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Data From 'The Surface Roughness Of Mercury From The Mercury Laser Altimeter: Investigating The Effects Of Volcanism, Tectonism, And Impact Cratering'

descriptionPublicationkeyboard_double_arrow_right Article 31 May 2017Publisher:Zenodo
Authors: Susorney, H.C.M.; Barnouin, O.S.; Ernst, C.M.; Byrne, P.K.;

doi: 10.5281/zenodo.801573 , 10.5281/zenodo.801574

Data From 'The Surface Roughness Of Mercury From The Mercury Laser Altimeter: Investigating The Effects Of Volcanism, Tectonism, And Impact Cratering'

Abstract

ASCII files of the surface roughness of Mercury generated for Susorney et al., [2017]. The data format is 3 column comma separated values in the order of longitude, latitude, and delta_h. The first number in the file name is the baseline in kilometers the surface roughness was measured at. This data was used to generate all maps and deviograms in the paper.

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Keywords

MESSENGER, Mercury, Surface Roughness, Planetary Science

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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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