Physics
Scientific paper
Mar 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002georl..29e..18p&link_type=abstract
Geophysical Research Letters, Volume 29, Issue 5, pp. 18-1, CiteID 1074, DOI 10.1029/2001GL014127
Physics
20
Planetology: Solar System Objects: Jovian Satellites, Planetology: Fluid Planets: Magnetospheres (2756), Magnetospheric Physics: Energetic Particles, Trapped
Scientific paper
This paper gives the composition, energy spectra, and time variability of energetic ions measured just upstream of Europa. From 100 keV to 100 MeV, ion intensities vary by less than a factor of ~5 among Europa passes considered between 1997 and 2000. We use the data to estimate the radiation dose rate into Europa's surface for depths 0.01 mm - 1 m. We find that in a critical fraction of the upper layer on Europa's trailing hemisphere, energetic electrons are the principal agent for radiolysis, and their bremsstrahlung photon products, not included in previous studies, dominate the dose below about 1 m. Because ion bombardment is more uniform across Europa's surface, the radiation dose on the leading hemisphere is dominated by the proton flux. Differences exist between this calculation and published doses based on the E4 wake pass. For instance, proton doses presented here are much greater below 1 mm.
Cohen Charon
Johnson Robert E.
Mauk Barry H.
Paranicas Chris
Ratliff J. M.
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