Wallis, D. and McBride, N.
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We describe a new project to obtain a global characterisation of Martian impact crater morphology from the 1/16 degree MOLA topography dataset. A new mathematical method applicable to both symmetric and asymmetric craters is used.
|Item Type:||Conference Item|
|Extra Information:||Abstract #1692|
|Academic Unit/Department:||Science > Physical Sciences
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Kyra Proctor|
|Date Deposited:||20 Jul 2007|
|Last Modified:||23 Feb 2016 18:00|
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