High temperature measurements of Mercury analog materials are extremely important. Temperature effects on the spectral characteristics might create „blind spots“ for visible and near infrared spectroscopy at the hot poles of Mercury. The thermal infrared shows much smaller and well defined temperature related effects – therefore MERTIS will not have any „blind spots“. The increased SNR means we can identify not only the general mineralogy but provide real petrological information.
MERTIS seeing Mercury for the first time in the TIR
2015 ; London, Grossbritannien
2015-04-01
Aufsatz (Konferenz)
Elektronische Ressource
Englisch
Mercury , emissivity , MERTIS
Power supply design for the Mercury thermal infrared spectrometer MERTIS
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