Scattering matrices of martian dust analogs at 488nm and 647nm

Author:

Dabrowska Dominika D.,Muñoz Olga,Moreno Fernando,Ramos José L.,Martínez-Frías Jesús,Wurm Gerhard

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference78 articles.

1. Allen, C.C., Morris, R.V., Lindstrom, D.J., Lindstrom, M.M., Lockwood, J.P., 1997. JSC Mars-1 – Martian regolith simulant. Lunar Planet. Sci. 28. p. 27.

2. Allen, C.C., et al., 1998. Martian regolith simulant JSC Mars-1. Lunar Planet. Sci. 29. p. 1690.

3. Banin, A., 1988. The soils of Mars. In: Drake, M.J., Greeley, R., McKay, G.A., Blanchard, D.P., Carr, M.H., Gooding, J., McKay, C.P., Spudis, P.D., Squyres, S.W. (Eds.), Mars Sample Return Science, pp. 35–36.

4. Laboratory investigations of Mars: Chemical and spectroscopic characteristics of a suite of clays as Mars soil analogs;Banin;Origins Life,1988

5. Banin, A., et al., 1988b. Constraining Mars soil mineralogical composition: Palagonite vs. iron enriched smectite clays. Lunar Planet. Sci. 19. p. 27.

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