Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007dps....39.0407m&link_type=abstract
American Astronomical Society, DPS meeting #39, #4.07; Bulletin of the American Astronomical Society, Vol. 39, p.414
Astronomy and Astrophysics
Astronomy
Scientific paper
A transient event in Cassini UVIS imaging of atomic hydrogen in the Saturn magnetosphere has been found in pre-SOI exposures obtained on May 18, 2004. The event occurred at 2.7 ± 0.2 RS in the orbital plane on the subsolar side of the planet in the 1.5 hour interval between exposures, and decayed inside the 17 hour interval to the next exposure. The time scale indicates that the gas was produced well above the escape velocity (0.6 eV/atom). Atomic oxygen in the magnetosphere also shows variability in abundance, but measurement time-scale is limited to a minimum to 2 weeks, compared to hours for the measurement of atomic hydrogen. The brightness of the flash object is estimated at 300 R in H Lya, compared to 1000 R for the Saturn dayglow. The FWHM latitudinal size of the feature is 0.8 RS(pixel size 0.38 RS ) with a density of 2500 atoms cm-3. The total population in the exposure is estimated to be 6 X 1032 atoms (total of 2. X 1035 magnetospheric H atoms). Enceladus has been assumed to be the major source of oxygen in the magnetosphere based on measurements of the recently discovered plume. The source of atomic hydrogen is evidently more complicated, showing evidence that the Saturn atmosphere delivers most of the broadly distributed HI in the magnetosphere. The Cassini UVIS images, however, show a persistent narrow HI torus near 3 RS above the broad background, where the flash reported here is located. The OI in UVIS images is in an irregular asymmetric distribution showing peak emissions positioned from 2 to 4 RS depending on time of observation. The properties of these features indicate Enceladus is not the only strong source of neutral gas in the magnetosphere.
This work is supported by the Cassini Program.
Melin Henrik
Shemansky Donald
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