Marten, A., Gautier, D., Griffin, Matthew ![]() |
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Abstract
We report submillimeter heterodyne observations of Jupiter taken with the JCMT during and after the infall of Comet Shoemaker‐Levy 9 into the planet. We detected the J = 4 ‐ 3 and J = 3 ‐ 2 rotational transitions of HCN in emission at many of the impact sites. Measurements suggest for fragment G a mixing ratio of ∼ 5 × 10−8 above the 0.5‐mbar pressure level and a total HCN mass of 6 × 1011g. Subsequent observations, made in September and November 1994, reveal that HCN is still present but that the lines now appear in absorption. This results from a cooling of the stratospheric thermal profile between July and September. Chemical implications of the observed persistence of HCN in the Jovian stratosphere for over 6 months are discussed.
Item Type: | Article |
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Date Type: | Publication |
Status: | Published |
Schools: | Schools > Physics and Astronomy |
Subjects: | Q Science > QB Astronomy Q Science > QC Physics |
Additional Information: | Pdf uploaded in accordance with publisher's policy at http://www.sherpa.ac.uk/romeo/issn/0094-8276/ (accessed 20/02/2014). |
Publisher: | American Geophysical Union |
ISSN: | 0094-8276 |
Date of First Compliant Deposit: | 30 March 2016 |
Last Modified: | 09 May 2023 03:15 |
URI: | https://orca.cardiff.ac.uk/id/eprint/7395 |
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