Semi-automated crater depth measurements.

Cratering Image processing Mars Semi-automated crater depth measurements Surface

Journal

MethodsX
ISSN: 2215-0161
Titre abrégé: MethodsX
Pays: Netherlands
ID NLM: 101639829

Informations de publication

Date de publication:
2019
Historique:
received: 20 05 2019
accepted: 07 08 2019
entrez: 1 11 2019
pubmed: 2 11 2019
medline: 2 11 2019
Statut: epublish

Résumé

Impact cratering is a major process driving planetary landscape evolution. Statistics of craters spatial density is extensively used to date planetary surfaces. Their degradation state and morphometry are also key parameters to understand surface processes. To exploit the increasing coverage of digital terrain models (DEM) on Mars at high spatial resolution, we propose a semi-automated pipeline for crater depth measurement based on coupled optical images and DEM. From a craters map shapefile coupled with a co-registered DEM, we propose to measure crater depth as the difference between the 60

Identifiants

pubmed: 31667129
doi: 10.1016/j.mex.2019.08.007
pii: S2215-0161(19)30209-2
pmc: PMC6812331
doi:

Types de publication

Journal Article

Langues

eng

Pagination

2293-2304

Informations de copyright

© 2019 The Authors.

Auteurs

Sylvain Breton (S)

Université Lyon 1, France.

Cathy Quantin-Nataf (C)

Université Lyon 1, France.

Thomas Bodin (T)

Université Lyon 1, France.

Damien Loizeau (D)

Université Lyon 1, France.

Matthieu Volat (M)

Université Lyon 1, France.

Loic Lozac'h (L)

Université Lyon 1, France.

Classifications MeSH