New morphometric data for fresh lunar craters
WebA model that provides a reference cone shape for fresh lunar craters is developed which can be used to compute volumetric differences between observed and reference shapes. … WebMorphometric relations have been determined for 2598 fresh craters on the lunar nearside using data given in the catalog of Wood and Andersson (1978). For each of five …
New morphometric data for fresh lunar craters
Did you know?
WebIn this research we are proposing an innovative method to determine and quantify the morphology of a simple fresh impact crater. Linné is a well preserved impact crater of … Web开馆时间:周一至周日7:00-22:30 周五 7:00-12:00; 我的图书馆
Web29 dec. 2024 · Lunar impact craters are important for studying lunar surface morphology because they are the most typical morphological units of the Moon. Impact crater … http://www.dlyj.ac.cn/EN/10.11821/dlyj201406001
WebThe presence of rocks in the ejecta of craters at the InSight landing site in southwestern Elysium Planitia indicates a strong, rock-producing unit at depth. A finer regolith above is … WebResults. The Tei index decreased 1 day after CRT (left ventricle [LV]: P < . 001, right ventricle [RV]: P = .01) and remained lower at follow-up (LV and RV: P < .001 vs baseline). Responders had a higher LV Tei index at baseline (P = .003) and achieved a sustained improvement in Tei index at follow-up (LV: P < .001, RV: P = .002) in contrast with …
WebThe article was published on 2009-03-01 and is currently open access. It has received 10 citation(s) till now. The article focuses on the topic(s): Mars Exploration Program & Impact crater.
WebThe SEIS (Seismic Experiment for Interior Structure) instrument onboard the InSight mission will be the first seismometer directly deployed on the surface of Mars. From studies on the Earth and the Moon, it is well known that site amplification in low-velocity sediments on top of more competent rocks has a strong influence on seismic signals, but can also be used … the hope trust edinburghWebAlthough wall failure does not occur until the crater diameter reaches 13 km, central peaks are found in flat floor craters as small as 2 km. Morphometric relations have been … the hope truckWeb23 mei 2016 · Using data from the LAMP instrument aboard the Lunar Reconnaissance Orbiter, ... Using data from the LAMP instrument aboard the Lunar Reconnaissance … the hope trust sunningdaleWebTitle: New morphometric data for fresh lunar craters Authors: Wood, C. A. & Anderson, L. Journal: In: Lunar and Planetary Science Conference, 9th, Houston, Tex., March 13 … the hope trustWebfresh simple crater. Morphometric analysis, conducted on recent high resolution DTM from LROC (NASA), quantitatively confirmed the pristine morphology of the crater, revealing … the hope trust scotlandWebDeriving Morphometric Parameters and the Simple-to-Complex Transition Diameter From a High-Resolution, Global Database of Fresh Lunar Impact Craters (D ≥ ... We compiled a high-resolution, global lunar impact crater database composed of 5,505 pristine craters ≥ ~3 km. This database contains detailed morphometri... T. KrügerS. HergartenT. the hope unit buryWebIn this study we have applied 3D morphometric analysis of impact craters on the Moon by means of high resolution DTMs derived from LROC (Lunar Reconnaissance Orbiter … the hope tv