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Best-Fit Biaxial Ellipsoid Shape of (4) Vesta, Crater Detection from Digital Topography and Comparison with Martian, Lunar and Mercurian Craters (CROSBI ID 608442)

Prilog sa skupa u zborniku | sažetak izlaganja sa skupa | međunarodna recenzija

Salamunićcar, Goran Best-Fit Biaxial Ellipsoid Shape of (4) Vesta, Crater Detection from Digital Topography and Comparison with Martian, Lunar and Mercurian Craters // 45th Annual Lunar and Planetary Science Conference. The Woodlands (TX), 2014

Podaci o odgovornosti

Salamunićcar, Goran

engleski

Best-Fit Biaxial Ellipsoid Shape of (4) Vesta, Crater Detection from Digital Topography and Comparison with Martian, Lunar and Mercurian Craters

Based on the entire digital topography, the best-fit biaxial ellipsoid was determined. Using a crater detection algorithm (CDA), the catalogue with 8749 craters was created. Additionally, craters were compared with Martian, Lunar, and Mercurian craters.

Crater Detection Algorithm; Vesta

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Podaci o prilogu

2014.

objavljeno

Podaci o matičnoj publikaciji

45th Annual Lunar and Planetary Science Conference

The Woodlands (TX):

Podaci o skupu

45th Annual Lunar and Planetary Science Conference – 45th LPSC

ostalo

17.03.2014-21.03.2014

The Woodlands (TX), Sjedinjene Američke Države

Povezanost rada

Računarstvo

Poveznice