The original software is from Brown University (http://www.planetary.brown.edu/mgm/)
The original repository is from Chip Legett (https://github.com/clegett/mgm)
This directory contains the MGM Matlab code from its original source.
This directory contains a few python scripts to generate the startup and asc files needed as input to MGM.
: [directory name; this is for mac, unix would be "/."]
exampledata [ascii file]
-220,50,50 [ymin, ymax, yint for plots]
300,2600,300 [xmin, xmax, xint for plots]
2E-03,1E-06 [stopping criteria, absolute, relative errors]
Q [Polynomial type, Q/T is straight/tangent line in energy]
0.85E+00 -0.1E-05 0.0E+00 0.0E+00 [starting continuum]
10.0 0.1E-03 0.1E-06 0.1E-06 [2 sigma uncertainies on above]
3 [number of bands]
0.3330E+03 0.400E+03 -0.20E+02 [starting center, width, strength]
10000.0 10000.0 100.0 [2 sigma uncertainies on above]
0.1000E+04 0.250E+03 -0.1E+01 [starting center, width, strength]
200.0 400.0 10.0 [2 sigma uncertainies on above]
0.2000E+04 0.300E+03 -0.1E+01 [starting center, width, strength]
300.0 400.0 10.0 [2 sigma uncertainies on above]
[1] Sunshine et al., 1990. Deconvolution of mineral absorption bands: An improved approach. Journal of Geophysical Research: Solid Earth, 95(B5), 6955-6966.
[2] Sunshine & Pieters, 1993. Estimating modal abundances from the spectra of natural and laboratory pyroxene mixtures using the modified Gaussian model. Journal of Geophysical Research: Planets, 98(E5), 9075-9087.
[3] Sunshine et al., 1999. Absorption Band Modeling in Reflectance Spectra: Availability of the Modified Gaussian Model. 30th Lunar and Planetary Science Conference, Abstract #1306.