Io's 5 micron variability

Details Io's 5 micron variability Io's 5 micron variability

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...235l..49s&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 235, Jan. 1, 1980, p. L49-L51.

Astronomy and Astrophysics

Astronomy

8

Astronomical Photometry, Infrared Astronomy, Io, Planetary Radiation, Albedo, Instrument Errors, Statistical Analysis, Jupiter, Satellites, Io, Photometry, Flux, Observations, Data, Radiation, Ganymede, Callisto, Geometry, Albedo, Infrared, Statistical Analysis, Time Dependency

Scientific paper

An outburst of Io, similar to that observed by Witteborn, Bregman, and Pollack, has been observed with M filter-band photometry. At the beginning of observing on 1979 June 11 (UT) the flux was about 3 times its normal value and decayed approximately linearly with time by 23% in the first hour of observing. The beginning of observations followed the emergence of Io from eclipse by 1.5 hours.

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