Modelling the influence of surface emittance and atmospheric transmittance on Martian spectra

Advances in Space Research

Volumn 19, Issue 8, 1997, Pages 1281-1284

  Blecka, M I ^a   Blanco, A ^b   Fonti, S ^b   Muci, A M ^b   Orofino, V ^b  

^a Borowiec Astrogeodynamic Observatory   (Poland)

^b UNIVERSITY OF SALENTO   (Italy)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0001130129     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0273-1177(97)00283-4     Document Type: Article

References (8)

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4. Moroz V.I., M.N. Isakov, and V.M. Linkin, Engineering Model of the Martian Atmosphere, Preprint of IKI No 1449, Moscow (1988).
5. Pollack, J.B.,T. Roush, F. Witterborn, J. Bregman, D. Wooden et al., J. Geophys. Res., 95, NO.B9, 14.595 (1990).
6. Richter R., Model SENSAT-3 SENSOR-ATMOSPHERE-TARGET, DLR-IB 552-06/89 Institute for Optoelectronics D-8031 Wessling, (1991).
7. Roush, T., J. Pollack and J. Orenberg , Derivation of Midinfrared (5 - 25 μm) Optical Constants of Some Silicates and Palagonite, Icarus, 94, 191, (1991).
8. -1 (5 - 25 μm) of Hawaiian palagonitic soils and their implications for Mars, J. Geophys. Res., 100, NO. E3, 5309 (1995).