
| spellingShingle |
Norbert Schorghofer Temperature response of Mars to Milankovitch cycles |
| author_facet |
Norbert Schorghofer |
| author_sort |
Norbert Schorghofer |
| title |
Temperature response of Mars to Milankovitch cycles |
| title_short |
Temperature response of Mars to Milankovitch cycles |
| title_full |
Temperature response of Mars to Milankovitch cycles |
| title_fullStr |
Temperature response of Mars to Milankovitch cycles |
| title_full_unstemmed |
Temperature response of Mars to Milankovitch cycles |
| title_sort |
temperature response of mars to milankovitch cycles |
| publishDate |
2008 |
| url |
http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.366.4045 http://www.ifa.hawaii.edu/~norb1/Papers/2008-milank.pdf |
| genre |
Ice permafrost |
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Ice permafrost |
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http://www.ifa.hawaii.edu/~norb1/Papers/2008-milank.pdf |
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http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.366.4045 http://www.ifa.hawaii.edu/~norb1/Papers/2008-milank.pdf |
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Metadata may be used without restrictions as long as the oai identifier remains attached to it. |
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1766027767491592192 |