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4,634 results for “orbit”
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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Observation of a Chern insulator in crystalline ABCA-tetralayer graphene with spin-orbit coupling
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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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GLASS Land Surface Temperature product (1981-2000): Orbital Drift Corrected LST
<ul> <li>GLASS Land Surface Temperature product (1981-2000): the ODC LST product is an orbital drift corrected (ODC) version of the instantaneous GLASS LST product. To compensate the effect of orbital drift on LST, an improved ODC method was used to normalize the instantaneous GLASS LSTs to 14:30 solar time.</li> <li>The dataset is organized by year and a sample data is provided in simple.zip</li> <li>Further details can be found in the readme.pdf.</li> </ul>
Improved effective equation for the Rashba spin-orbit coupling in semiconductor nanowires (dataset)
<p><strong>Description</strong></p> <p>This repository contains the dataset required to reproduce all the figures of the article "Samuel D. Escribano, Alfredo Levy Yeyati and Elsa Prada,<em> </em><strong><em>Improved effective equation for the Rashba spin-orbit coupling in semiconductor nanowires</em></strong>, arXiv:2001.04375 (2020)".</p> <p> </p> <p><strong>Structure of the dataset</strong></p> <p>All the data is saved in Matlab file-format .mat. Their file names correspond to the figure that they plot. Together with each dataset, there is a Python script .py which plots the corresponding figure. The output of every script is the corresponding figure in PDF-format .pdf. Please, read "reedme.txt" file for further information.</p>
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>
Weak probe readout of coherent impurity orbital superpositions in silicon
<p>Each file contains data which is similar to the one shown in Fig.3.b for different laser bandwidths: 001 and 002 - 0.078THz; 004 and 005 - 0.127THz; 007 and 009 - 0.223THz. The data files 001, 004, and 007 are the probe transmission changes as functions of the delay between one of the pumps and the probe in picoseconds (The other pump arrives a fixed time of 50ps before the probe). The data files 002, 005, and 009 are the same as 001, 004, and 007 but with the probe beam blocked. Please, see the paper for details. </p>
Dataset for the manuscript 'Orbital-optimized Density Functional Calculations of Molecular Rydberg Excited States with Real Space Grid Representation and Self-Interaction Correction'
<p>Dataset for the manuscript 'Orbital-optimized Density Functional Calculations of Molecular Rydberg Excited States with Real Space Grid Representation and Self-Interaction Correction'</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>
Supplementary video 2 for "Phase Memory of Orbital Angular Momentum in Multiple Scattering Environment"
<p>This is Supplementary video 2 for article Meglinski, et. al. "Phase Memory of Orbital Angular Momentum in Multiple Scattering Environment"</p>
Supplementary video for "Phase Memory of Orbital Angular Momentum in Multiple Scattering Environment"
<p>This is Supplementary video for article Meglinski, et. al. "Phase Memory of Orbital Angular Momentum in Multiple Scattering Environment"</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>
Transneptunian Binary Orbit Fits
<p>A set of Keplerian and non-Keplerian fits to the orbits of 45 individual TNO binaries. We provide full MCMC chains of our fits, as well as all diagnostics and outputs. We have verified that all Keplerian fits are converged. Non-Keplerian fits are not converged in almost all cases, but were run for a set amount of steps to try and identify targets for longer, converged analyses. A full paper about these fits and a discussion of their implications will soon be submitted to the Planetary Science Journal (PSJ).</p> <p>We provide these fits to allow anyone to fully examine the outputs of our fitting process. They can also be used a starting point for future analyses as the MCMC chains contain a full posterior distribution of the orbital properties of each TNO binary. A readme is contained within the dataset describing the outputs and the use of the MCMC chains. For any further assistance, please contact us.</p> <p>A "frozen" version of MultiMoon compatible with the dataset is also included.</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>
Dataset for publication "Resolving the Orbital Character of Low-energy Excitations in Mott Insulator with Intermediate Spin-orbit Coupling"
<p>Dataset providing the sourcedata of the main figures in the publication "Resolving the Orbital Character of Low-energy Excitations in Mott Insulator with Intermediate Spin-orbit Coupling"</p>
ScienceDex guides
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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.