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Supplemental Data: Mg-Fe olivine emissivity spectra

Hamilton, V.E. (2010) Thermal infrared (vibrational) spectroscopy of
Mg-Fe olivines: A review and applications to determining the
composition of planetary surfaces, Chemie der Erde, 70,doi:10.1016/
j.chemer.2009.12.005.


These data accompany the above referenced paper and include emissivity spectra of intermediate olivine compositions in the Mg-Fe series. Additionally, these spectra, and emissivity spectra of end member compositions (forsterite and fayalite), may be found in the Arizona State University spectral library.

The file linked below is in space-delimited ascii format. The header contains a citation to the original publication in which the spectra are documented and analyzed. Data are arranged as columns, with the first column being the x-axis in wavenumbers (cm-1) and subsequent columns being the emissivities of the olivine compositions in the order listed at the top of the file. Please refer to Hamilton [2010] for information on sample chemistry and the collection, calibration, and subsequent processing of the emissivity spectra. Additional information about the spectra may also be found in Koeppen and Hamilton [2008], and chemical information also is available in Morse [1996].

Data: Hamilton_CdE2010_Mg-Fe_olivines.txt


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page last updated: 8 June 2010