Published December 1, 1977
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Journal Article
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Search for Jovian auroral hot spots
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Abstract
Auroral emission originating at the foot of the Io-associated flux tube at Jupiter has been detected with a high-resolution spectrometer/telescope on board the Orbiting Astronomical Observatory Copernicus. The emission intensity at Ly-alpha is found to be greater than 100 kR, and the emission is located at zenographic latitudes greater than 65°.
Additional Information
© 1977 American Astronomical Society. Provided by the NASA Astrophysics Data System. Partial support provided by NASA grant NSG-5139 and AURA subcontract 86303 (NASA/JPL contract 7-100) is gratefully acknowledged.Attached Files
Published - 1977ApJ___218L__83A.pdf
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1977ApJ___218L__83A.pdf
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Additional details
- Eprint ID
- 49903
- Resolver ID
- CaltechAUTHORS:20140922-130207209
- NASA
- NSG-5139
- Association of Universities for Research in Astronomy (AURA)
- 86303
- NASA
- NAS 7-100
- Created
-
2014-09-22Created from EPrint's datestamp field
- Updated
-
2021-11-10Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences (GPS)