Temporal Behavior of Stratospheric Ammonia Abundance and Temperature Following the SL9 Impacts
Infrared emission lines of stratospheric ammonia (NH 3) were observed following the collisions of the fragments of Comet Shoemaker–Levy 9 with Jupiter in July of 1994 at the impact sites of fragments G and K. Infrared heterodyne spectra near 10.7 μm were obtained by A. Betz et al. (in Abstracts for...
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Veröffentlicht in: | Icarus (New York, N.Y. 1962) N.Y. 1962), 2002-04, Vol.156 (2), p.485-497 |
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Sprache: | eng |
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