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Volumn 307, Issue 5715, 2005, Pages 1594-1597

Olivine and pyroxene diversity in the crust of Mars

Author keywords

[No Author keywords available]

Indexed keywords

GEOLOGIC MODELS; HYDRATION; OBSERVATORIES; ROCKS; SPACECRAFT; WATER ABSORPTION;

EID: 14844364362     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.1109098     Document Type: Article
Times cited : (346)

References (28)
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    • note
    • The spectral index to map olivine is calculated from reduced, atmospherically corrected OMEGA data with the following formula: Index = [R1700/(0.1*R1020 + 0.1*R1210 + 0.4*R1330 + 0.4*R1470)], where R1700 is the reflectance at 1700 nanometers, R1020 is the reflectance at 1020 nanometers, and so on.
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    • note
    • J.F.M. acknowledges NASA support for this work. We thank the personnel involved in acquisition and reduction of Mars Express OMEGA data for their efforts.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.