The structure of the Jovian stratosphere at the Galileo probe entry site is investigated through calculations of radiative heating rates based on measurements of the temperature profile, composition, and aerosol distribution. From analysis of mid-IR observations of Jupiter, we determine a C 2 H 2 mo
Earth-Based Observations of the Galileo Probe Entry Site
β Scribed by Orton, G.; Ortiz, J. L.; Baines, K.; Bjoraker, G.; Carsenty, U.; Colas, F.; Dayal, A.; Deming, D.; Drossart, P.; Frappa, E.; Friedson, J.; Goguen, J.; Golisch, W.; Griep, D.; Hernandez, C.; Hoffmann, W.; Jennings, D.; Kaminski, C.; Kuhn, J.; Laques, P.; Limaye, S.; Lin, H.; Lecacheux, J.; Martin, T.; McCabe, G.; Momary, T.; Parker, D.; Puetter, R.; Ressler, M.; Reyes, G.; Sada, P.; Spencer, J.; Spitale, J.; Stewart, S.; Varsik, J.; Warell, J.; Wild, W.; Yanamandra-Fisher, P.; Fazio, G.; Hora, J.; Deutsch, L.
- Book ID
- 121156164
- Publisher
- American Association for the Advancement of Science
- Year
- 1996
- Tongue
- English
- Weight
- 527 KB
- Volume
- 272
- Category
- Article
- ISSN
- 0036-8075
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