Optimal Wavelengths for Studying Thermal Emission from Active Volcanoes on Io

Details Optimal Wavelengths for Studying Thermal Emission from Active Volcanoes on Io Optimal Wavelengths for Studying Thermal Emission from Active Volcanoes on Io

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.1943k&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

Physics

1

Scientific paper

Eruption temperature of Io lavas can be constrained by new observations
at ~0.8 and ~1 microns. Eruption style and heat flow are best studied at
2, 3, 4, 6, 8, 15, and 20 microns with 2, 5, and 8 microns being the
most essential.

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