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Volumn 315, Issue 5814, 2007, Pages 983-985

Fracture-controlled paleo-fluid flow in Candor Chasma, Mars

Author keywords

[No Author keywords available]

Indexed keywords

BLEACHING; CEMENTATION; CHEMICAL ALTERATION; EXPERIMENTAL STUDY; FLUID FLOW; FRACTURE; IMAGING METHOD; MARS; WATER;

EID: 33847139794     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1136855     Document Type: Article
Times cited : (73)

References (24)
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    • For more information on HiRISE, see
    • For more information on HiRISE, see http://hirise.tpl. arizona.edu.
  • 3
    • 33847168781 scopus 로고    scopus 로고
    • N. E. Witbeck, K. L. Tanaka, D. H. Scott, Geologic Map of the Valles Marineris Region of Mars, scale 1:2,000,000, U.S. Geol. Surv. Misc. Geol. Invest. Map I-2010 (U.S. Geological Survey, Denver, CO, 1991).
    • N. E. Witbeck, K. L. Tanaka, D. H. Scott, Geologic Map of the Valles Marineris Region of Mars, scale 1:2,000,000, U.S. Geol. Surv. Misc. Geol. Invest. Map I-2010 (U.S. Geological Survey, Denver, CO, 1991).
  • 4
    • 33847109544 scopus 로고    scopus 로고
    • B. K. Lucchitta et al., Mors (Univ. of Arizona Press, Tucson, AZ, 1992), pp. 423-492.
    • B. K. Lucchitta et al., Mors (Univ. of Arizona Press, Tucson, AZ, 1992), pp. 423-492.
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  • 21
    • 20144363710 scopus 로고    scopus 로고
    • A. Gendrin et al., Science 307, 1587 (2005).
    • (2005) Science , vol.307 , pp. 1587
    • Gendrin, A.1
  • 22
    • 33847170758 scopus 로고    scopus 로고
    • Z. K. Shipton et al., Geological Storage of Carbon Dioxide (Geological Society of London, London, 2004), pp. 43-58.
    • Z. K. Shipton et al., Geological Storage of Carbon Dioxide (Geological Society of London, London, 2004), pp. 43-58.
  • 24
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    • We are grateful to the science, operations, and engineering teams of HiRISE and the MRO project, whose diligent efforts made this work possible. Comments by HiRISE team members and two anonymous reviewers are also appreciated. Portions of this work were conducted under contract with NASA, with additional support by a grant from NASA's Mars Data Analysis Program
    • We are grateful to the science, operations, and engineering teams of HiRISE and the MRO project, whose diligent efforts made this work possible. Comments by HiRISE team members and two anonymous reviewers are also appreciated. Portions of this work were conducted under contract with NASA, with additional support by a grant from NASA's Mars Data Analysis Program.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.