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34 results for “impact craters”
Impact crater identification results for Chang'e-4 satellite image area and landing camera image area
<p>Here are the results of impact crater identification from Chang'e-4 satellite image data and Chang'e-4 landing camera image data.</p> <p>There are 99 impact craters identified in the landing camera, with diameters ranging from 1.55m to 50.87m.There are 947 impact craters identified in the satellite images, with diameters ranging from 48.37m to 2,222.34m in diameter.</p> <p>All impact craters are categorised into five degradation classes (A, AB, B, BC, C).</p> <p>Landing camera image source: <a href="https://doi.org/10.5281/zenodo.3600427" target="_blank" rel="noopener noreferrer">https://doi.org/10.5281/zenodo.3600427</a><br>Satellite image source: <span>https://darts.isas.jaxa.jp/planet/pdap/selene/index.html.en</span></p> <p> </p>
The dataset for the paper "Ambient noise tomography reveals asymmetric impact damage zone beneath Lonar crater, India: Implications for oblique impact cratering in heterogeneous basalt with planetary applications"
<p>These datasets are used to produce the results and generate figures and tables in the manuscript titled as "Ambient Noise Tomography Reveals Asymmetric Impact Damage Zone Beneath Lonar Crater, India: Implications for Oblique Impact Cratering in Heterogeneous Basalt with Planetary Applications" submitted to JGR-Planets.</p>
Unveiling Surface and Near-Surface Properties of Inner Solar System Bodies Through Impact Cratering: Datasets
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Data from "Impact-induced hydrothermal conditions in complex craters on Mars"
<p>Supplementary materials for the paper "Impact-induced hydrothermal conditions in complex craters on Mars". It includes iSALE input files for simulations presented in Figures 1, 2, 5, S1, S2, S3, and S4. It also includes select data processing and plotting files. Refer to readme.txt file for instructions.</p>
The production population of impact craters in the Chang'E-6 landing mare
<p>The uploaded file contains the statistical results from various regions within the Chang'E-6 landing mare for the manuscript titled "The Production Population of Impact Craters in the Chang'E-6 Landing Mare" . The data included in this file directly supports the statistical analysis and conclusions presented in the manuscript. The results were exported using CraterTools in ArcGIS and are provided in an SCC file format, which contains information of both the defined counting areas and the collected craters. These SCC files can be used to construct crater size-frequency distributions of production populations on the Chang'E-6 landing mare, thereby assisting in the study of the evolution history of local crater populations.</p>
Dataset for "Mars' axial and reversing dynamo recorded in a magnetized impact crater 4.2 billion years ago"
<p>This dataset is for the research titled "<em><strong>Mars’ axial and reversing dynamo recorded in a magnetized impact crater 4.2 billion years ago</strong></em>".</p> <ul> <li>Please ensure that all files are placed in the same directory</li> <li><strong>ESD.m</strong> contains all the procedures needed to invert crustal magnetization from crustal magnetic field data. </li> <li>The remaining files are crustal magnetic field datasets generated by IDL, which are used as input for <strong>ESD.m</strong>.</li> <li>For MATLAB users, it is necessary to install the <strong><em>restore_idl</em></strong> package to read these IDL-generated files within MATLAB.</li> </ul> <p>Don't hesitate to email me (jfqin@berkeley.edu) if you have any trouble running this code.</p>
Online Repository for One-dimensional Power Spectral Analysis of Fresh Lunar Impact Craters
<p>This dataset includes:</p> <p>(1) Shape files of the rim crest, floor, and rim flank outlines of our selected fresh lunar craters.</p> <p>(2) Power spectral densities of the rim crest, floor, and rim flank outlines of our selected fresh lunar craters.</p> <p>(3) Python scripts to generate synthetic fresh lunar craters.</p> <p>(4) A spreadsheet that contains the morphometric parameters and the breakpoints (wavelengths and powers).</p>
A Global Catalog of Martian Impact Craters with Actual Boundaries and Degradation Degrees
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Dataset:Ray and Halo impact craters on Ganymede : fingerprint for decoding Ganymede´s crustal structure
<p>The geological basemap used in the study is from Kersten et al., 2021. </p>
"Onset of post-cratering melting of target rocks at the impact melt contact: observations from the Vredefort impact structure, South Africa" µCT data
<p>µCT Dataset. </p>
Datasets for the Icarus paper "Evidence for trail forming ejecta boulder falls around fresh simple impact craters at the lunar Orientale multi-ring basin and implications for ballistic ejecta sedimentation"
<p>This dataset has been used to prepare some figures in our Icarus paper. </p>
Measurements of Pits and Impact Craters of the Cauchy 5 Small Shield Volcano
<p><strong>This page archives data used in the following article:</strong></p> <p><strong>Qiao, L., Head, J. W., Wilson, L., & Ling, Z. (2020). The Cauchy 5 Small, Low-Volume Lunar Shield Volcano: Evidence for Volatile Exsolution-Eruption Patterns and Type 1/Type 2 Hybrid Irregular Mare Patch (IMP) Formation. <em>Journal of Geophysical Research: Planets</em>, 125, e2019JE006171. <a href="https://doi.org/10.1029/2019JE006171" target="_blank" rel="noopener">https://doi.org/10.1029/2019JE006171</a></strong></p> <p><strong>It includes measurements of pits on Cauchy 5 small shield volcano north flank (Sheet “Pits_NorthFlank”) and SE rim (Sheet “Pits_NE-Rim”), and superposed impact craters on shield flank (Sheet “Craters_Flank”), smaller surrounding mare region (Sheet “Craters_Mare_Small”), and larger surrounding mare region (Sheet “Craters_Mare_Large”).</strong></p>
A Global Catalog of Martian Impact Craters with Actual Boundaries and Degradation Degrees
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LU3M7TGT: An AI-Powered Global Database of impact craters >=0.5 km on the Moon.
<p>Release of a new global craters catalog (<strong>LU3M7TGT</strong>) with more than 3.7 million craters (>=0.5 km in diameter)</p> <ul> <li><em>File source csv</em></li> <li><em>Header: Longitude, Latitude, Diameter_w, Diameter_h, Confidence, WindowMinLon, WindowMaxLon, WindowMinLat, WindowMaxLat.</em></li> <li><em>The coordinates are absolute in the range of [-180, +180] of Longitude and [-90, +90] of Latitude. All coordinates are expressed in <strong>cylindrical projection system</strong>.</em></li> <li><em>Diameters (km)</em></li> </ul>
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International Brain Laboratory public data
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OpenNeuro
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