dc.contributor.author
Neu, Dominik
dc.contributor.author
Schreiner, Björn
dc.contributor.other
Walter, Sebastian
dc.date.accessioned
2024-01-22T11:16:34Z
dc.date.available
2024-01-22T11:16:34Z
dc.identifier.uri
https://refubium.fu-berlin.de/handle/fub188/42039
dc.identifier.uri
http://dx.doi.org/10.17169/refubium-41764
dc.description.abstract
The Noctis Labyrinthus region (Latin for “labyrinth of night”) is located between the western edge of Valles Marineris and the Tharsis upland. It has a length of 1,190 km and is characterized by a system of deep and steep-walled valleys formed by faulting. Many of the valleys show the classical appearance of so-called graben. We feature an image mosaic which consists of 8 high-definition images from the HRSC camera with a resolution of 12.5 m per pixel. We also provide a Digital Terrain Model of the area in 100 m per pixel, which has been constructed from the same HRSC orbits.
en
dc.publisher
Freie Universität Berlin
dc.rights.uri
https://creativecommons.org/licenses/by/4.0/
dc.subject
Noctis Labyrinthus
en
dc.subject
Mars Express
en
dc.subject.ddc
500 Natural sciences and mathematics::520 Astronomy and allied sciences::523 Specific celestial bodies and phenomena
dc.title
Noctis Labyrinthus HRSC image mosaic and DTM
dcterms.spatial
Noctis Labyrinthus
dc.contributor.type
data_collector
dc.coverage.pointLatitude
-7
dc.coverage.pointLongitude
265 E
dc.title.subtitle
Mosaic from 8 HRSC orbits (0442, 1085, 1944, 1977, 1988, 10497, 14632, 16684)
refubium.affiliation
Geowissenschaften
refubium.affiliation.other
Planetary sciences and remote sensing
refubium.affiliation.other
Institut für Geologische Wissenschaften / Fachrichtung Planetologie und Fernerkundung
refubium.funding.funder
other
dcterms.accessRights.openaire
open access
