Terrestrial analogues for lunar impact melt flows
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- 作者：C.D. Neisha ; b ; cneish@uwo.ca" class="auth_mail" title="E-mail the corresponding author ; C.W. Hamiltonc ; S.S. Hughesd ; S. Kobs Nawotniakd ; W.B. Garrye ; J.R. Skokf ; R.C. Elphicg ; E. Schaeferc ; L.M. Cartere ; J.L. Bandfieldh ; G.R. Osinskia ; b ; D. Limg ; i ; J.L. Heldmanng
- 关键词：Earth ; Impact processes ; Moon ; surface ; Radar observations ; Volcanism
- 刊名：Icarus
- 出版年：2017
- 出版时间：1 January 2017
- 年：2017
- 卷：281
- 期：Complete
- 页码：73-89
- 全文大小：7680 K
文摘
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Lunar impact melts are rough at the decimeter scale but smooth at meter scales.
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Physical properties of lunar impact melt flows differ from terrestrial lava flows.
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Differences in post-emplacement modification may explain this observation.
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Alternately, differences may relate to the melts’ unique emplacement conditions.