dc.contributor.author
Walter, S. H. G.
dc.contributor.author
Muller, J. P.
dc.contributor.author
Sidiropoulos, P.
dc.contributor.author
Tao, Y.
dc.contributor.author
Gwinner, K.
dc.contributor.author
Putri, A. R. D.
dc.contributor.author
Kim, J.-R.
dc.contributor.author
Steikert, R.
dc.contributor.author
Gasselt, S. van
dc.contributor.author
Michael, G. G.
dc.contributor.author
Watson, G.
dc.contributor.author
Schreiner, B. P.
dc.date.accessioned
2018-09-11T12:25:48Z
dc.date.available
2018-09-11T12:25:48Z
dc.identifier.uri
https://refubium.fu-berlin.de/handle/fub188/22830
dc.identifier.uri
http://dx.doi.org/10.17169/refubium-629
dc.description.abstract
Web‐based planetary image dissemination platforms usually show outline coverage of available data and offer querying for metadata as well as preview and download. While the usual form of presenting multiorbit data sets is to merge the data into a larger mosaic, for change detection purposes it is essential to maintain the individual images as an important snapshot of the planetary surface taken at a specific time. We introduce the web‐based interactive Mars Analysis and Research System (iMARS web‐GIS), which is specialized on planetary surface change analysis with novel tools for simultaneous visualization of single images as time series in their original sequence. As the data foundation, we use the vast quantity of automatically coregistered orthoimages and digital terrain models (DTM) from three NASA missions' instruments processed and ingested in the context of the EU‐funded iMars project. The baseline for the coregistered images are the High‐Resolution Stereo Camera (HRSC) multiorbit quadrangle image mosaics, which are based on bundle block‐adjusted multiorbit DTM mosaics. Additionally, we make use of the existing along‐track bundle‐adjusted HRSC single images and DTMs available at the planetary data archives. We provide two science cases for exemplary workflows of the multitemporal single‐image analysis, demonstrating the dedicated tools for surface change interpretation—one near Mawrth Vallis and one near the south pole. A web mapping application including the presented functionality has been implemented and is available at http://imars.planet.fu-berlin.de with the iMars project website (http://www.i-mars.eu/web-gis) serving as a mirror.
dc.format.extent
16 Seiten
de
dc.rights.uri
https://creativecommons.org/licenses/by-nc-nd/4.0/
de
dc.subject
surface changes
en
dc.subject
planetary mapping
en
dc.subject.ddc
000 Informatik, Informationswissenschaft, allgemeine Werke::000 Informatik, Wissen, Systeme::006 Spezielle Computerverfahren
de
dc.subject.ddc
500 Naturwissenschaften und Mathematik::550 Geowissenschaften, Geologie::551 Geologie, Hydrologie, Meteorologie
de
dc.subject.ddc
500 Naturwissenschaften und Mathematik::520 Astronomie::526 Mathematische Geografie
de
dc.title
The Web-Based Interactive Mars Analysis and Research System for HRSC and the iMars Project
de
dc.type
Wissenschaftlicher Artikel
de
dcterms.bibliographicCitation.doi
10.1029/2018EA000389
dcterms.bibliographicCitation.journaltitle
Earth and Space Science
dcterms.bibliographicCitation.url
https://doi.org/10.1029/2018EA000389
de
refubium.affiliation
Geowissenschaften
de
refubium.affiliation.other
Institut für Geologische Wissenschaften / Fachrichtung Geophysik
de
refubium.note.author
Der Artikel wurde in einer reinen Open-Access-Zeitschrift publiziert.
de
refubium.resourceType.isindependentpub
no
de
dcterms.accessRights.openaire
open access
dcterms.isPartOf.issn
2333-5084