Nalazite se na CroRIS probnoj okolini. Ovdje evidentirani podaci neće biti pohranjeni u Informacijskom sustavu znanosti RH. Ako je ovo greška, CroRIS produkcijskoj okolini moguće je pristupi putem poveznice www.croris.hr
izvor podataka: crosbi

LU60645GT and MA132843GT catalogues of Lunar and Martian impact craters developed using a Crater Shape-based interpolation crater detection algorithm for topography data. (CROSBI ID 181168)

Prilog u časopisu | izvorni znanstveni rad | međunarodna recenzija

Salamunićcar, Goran ; Lončarić, Sven ; Mazarico, Erwan LU60645GT and MA132843GT catalogues of Lunar and Martian impact craters developed using a Crater Shape-based interpolation crater detection algorithm for topography data. // Planetary and space science, 60 (2012), 1; 236-247. doi: 10.1016/j.pss.2011.09.003

Podaci o odgovornosti

Salamunićcar, Goran ; Lončarić, Sven ; Mazarico, Erwan

engleski

LU60645GT and MA132843GT catalogues of Lunar and Martian impact craters developed using a Crater Shape-based interpolation crater detection algorithm for topography data.

For Mars, 57633 craters from the manually assembled catalogues and 72668 additional craters identified using several crater detection algorithms (CDAs) have been merged into the MA130301GT catalogue. By contrast, for the Moon the most complete previous catalogue contains only 14923 craters. Two recent missions provided higher-quality digital elevation maps (DEMs): SELENE (in 1/16° resolution) and Lunar Reconnaissance Orbiter (we used up to 1/512°). This was the main motivation for work on the new Crater Shape-based interpolation module which improves previous CDA as follows: (1) it decreases the number of false-detections for the required number of true detections ; (2) it improves detection capabilities for very small craters ; and (3) it provides more accurate automated measurements of craters' properties. The results are: (1) LU60645GT, which is currently the most complete (up to ~ D ≥ 8 km) catalogue of Lunar craters ; and (2) MA132843GT catalogue of Martian craters complete up to ~ D ≥ 2 km, which is the extension of the previous MA130301GT catalogue. As previously achieved for Mars, LU60645GT provides all properties that were provided by the previous Lunar catalogues, plus: (1) correlation between morphological descriptors from used catalogues ; (2) correlation between manually assigned attributes and automated measurements ; (3) average errors and their standard deviations for manually and automatically assigned attributes such as position coordinates, diameter, depth/diameter ratio, etc ; and (4) a review of positional accuracy of used datasets. Additionally, surface dating could potentially be improved with the exhaustiveness of this new catalogue. The accompanying results are: (1) the possibility of comparing a large number of Lunar and Martian craters, of e.g. depth/diameter ratio and 2D profiles ; (2) utilization of a method for re-projection of datasets and catalogues, which is very useful for craters that are very close to poles ; and (3) the extension of the previous framework for evaluation of CDAs with datasets and ground-truth catalogue for the Moon.

Moon; Mars; surface; cratering; iImage processing

nije evidentirano

nije evidentirano

nije evidentirano

nije evidentirano

nije evidentirano

nije evidentirano

Podaci o izdanju

60 (1)

2012.

236-247

objavljeno

0032-0633

10.1016/j.pss.2011.09.003

Povezanost rada

Elektrotehnika, Računarstvo

Poveznice
Indeksiranost