Flasar, F. M., Kunde, V. G., Abbas, M., Achterberg, R. K., Ade, Peter A. R. ![]() |
Abstract
The Composite Infrared Spectrometer (CIRS) consists of two interferometers, one polarizing, the other a conventional Michaelson interferometer, which together provide broad spectral coverage from 10 cm-1 to 1400 cm-1 (1 mm to 7 μ m), at a resolution as high as 0.5 cm-1. CIRS functions both as a thermometer and assayer of the target body, retrieving both thermal structure and composition. The Cassini spacecraft's 140-RJ flyby past Jupiter has enabled CIRS to observe Jupiter, its satellites, and its ring for six months with a spatial resolution up to 2.5o of jovian latitude at the subspacecraft point. This talk will include early results on Jupiter's atmospheric composition obtained from the relatively unexplored spectral region >50 μm, Jupiter's planetary-scale temperature field, and the compositional anomalies and temperatures associated with its auroral hot spots.
Item Type: | Conference or Workshop Item (Other) |
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Date Type: | Publication |
Status: | Published |
Schools: | Physics and Astronomy |
Subjects: | Q Science > QB Astronomy |
Uncontrolled Keywords: | 5704 Atmospheres--composition and chemistry, 5707 Atmospheres--structure and dynamics, 5739 Meteorology (3346), 5757 Remote sensing, 5764 Surfaces. |
Additional Information: | Unable to confirm full publication information for this item. Abstract #P51A-05. |
Publisher: | American Geophysical Union |
Last Modified: | 27 Oct 2022 08:59 |
URI: | https://orca.cardiff.ac.uk/id/eprint/64031 |
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