Mapping the zonal structure of Titan’s northern polar vortex
Saturn exhibits an obliquity of 26.7° such that the largest moon, Titan, experiences seasonal variations including the formation of a polar vortex in the winter hemisphere. Titan's polar vortex is characterised by cold stratospheric temperatures due to the lack of insolation over the winter pol...
| 主要な著者: | , , , , , , |
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| フォーマット: | Journal article |
| 言語: | English |
| 出版事項: |
Elsevier
2019
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