Garrard, T. L. and Stone, E. C. and Murphy, N. (1996) Effects of Absorption by lo on Composition of Energetic Heavy lons. Science, 274 (5286). pp. 393-394. ISSN 0036-8075. https://resolver.caltech.edu/CaltechAUTHORS:20140225-110013580
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Abstract
The Galileo heavy ion counter is sensitive to ions with atomic numbers Z ≥ 6 and energies greater than ~6 MeV per nucleon. During Galileo's passage through Jupiter's inner magnetosphere, the observed composition of these heavy ions was consistent with the presence of singly ionized iogenic O, Na, and S and highly ionized solar C, O, and Ne. The solar component is absorbed more strongly by lo because its gyroradius is smaller than Io's diameter.
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| Additional Information: | © 1996 American Association for the Advancement of Science. Received 4 September 1996; accepted 23 September 1996. This work was supported in part by NASA under NAS7-918. | ||||||
| Group: | Space Radiation Laboratory | ||||||
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| Issue or Number: | 5286 | ||||||
| Record Number: | CaltechAUTHORS:20140225-110013580 | ||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20140225-110013580 | ||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||||
| ID Code: | 43979 | ||||||
| Collection: | CaltechAUTHORS | ||||||
| Deposited By: | Tony Diaz | ||||||
| Deposited On: | 25 Feb 2014 19:21 | ||||||
| Last Modified: | 20 Feb 2020 14:33 |
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