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The mission also collected detailed information on the composition and structure of Mercury''s crust, its geologic history, the nature of its thin atmosphere and active magnetosphere, and the makeup of its
The challenges encountered during surface analysis, especially for phase composition identification, are briefly discussed. Further, a few selected recent applications of the XPS technique
The Mercury Atmospheric and Surface Composition Spectrometer (MASCS) is one of seven science instruments onboard the MErcury Surface, Space ENvironment, GEo-chemistry, and Ranging
It includes a quick technique selection guide for narrowing down suitable methods for obtaining a range of compositional, structural, and surface properties. Considerations and
It will measure altitude profiles of known species in order to determine the composition and structure of Mercury''s exosphere and its variability and will search for previously undetected
The Mercury Atmospheric and Surface Composition Spectrometer (MASCS) is comprised of a small Cassegrain telescope with a 257-mm effective focal length and a 50-mm aperture that
MASCS is the Mercury Atmospheric and Surface Composition Spectrometer instrument on MESSENGER. The data sets are produced by the MASCS Science Team at Johns Hopkins
This page discusses surface analytical techniques in spectroscopy, emphasizing surface sensitivity and the challenge of isolating surface signals from bulk signals.
It includes a quick technique selection guide for narrowing down suitable methods for obtaining a range of compositional, structural, and surface
The MESSENGER Mercury Atmospheric and Surface Composition Spectrometer (MASCS) instrument consists of an Ultraviolet-Visible Spectrometer (UVVS) and a Visible-Infrared Spectrograph (VIRS).