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Detailed Reference Information |
Kiehling, J.E., Ammirati, T.F., Moore, M.D., Monce, M.N. and Hansel, E.F. (2001). Proton impact excitation of SO2. Journal of Geophysical Research 106: doi: 10.1029/2000JA002502. issn: 0148-0227. |
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Because of the interest in atomic emissions observed from the Io plasma torus, we have investigated the spectrum produced by proton impact on SO2 in the wavelength region of 380--800 nm. The proton energy was varied from 50 to 225 keV. The spectrum shows numerous S, O, S+, and O+ lines. A weak series of SO2 bands has also been tentatively identified. In addition, Balmer series lines are seen, which indicates charge-transfer ionization of the SO2 target. Preliminary absolute emission cross sections on the order of 10-18 cm2 have been measured for the most dominant line in the spectrum, an oxygen triplet at 777 nm. ¿ 2001 American Geophysical Union |
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Abstract |
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Keywords
Atmospheric Composition and Structure, Airglow and aurora, Atmospheric Composition and Structure, Planetary atmospheres (5405, 5407, 5409, 5704, 5705, 5707), Magnetospheric Physics, Auroral phenomena, Planetology, Solar System Objects, Jovian satellites |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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