Trauger, J. T. and Münch, G. and Roesler, F. L. (1980) A study of the Jovian [S II] nebula at high spectral resolution. Astrophysical Journal, 236 (1). pp. 1035-1042. ISSN 0004-637X. doi:10.1086/157831. https://resolver.caltech.edu/CaltechAUTHORS:20140514-093628146
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Abstract
Observations of forbidden line S II λλ6716-6731 A emissions from the Jovian magnetosphere have been carried out with a PEPSIOS spectrometer at the Hale 5 m telescope. Spectral resolving power was sufficient to resolve the forbidden line S II line widths. From measured λλ6716-6731 A doublet ratios and spectral line widths a thermal plasma is found characterized by temperatures about 2 x 10^4 K and electron densities about ~2 x 10^3 cm^(-3). The source of forbidden line S II emissions was centered within a toroidal region of radius 5 Jupiter radii (inside the orbit of Io), with tight latitudinal confinement near the equilibrium equator for ions in the tilted corotating Jovian magnetic field, and significant long-lived longitudinal structure.
Item Type: | Article | |||||||||
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Additional Information: | © 1980 American Astronomical Society. Provided by the NASA Astrophysical Data System. This work has been supported by NASA through grant NGL 05-002-003 to the California Institute of Technology and by NSF through grant GA 15733 to the University of Wisconsin. | |||||||||
Issue or Number: | 1 | |||||||||
DOI: | 10.1086/157831 | |||||||||
Record Number: | CaltechAUTHORS:20140514-093628146 | |||||||||
Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20140514-093628146 | |||||||||
Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
ID Code: | 45737 | |||||||||
Collection: | CaltechAUTHORS | |||||||||
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Deposited On: | 14 May 2014 19:24 | |||||||||
Last Modified: | 10 Nov 2021 17:15 |
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