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Volumn 27, Issue 1, 1976, Pages 25-50

Distribution of small channels on the Martian surface

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EID: 0002841919     PISSN: 00191035     EISSN: 10902643     Source Type: Journal    
DOI: 10.1016/0019-1035(76)90182-2     Document Type: Article
Times cited : (91)

References (32)
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  • 4
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    • Chapman1
  • 7
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    • Martian Cratering. 3. Theory of crater obliteration
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  • 10
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    • Mariner 9 ultraviolet spectrometer experiment: Photometry and topography of Mars
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    • Hord1    Barth2    Stewart3    Lane4
  • 14
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    • Lucchitta, B. (1973). Private communication.
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    • Masursky, H., and Granata, G. (1974). Private communication.
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    • Structural origin of large Martian channels
    • (1974) Icarus , vol.22 , pp. 371-384
    • Schumm1
  • 26
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    • Comparison of Earth and Mars as differentiated planets
    • (1974) Icarus , vol.22 , pp. 312-324
    • Siever1
  • 29
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    • Soderblom, L. A. (1974). Private communication.
  • 30
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    • Large scale obliquity variations on Mars
    • (1973) Science , vol.181 , pp. 260-262
    • Ward1
  • 32
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    • Size frequency distribution of Martian craters and relative age of light and dark terrains
    • (1972) Science , vol.175 , pp. 755-757
    • Woronow1    King2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.