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Volumn 323, Issue 5917, 2009, Pages 1041-1045

Strong release of methane on Mars in northern summer 2003

Author keywords

[No Author keywords available]

Indexed keywords

HYDROCARBON; METHANE; PERCHLORATE; SULFATE;

EID: 60949103904     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1165243     Document Type: Article
Times cited : (525)

References (47)
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    • We binned spectra over 46° of longitude (centered at CML 300°) for Fig. 1, B and C (and Fig. 2, A and B), but over only 16° for Fig. 2C. Profile d is centered at CML 310°, leading to lower mean mixing ratios in Fig. 2B as compared with Fig. 2C (profile d). See detailed map in Fig. 3.
    • We binned spectra over 46° of longitude (centered at CML 300°) for Fig. 1, B and C (and Fig. 2, A and B), but over only 16° for Fig. 2C. Profile d is centered at CML 310°, leading to lower mean mixing ratios in Fig. 2B as compared with Fig. 2C (profile d). See detailed map in Fig. 3.
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    • We thank T. C. Onstott and L. M. Pratt for helpful comments and two anonymous referees for their comments and suggestions. This work was supported by NASA [the Planetary Astronomy Program (RTOP 344-32-07 to M.J.M, Astrobiology Institute (RTOP 344-53-51, to M.J.M, and Postdoctoral Program (G.L.V, and by NSF (Research at Undergraduate Institutions Program AST-0505765 to R.E.N, We thank the director and staff of NASA's InfraRed Telescope Facility (operated for NASA by the University of Hawaii) for exceptional support throughout our long Mars observing program. Data were also obtained at the W. M. Keck Observatory, operated as a scientific partnership by CalTech, the University of California Los Angeles, and NASA
    • We thank T. C. Onstott and L. M. Pratt for helpful comments and two anonymous referees for their comments and suggestions. This work was supported by NASA [the Planetary Astronomy Program (RTOP 344-32-07 to M.J.M), Astrobiology Institute (RTOP 344-53-51, to M.J.M), and Postdoctoral Program (G.L.V.)] and by NSF (Research at Undergraduate Institutions Program AST-0505765 to R.E.N.). We thank the director and staff of NASA's InfraRed Telescope Facility (operated for NASA by the University of Hawaii) for exceptional support throughout our long Mars observing program. Data were also obtained at the W. M. Keck Observatory, operated as a scientific partnership by CalTech, the University of California Los Angeles, and NASA.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.