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283 results for “orbital data”
Simulation Data for Electron Scattering due to Asymmetric Drift-Orbit Bifurcation: Geometric Jumps of Adiabatic Invariant
<p>Simulation dataset for the paper “Electron Scattering due to Asymmetric Drift-Orbit Bifurcation: Geometric Jumps of Adiabatic Invariant.” The archive “artemis_solar_dataset.zip” contains the solar wind magnetic field data used to plot Figure 1. The three “…_jump.txt” files are tracing data used to plot Figures 6a, 6b, and 6c, while “test_particle.txt” is the tracing data for Figure 5. The file “t04_L_shells__Pd_4.00_B_5.00_theta_225.txt” provides magnetic field B(s, MLT) profiles at different L-shells (used to plot Figure 7); each line corresponds to a specific MLT sector at one specific L-shell.</p>
Data from: The effect of sampling methods on the validity and reliability of the estimation of the orbital stability of human gait
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Data from: Structural and mechanical properties facilitate shock wave damping by helmet-like orbital hoods in snapping shrimp
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Data from: Novel roles of chloroquine and hydroxychloroquine in Graves’ orbitopathy therapy by targeting orbital fibroblasts
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DQ-1 Aerosols and Carbon Dioxide Lidar detects orbital data on power plant emissions
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Data from: The seasonal cycles of tropical sea surface temperature from Earth's axial tilt and orbital eccentricity
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Data from: Field-free deterministic switching of all-van der Waals spin-orbit torque system above room temperature
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Data from: Emergent Rashba spin-orbit coupling in bulk gold with buried network of nanoscale interfaces
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Mars orbital image (HiRISE) labeled data set version 3.2
<p> </p> <p><strong>Please note that the file hirise-map-proj-v3_2.zip below contains the latest images and labels associated with this data set. </strong></p> <p> </p> <p>This dataset contains a total of 64,947 landmark images that were detected and extracted from HiRISE browse images, spanning 232 separate source images.</p> <p>This set was formed from 10,815 original landmarks. Each original landmark was cropped to a square bounding box that included the full extent of the landmark plus a 30-pixel margin to the left, right, top, and bottom. Each landmark was then resized to 227x227 pixels. 9,022 of these images were then augmented to generate 6 additional landmarks using the following methods:</p> <p>1. 90 degrees clockwise rotation<br> 2. 180 degrees clockwise rotation<br> 3. 270 degrees clockwise rotation<br> 4. Horizontal flip<br> 5. Vertical flip<br> 6. Random brightness adjustment</p> <p>The remaining 1,793 images were not augmented. Combining these with the 7*9,022 images, gives a total of 64,947 separate images.</p> <p><br> <strong>Contents:</strong><br> - map-proj-v3_2/: Directory containing individual cropped landmark images<br> - labels-map-proj-v3_2.txt: Class labels (ids) for each landmark image. File includes two columns separated by a space: filename, class_id</p> <p>- labels-map-proj-v3_2_train_val_test.txt: Includes train/test/val labels and upsampling used for trained model. File includes three columns separated by a space: filename, class_id, set<br> - landmarks_map-proj-v3_2_classmap.csv: Dictionary that maps class ids to semantic names</p> <p><strong>Class Discussion:</strong></p> <p>We give a discussion of the various landmarks that make up our classes.<strong> </strong></p> <p>Bright dune and dark dune are two sand dune classes found on Mars. Dark dunes are completely defrosted, whereas bright dunes are not. Bright dunes are generally bright due to overlying frost and can exhibit black spots where parts of the dune are defrosting.</p> <p>The crater class consists of crater images in which the diameter of the crater is greater than or equal to 1/5 the width of the image and the circular rim is visible for at least half the crater's circumference.</p> <p>The slope streak class consists of images of dark flow-like features on slopes. These features are believed to be formed by a dry process in which overlying (bright) dust slides down a slope and reveals a darker sub-surface.</p> <p>Impact ejecta refers to material that is blasted out from the impact of a meteorite or the eruption of a volcano. We also include cases in which the impact cleared away overlying dust, exposing the underlying surface. In some cases, the associated crater may be too small to see. Impact ejecta can also include lava that spilled out from the impact (blobby ("lobate") instead of blast-like), more like an eruption (triggered by the impact). Impact ejecta can be isolated, or they can form in clusters when the impactor breaks up into multiple fragments.</p> <p>Spiders and Swiss cheese are phenomena that occur in the south polar region of Mars. Spiders have a central pit with radial troughs, and they are believed to form as a result of sublimation of carbon dioxide ice. This process can produce mineral deposits on top, which look like dark or light dust that highlights cracks in the CO2 ice. Spiders can resemble impact ejecta due to their radial troughs, but impact ejecta tends to have straight radial jets that fade as they get farther from the center. The spider class also includes fan-like features that form when a geyser erupts through the CO2 layer and the material is blown by the wind away from the cracks. Fans are typically unidirectional (following the wind direction), whereas impact ejecta often extends in multiple directions. Swiss cheese is a terrain type that consists of pits that are formed when the sun heats the ice making it sublimate (change solid to gas).</p> <p>Other is a catch-all class that contains images that fit none of the defined classes of interest. This class makes up the majority of our data set.</p>
Raw Data: Signatures of a surface spin-orbital chiral current metal
<p>Authors:</p><p>Federico Mazzola, Wojciech Brzezicki, Maria Teresa Mercaldo, Anita Guarino, Chiara Bigi, Jill A. Miwa, Domenico De Fazio, Alberto Crepaldi, Jun Fujii, Giorgio Rossi, Pasquale Orgiani, Sandeep Kumar Chaluvadi, Shyni Punathum Chalil, Giancarlo Panaccione, Anupam Jana, Vincent Polewczyk, Ivana Vobornik, Changyoung Kim, Fabio Miletto Granozio, Rosalba Fittipaldi, Carmine Ortix, Mario Cuoco, and Antonio Vecchione</p>
SuperDARN data used in the study of "Localized Magnetopause Erosion at Geosynchronous Orbit by Reconnection"
<p>Convection velocity data (20140227.north.nc) is available in the netCDF file format.</p> <p>Each SuperDARN data is provided in the fitacf file format.</p> <p> </p>
Data for "Interplay of magnetic order and ferroelasticity in the spin-orbit coupled antiferromagnet K2ReCl6" published in PRB 109, 094409 (2024)
<p>The manuscript of paper is also available on arXiv:2207.11101</p> <p>The manuscript of this <a href="https://doi.org/10.1103/PhysRevB.109.094409">Phys. Rev. B paper</a> is also available on arxiv <a href="https://arxiv.org/abs/2207.11101">2401.03064</a>. </p> <p> </p>
Data for the article "Harnessing Orbital Hall Effect in Spin-Orbit Torque MRAM"
<p>Dataset for the article: R. Gupta et al., “Harnessing Orbital Hall Effect in Spin-Orbit Torque MRAM,” Nature Communications XX, XXXX (202X).</p> <p> </p>
Simulation data for the article "On the Effect of the Large Magellanic Cloud on the Orbital Poles of Milky Way Satellite Galaxies"
<p>This archive contains the data shared in the context of the "On the Effect of the Large Magellanic Cloud on the Orbital Poles of Milky Way Satellite Galaxies" article.</p> <p>In particular, it contains the initial conditions and final snapshots of our N-body simulation.</p>
Data for 'Experimental Determination of a Single Atom Ground State Orbital through Hyperfine Anisotropy'
<p>This folder contains the raw data and scripts used for the paper <em>'Experimental Determination of a Single Atom Ground State Orbital through Hyperfine Anisotropy'</em>.</p>
The Data for Gaseous Dynamical Friction on Elliptical Keplerian Orbits
<p>The results for the the changing orbital elements of single perturbers and equal mass binaries due to Gaseous Dynamical Friction. The arrays ecc0, Mp represent the eccentricities and Mach numbers over which the change in semi-major axis (adot) eccentricity (edot) and precession (omegadot) are calculated. </p>
Data from: "Eddington envelopes: The fate of stars on parabolic orbits tidally disrupted by supermassive black holes" (Price et al. 2024)
<p>The paper by Price et al. (2024; <a href="https://arxiv.org/abs/2404.09381">arXiv:2404.09381</a>) simulates the tidal disruption of a one solar mass polytropic star by a million-solar-mass supermassive black hole, using the Phantom general relativistic smoothed particle hydrodynamics code (Price et al. 2018). The code used to perform the simulations is available at:</p> <p><a href="https://github.com/danieljprice/phantom">https://github.com/danieljprice/phantom</a></p> <p>This dataset contains:</p> <ol> <li>Scripts, intermediate data products and other small files used to create each figure in the paper</li> <li>Selected snapshots and other raw data from the four main calculations shown in the paper</li> </ol> <p>The main datasets contain parameter files and snapshots from the simulations used to create figures in the paper.small data files from the simulations and post-processing scripts used to create the scientific results and figures shown in the paper. Each simulation dataset contains:</p> <p><strong>.setup file:</strong> parameter file used by phantomsetup to create the initial conditions for the star itself<br><br><strong>.in file:</strong> parameter file used by phantom to perform the calculation<br><br><strong>tde_00000, tde_00100, tde_00200 etc:</strong> binary code snapshots containing raw data (particle positions, velocities, thermal energy, etc), these can be read/visualised/converted using the free and open source codes SPLASH (Price et al. 2007):<br><br><a href="https://github.com/danieljprice/splash">https://github.com/danieljprice/splash</a></p> <p>or Sarracen:</p> <p><a href="https://github.com/ttricco/sarracen">https://github.com/ttricco/sarracen</a></p> <p>SPLASH was used to create figures in the paper. The format and ways to read these data files are described in:</p> <p><a href="https://phantomsph.readthedocs.io/en/latest/user-guide/dumpfile.html">https://phantomsph.readthedocs.io/en/latest/user-guide/dumpfile.html</a></p> <p><strong>tde01.ev, tde02.ev etc:</strong> ascii files (see header) containing global quantities like total angular momentum, total momentum, total energy etc as a function of time. Each number corresponds to a restart of the code (i.e. resubmission of the job to the queue on the cluster).</p> <p><strong>tde01.log, tde02.log: </strong>output log from the simulations themselves, this contains some useful information like the unit scalings, typical timestep and code performance, hardware information etc.</p> <p><em><strong>.defaults, .limits, .units and .filenames:</strong> parameter files used by SPLASH to create particular figures. For example, to use the files lightcurve.defaults, lightcurve.units, lightcurve.limits and lightcurve.filenames one would plot using splash -p lightcurve</em></p> <p>The relevant raw data directories are:</p> <p><strong>beta1_hres: </strong>raw data from the adiabatic, beta=1 calculation</p> <p><strong>beta5_hres:</strong> raw data from the adiabatic, beta=5 calculation</p> <p><strong>beta1_isentropic: </strong>raw data from the isentropic, beta=1 calculation with a non-spinning black hole</p> <p><strong>beta1_isentropic_kerr_a99_i60:</strong> raw data from the isentropic, beta=1 calculation with a maximally-spinning black hole with the initial stellar orbit at an incliation of 60 degrees to the black hole spin</p> <p><strong>The procedure to recreate each figure and post-processing analysis used in the paper is explained in the README.md placed in each directory unpacked from the figureX.zip file</strong></p> <p> </p>
Research data for: "Band Structure Interpolation using Optimized Local Orbitals from Linear-Scaling Density-Functional Theory"
<p>This file was created by Laura E. Ratcliff on 23rd March 2018. It contains the input files employed for the ONETEP and CASTEP calculations in the above publication.</p> <p>Directory Listing:</p> <p>castep/</p> <p>Contains the input files used to generate the CASTEP reference data.</p> <p>onetep/</p> <p>Contains the input files used to generate all of the ONETEP data, where filenames are labelled with the number of repeat CNT units, val (cond) indicates a valence (conduction) calculation and the suffixes follow a similar labelling convention to that employed in the manuscript.</p>
Supporting Data for the paper titled"Diurnal Variation of Liquid Water Path Derived from Two Polar-Orbiting FengYun-3 Microwave Radiation Imagers"
<p>The dataset contains:</p> <p>a) 4 files with name indicating collocated satellite, sensor, latitude,longitude and brightness temperature; format</p> <p>b) annual mean liquid water path derived from FY-3B/C Level 1 data; satellite,sensor, region; format</p> <p>c) annual mean amplitude and phase</p> <p>d) four seasons (winter,spring,summer, and autumn) mean amplitude</p> <p>d) 24 files with name indicating sensor, lwp, region, local solar time hour, format</p> <p>All files can be read by using matlab language.</p> <p> </p> <p>The first author was supported by National Natural Science Foundation of China Grant 91337218, and the second author was supported by NOAA grant NA14NES4320003 (Cooperative Institute for Climate and Satellites-CICS) at the University of Maryland/ESSIC.</p> <p>Corresponding author: Xiaolei Zou,xzou1@umd.edu</p>
Supporting data for "Spectroscopy of Quantum Dot Orbitals with In-Plane Magnetic Fields"
<p>Supporting data for<br> "Hyperfine-phonon spin relaxation in a single-electron GaAs quantum dot"<br> Leon C. Camenzind, Liuqi Yu, Peter Stano, Jeramy D. Zimmerman, Arthur C. Gossard, Daniel Loss & Dominik M. Zumbühl</p> <p><em>Phys. Rev. Lett. <strong>122</strong>, 207701 – Published 22 May 2019</em></p>
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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)
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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.