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Hypotheses for the Origin of the Hypanis Fan-Shaped Deposit at the Edge of the Chryse Escarpment, Mars: Is it a Delta?
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2018-05
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2018-08-17
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Mars
surface
Geological processes
surface
Geological processes
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Jacob B. Adler, James F. Bell, Peter Fawdon, Joel Davis,Nicholas H. Warner, Eliott Sefton-Nash, Tanya N. Harrison, Hypotheses for the Origin of the Hy-panis Fan-Shaped Deposit at the Edge of the Chryse Escarpment, Mars: Is it a Delta?, Icarus (2018),doi: 10.1016/j.icarus.2018.05.021
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© 2018 The Authors. Published by Elsevier Inc. Open Access funded by Science and Technology Facilities Council. Published under a Creative Commons license. This is a PDF file of an unedited manuscript that has been accepted for publication. As a service to our customers we are providing this early version of the manuscript. The manuscript will undergo copyediting, typesetting, and review of the resulting proof before it is published in its final form. Please note that during the production process errors may be discovered which could affect the content, and all legal disclaimers that apply to the journal pertain.
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0019-1035