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270 results for “crater”
raw crater counts for radial ejecta craters
<p>JMARS .jlf shape files that contain the measurement area polygon and crater measurements (diameters, center lat/lon, and a degradation classification). And .csv files of crater measurements. Names of files indicate the region for the counts. See associated publication for descriptions of those regions.</p>
Ariel and Miranda Crater Counts
<p>JMARS files containing the study area outlines and crater counts for Ariel and Miranda to accompany the paper "Simple-to-complex crater transition for the Uranian satellites Ariel and Miranda". The crater coordinates, simple/complex categorizations, and R calculations are also included as an excel file.</p>
HiRISE-generated DTMs over Sakarya Vallis in Gale crater, Mars
<p>HiRISE-generated DTMs over Sakarya Vallis in Gale crater, Mars. Produced at the University of Chicago by David P. Mayer. </p>
The crater detection results (necessary data for making Figs 6 and 7) for areas A2, A4 and A7 to estimate the ages of RMDS-overlapped craters in Figs 2a-2c
<p>To estimate the ages of RMDS-overlapped craters in Figs 2a-2c ( located in areas A2, A4 and A7, respectively) with a locally calibrated Monte Carlo model, the NAC-DEM-based crater detection results are provided here, as the basis input and necessary data to make Figs 6 and 7.</p> <p>They have been introduced in the following publication, where more details can be found:</p> <p>F. Zhang, J. W. Head, C. Wöhler, A. T. Basilevsky, L. Wilson, M. Xie, R. Bugiolacchi, T. Wilhelm, S. Althoff, Y. L. Zou.</p> <p>The Lunar Mare Ring-Moat Dome Structure (RMDS) Age Conundrum: Contemporaneous with Imbrian-Aged Host Lava Flows or Emplaced in the Copernican?</p> <p>Journal of Geophysical Research: Planets, 126, e2021JE006880. https://doi. org/10.1029/2021JE006880</p>
Chang'e-5 Mare Unit and Crater Catalogue
<p><strong>This page archives data used in the following article:<br>Qiao, L., Xu, L., Yang, Y., Xie, M., Chen, J., Fang, K., & Ling, Z. (2021). Cratering Records in the Chang’e-5 Mare Unit: Filling the "Age Gap" of the Lunar Crater Chronology and Preparation for its Re-calibration. <em>Geophysical Research Letters</em>, 48, e2021GL095132. <a href="https://doi.org/10.1029/2021GL095132" target="_blank" rel="noopener">https://doi.org/10.1029/2021GL095132</a></strong></p> <p><strong>They include files of the Chang'e-5 mare unit and crater catalogue:</strong></p> <p><strong>Chang'e-5_Mare.7z: ArcGIS shapefile for the mare unit;</strong></p> <p><strong>Chang'e-5_Crater.7z: ArcGIS shapefile for the crater catalogue;</strong></p> <p><strong>Chang'e-5_Crater.txt: text file for the crater catalogue.</strong></p>
Data for Chandnani and Herrick, Influence of Target Properties on Wall Slumping in Lunar Impact Craters within the Simple-to-Complex Transition
<p>Data files for Figures 3 and S1 of the manuscript. These are craters counted in slump and ejecta units for the purpose of comparing their relative ages.</p> <p>The directory sf_shapefiles contains subdirectories for the 20 craters for which a slump unit and an ejecta unit had crater counts performed. The AREA_* shapefiles are polygons that outline the area studied, and the CRATER_* files are the individual craters counted. These files were created using CraterTools (<a href="https://www.geo.fu-berlin.de/en/geol/fachrichtungen/planet/software/_content/software/index.html">https://www.geo.fu-berlin.de/en/geol/fachrichtungen/planet/software/_content/software/index.html</a>) in ArcGIS, but that software is not necessary to use the shapefiles. </p> <p>The subdirectory SFD_figs_color and SFC_suppl_figs_color are, respectively, the CraterStats (https://www.geo.fu-berlin.de/en/geol/fachrichtungen/planet/software/_content/software/index.html) files used to generate Figure 3 of the main manuscript and Supplemental Figure S1. Each crater comprises a subdirectory of those main directories. Within each subdirectory, the *.plt file is the file directing CraterStats how to make the figure. The *.png file is the output figure from CraterStats, and the *.jpg file is the .png file after it has been cropped and the error bars have been changed from grey to black. The *.txt file provides the output from CraterStats that, among other things, provides the data fit of isochrons to the data. The *.diam files are data extracted from the shapefiles and provide the input into Craterstats. They have the lat-lon-diameter information on the craters and the counting area. All of these are commented text files, so you don’t need CraterStats to look at them and use them.</p>
Seismic efficiency and seismic moment for small craters on Mars formed in layered uppermost crust
<p>Input files used in the paper submitted to JGR: Planets, November 2022.</p> <p>Table with location and sizes of all mapped craters.</p>
Measurement of the fumarole temperature of the north eastern crater rim of Vesuvius -----Long-term variations of fumarole temperature of the north eastern crater rim of Vesuvius (Italy)
<pre>Measurements of the fumarole temperature of the north eastern edge of Vesuvius have been carried out since 1995. The temperature is measured at a depth of 10 cm using a K-type thermocouple. The coordinate of the fumarole is 33T 451833.1m E - 4519224.8m N.</pre> <pre>The monitored fumarole is the one at the highest altitude present on Vesuvius </pre> <p>The fumarole is characterized by low temperatures (59.5 - 75.6 ˚C) and discharge a mixture of air (46% -72%), steam (25% -45%) and CO2 (0.2% -2%). The air is the main component of fumarole, is most likely included in the upper fluids part of the fumarolic ducts found in the highly permeable products of the Vesuvian cone. </p>
Data for "Formation of topographic benches and noses from the exhumation of crater-filling alluvial strata on Mars"
<p>Numerical model, batch scripts, experiment parameters, and results used for the publication "Formation of topographic benches and noses from the exhumation of crater-filling alluvial strata on Mars".</p>
supplementary data for Bemelmans et al., 2023, High-resolution InSAR reveals localised pre-eruptive deformation inside the crater of Agung volcano, Indonesia.
<p>This repository contains the supplementary materials for the paper "High-resolution InSAR reveals localised pre-eruptive deformation inside the crater of Agung volcano, Indonesia." to be published in JGR: Solid Earth.</p> <p>The dataset contains files assiciated with the StaMPS time series processing. Each dataset has its own folder containing:</p> <ol> <li>*_data.csv : data file containing latitude, longitude, incidence angle, heading and LOS displacement for each acquistion (date is listed in the column name in the format yyyymmdd).</li> <li>parms.mat : parameter file used for StaMPS processing of that dataset</li> </ol> <p>The dataset also contains input and results from the GBIS modelling (/GBIS_results/). the *.inp files are the input files for each model inversion where the letter ('M','T','P','Y', or 'D') refer to the Mogi (point), McTigue (sphere), penny-shaped crack, Yang (ellipsoid), and dyke (also sill) model used for that run. folders with the same name as the *.inp file contain the inversion results (invert_*.mat), a summary table (summary_*.txt) and several figures showing the distribution and convergence of the model inversion.</p> <p>The input for the GBIS inversions is stored in /GBIS_results/INSAR_input/</p> <p>the file <a href="https://zenodo.org/api/files/f30be116-1e2f-4d52-8fcf-a54e11ab691f/matlab_functions.zip?versionId=490de786-f245-45b5-92bb-d2ae0d50be56">matlab_functions.zip </a>contains matlab functions used for data processing, visualisation, storage and conversion.</p> <p>the file <a href="https://zenodo.org/api/files/f30be116-1e2f-4d52-8fcf-a54e11ab691f/GBISv1_1_MJWB.zip?versionId=cec83c81-a0b7-4e4a-8aa8-ac81e32b8772">GBISv1_1_MJWB.zip </a>contains GBIS code adapted by the author to perform statistical analysis of the model inversion, perform region-of-interest based subsampling and store modeled results as shapefiles for further processing.</p> <p> </p>
Phenomenological images (CL-CAM1B) of Crater Lake CALM site, Deception island, Antarctica (2021).
<p>Images acquired by a phenomenological automatic time-lapse camera (CL-CAM1B) located in Crater Lake permafrost and active layer monitoring site in Crater Lake sounders in Deception island, Antarctica, in 2021.</p> <ul> <li>File code: DEC_CL_CAM1B_2021_v100</li> <li>Location code: DEC</li> <li>Site code: CL</li> <li>Instrument code: CAM1B</li> <li>Period: 2021</li> <li>Version: 1.0.0 (jpg images as they were obtained from camera, without processing)</li> <li>Camera/manufacturer: CC5MPX by Campbell Scientific Inc.</li> <li>Resolution/Type/Format: 5Mpixels in RGB in jpg files</li> <li>Frequency: 3 images per day at 14h, 15h and 16h GMT</li> <li>Site: Close to Crater Lake CALM site, in Crater Lake sounders of Deception island, Antarctica.</li> <li>Location: </li> <li>Elevation:</li> <li>Initial dataset date/time: February 20, 2021 14:00h GMT</li> <li>Final dataset date/time: January 13, 2022 15:00h GMT</li> <li>Gaps: None</li> <li>Notes: <ul> <li>Folders: 12</li> <li>Files: 983</li> <li>Other files: none</li> <li>Folder names structure: year_month</li> <li>Datafiles names structure: Site_camera_year_month_day_hour_minute_second.jpg</li> </ul> </li> </ul>
Phenomenological images (CL-CAM2) of Crater Lake CALM site, Deception island, Antarctica (2021).
<p>Images acquired by a phenomenological automatic time-lapse camera (CL-CAM2) located in Crater Lake permafrost and active layer monitoring site in Crater Lake sounders in Deception island, Antarctica, in 2021.</p> <ul> <li>File code: DEC_CL_CAM2_2021_v100</li> <li>Location code: DEC</li> <li>Site code: CL</li> <li>Instrument code: CAM2</li> <li>Period: 2021</li> <li>Version: 1.0.0 (jpg images as they were obtained from camera, without processing)</li> <li>Camera/manufacturer: CC5MPX by Campbell Scientific Inc.</li> <li>Resolution/Type/Format: 5Mpixels in RGB in jpg files</li> <li>Frequency: 3 images per day at 14h, 15h and 16h GMT</li> <li>Site: Close to Crater Lake CALM site, in Crater Lake sounders of Deception island, Antarctica.</li> <li>Location: </li> <li>Elevation:</li> <li>Initial dataset date/time: February 17, 2021 14:00h GMT</li> <li>Final dataset date/time: January 8, 2022 15:00h GMT</li> <li>Gaps: Yes, multiple due to power failure</li> <li>Notes: <ul> <li>Folders: 4</li> <li>Files: 93</li> <li>Other files: no</li> <li>Folder names structure: year_month</li> <li>Datafiles names structure: Site_camera_year_month_day_hour_minute_second.jpg</li> </ul> </li> </ul>
All figures for thermochemical modeling of wet-dry cycles in Gale crater
<p>All figures for thermochemical modeling of wet-dry cycles in Gale crater including model flowchart, result and extrapolation visualizations.</p>
Ceraunius Fossae and Tractus Fossae Crater Catalogue
<p>Catalogue of all craters in Ceraunius Fossae and Tractus Fossae, Mars, with a diameter >800m in shapefile format. Craters are mapped on Context Camera (CTX) images, within the Tanaka et al. (2014) unit boundary outlines.</p>
Recent tectonic activity in and around the Posidonius crater, Moon.
<p>The shapefiles and .scc files of the manuscript: "Recent tectonic activity in and around the Posidonius crater, Moon."</p>
Data from: Repeated divergence in opsin gene expression mirrors photic habitat changes in rapidly evolving crater lake cichlid fishes
Open the record for dataset details and reuse information.
Gini index mean score grain size estimates for Murray formation rocks in the Vera Rubin ridge (Gale crater, Mars) from ChemCam LIBS data (sols 1808-2298)
<p>Data in this repository are included as main research results in the Journal of Geophysical Research: Planets manuscripts entitled:</p> <p><em>"</em>Extensive diagenesis revealed by fine-scale features at Vera Rubin ridge, Gale crater, Mars<em>" </em></p> <p>"A lacustrine paleoenvironment recorded at Vera Rubin ridge, Gale crater: Overview of the sedimentology and stratigraphy observed by the Mars Science Laboratory Curiosity rover".</p> <p> </p> <p><strong>Table captions:</strong></p> <p><em>Table 1. </em>Murray formation targets from the Vera Rubin ridge used in the Gini mean index score (GIMS) analysis (sols 1808-2298) with summary information and G<sub>MEAN </sub>values with associated standard deviation errors. The grain size regimes (GSRs) were defined during the calibration procedure in Rivera-Hernández et al. (2020) and are defined as: mud (G<sub>MEAN</sub>=0.00-0.07; GSR1) and coarse silt to very fine sand (G<sub>MEAN</sub>=0.07-0.10; GSR2). Rocks with G<sub>MEAN</sub>=0.07 are exactly at GSR1 and GSR2 boundary and are reported as GSR1/GSR2. Next to the target names, the symbol * denotes that the ChemCam target was imaged by the Mars Hand Lens Imager (MAHLI), the symbol ** denotes that the dust removal tool was used before the MAHLI image was taken, and ~ signifies that a location close to the ChemCam target was imaged by the MAHLI. </p> <p><em>Table 2</em>. The mean, median, minimum and maximum G<sub>MEAN</sub> and the minimum and maximum grain size regime (GSR) for each Murray formation locality in the Vera Rubin ridge.</p> <p> </p> <p>References:</p> <p>Rivera-Hernández, F., Sumner, D. Y., Mangold N., Wiens, R.W., Edgett, K., Fedo, C., Schieber, J., Banham, S.G., Newsom, H., Gupta, S., Heydari, E., Stack, K.M., Nachon, M., Stein, N., & Maurice, S. (2020) Grain Size Variations in the Murray Formation: Stratigraphic Evidence for Changing Depositional Environments in Gale Crater, Mars. <em>Journal of Geophysical Research:</em><em> Planets.</em> doi:10.1029/2019JE006230</p>
Model Results for "Groundwater Flow to Gale Crater in an Episodically Warm Climate"
<p>Results from the bous_therm code for "Groundwater Flow to Gale Crater in an Episodically Warm Climate"</p> <p>bous_therm code is at doi:10.5281/zenodo.3779418</p> <p>After extraction, the folder goes in the top directory of the bous_therm repository. It can then be read, analyzed, and plotted by scripts in the repository.</p>
Crater Gravity and Parameter Database
<p>This dataset is created for an accompanying paper "Investigating the Influences of Crustal Thickness and Temperature on the Uplift of Mantle Material Beneath Large Impact Craters on the Moon". This dataset includes 324 impact craters/basins with a rim diameter from 100 to 650 km from the LOLA database. Listed crater information is: Name, Location, Diameter, Central Bouguer Anomaly (from GRAIL data), Mare existence (Nelson+2014), Inverted central Moho uplift, Crustal thickness and porosity (Wieczorek+2013), and Crater age (Losiak+2009).</p>
Elevation Models for Reproducible Evaluation of Terrain Representation – Archetypal Landforms – Crater Lake ASCII
<p>An elevation model of Crater Lake, Oregon, USA</p> <p>Landform features: caldera, cinder cone, lava flow</p> <p>Resolution: 3.33 meter, 5,200 x 5,200 height samples</p> <p>File format: Esri ASCII grid</p> <p>This is one model of a set of elevation models: <a href="https://doi.org/10.5281/zenodo.3938020">https://doi.org/10.5281/zenodo.3938020</a>. Please cite the entire set of models.</p> <p>Version 1.0.1 removes empty space characters from the file header, which prevented the file from being opened by some software.</p> <p>When using this elevation model in an academic publication, please cite the following article, which describes the process and rationale for compiling elevation models:</p> <p><em>Kennelly, P. J., Patterson, T., Jenny, B., Huffman, D. P., Marston, B. E., Bell, S. and Tait, A. M. (2021). Elevation models for reproducible evaluation of terrain representation. Cartography and Geographic Information Science, 48:1, 63–77. DOI: <a href="http://doi.org/10.1080/15230406.2020.1830856">10.1080/15230406.2020.1830856</a></em></p>
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These curated guides explain access requirements, typical timelines, costs, and reuse considerations for widely used research datasets.
Allen Brain Atlas
Allen Brain Atlas is an Allen Institute collection of brain map atlases, datasets, APIs, and analysis tools covering mouse, human, and non-human primate brain resources.
Annotated Behaviour and Observability Dataset (ABODe)
ABODe is a University of Edinburgh DataShare dataset for behavior classification in group-housed mice using home-cage video, identities, bounding boxes, ground-plate positions, and annotator labels.
DANDI Archive for NWB datasets
DANDI is a BRAIN Initiative archive for publishing and sharing neurophysiology data, including electrophysiology, optophysiology, and behavioral data packaged as NWB and related standards.
International Brain Laboratory public data
The International Brain Laboratory public data releases expose standardized mouse decision-making experiments, including Neuropixels recordings, widefield calcium imaging, behavior, and session metadata accessed through the ONE API.
OpenNeuro
OpenNeuro is a free, open platform for sharing neuroimaging datasets, with public search, dataset pages, and download paths for web, S3, DataLad, and the OpenNeuro CLI.