يعرض 1 - 4 نتائج من 4 نتيجة بحث عن '"crater size-frequency distribution (CSFD)"', وقت الاستعلام: 1.10s تنقيح النتائج
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    دورية أكاديمية
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    دورية أكاديمية

    المصدر: Remote Sensing; Volume 14; Issue 1; Pages: 49

    وصف الملف: application/pdf

    العلاقة: Satellite Missions for Earth and Planetary Exploration; https://dx.doi.org/10.3390/rs14010049Test

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    العلاقة: * The shapefiles of our count areas and the crater measurements are available in Oetting (2023, https://doi.org/10.35003/V9AFAZTest). * The LROC NAC images were obtained from the Planetary Data Systems (Robinson, 2011) and downloaded from https://ode.rsl.wustl.edu/moonTest/. * NAC DTMs (Henriksen et al., 2017) were taken from https://wms.lroc.asu.edu/lroc/rdr_product_selectTest. * The Clementine ultraviolet-visible color ratio composite map of Lucey et al. (2000) was obtained from https://astrogeology.usgs.gov/search/map/Moon/Clementine/UVVIS/Lunar_Clementine_UVVIS_Warp_ClrRatio_Global_200mTest. * To assess the potential for seismic activity from nearby lobate scarps, we used Quickmap (quickmap.lroc.asu.edu) lobate-scarp map (Nelson et al., 2014). * The algorithm from Clauset et al. (2009) for calculating the CSFD slope and its uncertainties is available at https://aaronclauset.github.io/powerlawsTest/.; https://doi.org/10.35003/YSPCHCTest

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