MESSENGER X-Ray Spectrometer Detection of Electron-Induced X-Ray Fluorescence from Mercury's Surface

Details MESSENGER X-Ray Spectrometer Detection of Electron-Induced X-Ray Fluorescence from Mercury's Surface MESSENGER X-Ray Spectrometer Detection of Electron-Induced X-Ray Fluorescence from Mercury's Surface

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1176s&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1176

Computer Science

Scientific paper

X-ray emissions observed from the dark side of Mercury are the result of
~1-10 keV electrons impinging on the planet’s surface.
Knowledge of the precipitating electron distribution makes it possible
to infer surface composition from the measured fluorescent spectra.

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