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319 results for “Lunar”
Illuminating Tycho's Rays: Automated Crater Census Uncovers Equilibrium Dynamics and Regolith Stratification on the Lunar Surface
<p>Excel files containing all crater data are output from ArcMap.</p> <p><br>DATA_HUMA_craters_raw contains two files for the *186 and *808 NAC images as coordinates and diameter (km). These are all the manual labelling for the NACs, with not-included data. Full set.</p> <p>DATA_YOLO_craters_raw contains several files for each sub-area, coordinates, diameter, and additional information</p> <p>DATA_selected_craters is a table that formed the <strong>basis for the analysis</strong>. It lists the crater sizes for each area (summed) and gives the surface area of the regions under investigation.</p>
Chemical compositions data for "Space weathering of the Chang'e-5 lunar sample from a mid-high latitude region on the Moon"
<p>Data for “Space weathering of the Chang’e-5 lunar sample from a mid-high latitude region on the Moon”</p>
The datasets for the paper "Spatial and temporal distribution of lobate scarps in the lunar south polar region: Evidence for latitudinal variation of scarp geometry, kinematics and formation ages, continuous tectonic activity in the last 100 million years and seismically safe south pole Artemis human landing site" Geophysical Research Letters.
<p>This dataset provides the original data that were used for preparing the illustrations, figures and tables.</p>
Modeling Thermal Emission Under Lunar Surface Environmental Conditions
<p>Codes and data required to reproduce results from Prem et al. (2022), Modeling Thermal Emission Under Lunar Surface Environmental Conditions, Planetary Science Journal (https://doi.org/10.3847/PSJ/ac7ced).</p> <p>The file flowchart.pdf contains an overview of the workflow to model ambient and anisothermal thermal emission spectra using the codes contained in codes.zip. The file lab_spectra.xlsx contains the laboratory spectra used in the publication, together with citation information. Please feel free to contact lead author Dr. Parvathy Prem (parvathy.prem@jhuapl.edu) with any questions. </p>
Thermal Environment and Illumination of Lunar Pits and Caves Data, Code, and Images
<p>Lunar Reconnaissance Orbiter Diviner data focusing on the Tranquillitatis pit and analysis code for determining the thermal and illumination environments of the collapse pits and caves on the Moon. Also includes figures created using the code.</p>
Wave transmission through the megaregolith as a mechanism for lunar cold spot formation: supplementary information
<p>Supplementary information for Frizzell and Hartzell, 2024 - Wave transmission through the megaregolith as a mechanism for lunar cold spot formation. Contains LIGGGTS input scripts and restart files, MATLAB processing and analysis codes along with example processed *.mat files. Any generated code can be found at our linked public repository.</p>
The dataset for the Icarus paper "Crustal origin for olivine in the lunar Shioli crater ejecta boulders: Insights from the geological setting of Theophilus crater and Nectaris basin" [dataset]
<p><span>The dataset is for the Icarus paper “Crustal origin for olivine in the lunar Shioli crater ejecta boulders: Insights from the geological setting of Theophilus crater and Nectaris basin” [dataset]</span></p>
Rock distribution data on lunar surface
<p>This dataset includes the rock distribution data on lunar surface as reported in an article by Yuan Li and Bo Wu (Analysis of Rock Abundance on Lunar Surface from Orbital and Descent images Using Automatic Rock Detection).</p>
Digital versions of lunar geological maps
<p>As the link for this database is not working at USGS website (i.e., https://astrogeology.usgs.gov/search/map/Moon/Geology/Lunar_Geologic_GIS_Renovation_March2013), we upload this database.</p>
Petrological and chemical modifications during impact melting and cooling in shocked lunar regolith: Insights from heterogeneous Chang'E-5 impact melt-bearing particle
<p>Petrological, mineralogical and chemical data of the lunar impact-melt bearing particle C10 from the Chang'E-5 regolith, and scripts for mesoscale modeling and mixing composition calculations.</p>
Radiation exposure and shielding effects on the lunar surface - supplementary data
<p>Supplementary data for submission of "Radiation exposure and shielding effects on the lunar surface"</p>
Raman spectral data for ''The evaluation of space weathering effects on lunar samples from a Raman spectroscopic perspective''
Open the record for dataset details and reuse information.
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>
Lunar dichotomy: Chang'e-6 2.83 Ga farside mare basalts reveal most depleted mantle to date
<p>The uploaded files contain the data and code used for plotting lunar crater chronology funtions. The Excel spreadsheet provides the N(1) values and sample ages for calibration points, along with the corresponding references.</p>
Repository: Lunar farside volcanism 2.8 billion years ago from Chang'e-6 basalts
<p>This repository contains all geochemical data (Supplementary Tables 1-5) generated in the paper "Lunar farside volcanism 2.8 billion years ago from Chang’e-6 basalts".</p> <p><strong>Supplementary Tables</strong></p> <p>Table 1. Pb-Pb isochron data for the Chang'e-6 basalts.</p> <p>Table 2. EMPA data of plagioclase and clinopyroxene in the 4.2 Ga high-Al basalt clast.</p> <p>Table 3. EPMA condition applied for mineral composition measurement.</p> <p>Table 4. Data of glass standard NIST610 of SIMS Pb isotope analyses.</p> <p>Table 5. Background measurements for electronic multiplier (EM) collectors.</p>
Data from: Singing in the moonlight: dawn song performance of a diurnal bird varies with lunar phase
It is well established that the lunar cycle can affect the behaviour of nocturnal animals, but its potential to have a similar influence on diurnal species has received less research attention. Here we demonstrate that the dawn song of a cooperative songbird, the white-browed sparrow weaver (Plocepasser mahali), varies with moon phase. When the moon was above the horizon at dawn, males began singing on average 10 minutes earlier if there was a full moon compared to a new moon, resulting in a 67% mean increase in performance period and greater total song output. The lack of a difference between full and new moon dawns when the moon was below the horizon suggests that the observed effects were driven by light intensity, rather than other factors associated with moon phase. Effects of the lunar cycle on twilight signalling behaviour have implications for both pure and applied animal communication research.
Lunar heat flow constrained from Chang'E-2 Microwave Radiometer and Diviner observations at the Moon's south pole
<p>This data repository includes the Chang'E-2 microwave radiometer data which is provided by the Ground Research and Application System of Chinese Lunar Exploration Program.</p>
Repository: A dry lunar mantle reservoir for young mare basalts of Chang'E-5
<p>This repository contains all geochemical data (Extended Data Tables 1-5 and Supplementary Tables S1-S5) generated in the paper "A dry lunar mantle reservoir for young mare basalts of Chang'E-5".</p> <p><strong>Extended Data Tables:</strong></p> <p>Extended Data Table 1 | The Chang’E-5 basalt clasts</p> <p>Extended Data Table 2 | Water abundance and hydrogen isotopes of CE5 apatite</p> <p>Extended Data Table 3 | Water abundance and hydrogen isotopes of CE5 ilmenite-hosted melt inclusions</p> <p>Extended Data Table 4 | H/O ratios of CE5 clinopyroxene and reference San Carlos olivine measured by NanoSIMS 50L</p> <p>Extended Data Table 5 | Summary of the water abundances estimated for the lunar mantle source regions of basaltic products formed between ca. 4-2 Ga.</p> <p><strong>Supplementary Tables.</strong></p> <p>Table S1. Modal abundance of apatite in the CE5 basalt clasts.</p> <p>Table S2. EPMA analytical results of CE5 basalt clasts.</p> <p>Table S3. NanoSIMS analytical results of the standards and silicates of CE5 basalt clasts.</p> <p>Table S4. Water abundances and hydrogen isotope compositions of ilmenite-hosted melt inclusions with correction for spallation effects.</p> <p>Table S5. Summary of water abundances and hydrogen isotope compositions of apatite and melt inclusions from Apollo samples in the literature.</p>
Data sets associated with "Deep structure of the lunar South Pole–Aitken basin"
<p>These grid files contain the data used in Figures 2 and 3 of the submitted manuscript, "Deep structure of the lunar South Pole–Aitken basin". Although the data are global, note that they are not meant to be used outside of the South Pole–Aitken basin.</p>
Oxide abundances on the lunar surface
<p>Abundance and distribution of oxide abundances and Mg# values generated from KAGUYA multiband imager (MI) spectra</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
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DANDI Archive for NWB datasets
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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.