Find research datasets worth reusing
Search datasets from major research repositories and use ShareScore to quickly assess how well each record supports discovery, access, and reuse.
390
datasets available to search
ShareScore release 0.9.0
Dataset results
390 results for “after movie”
Data from: Gigapixel big data movies provide cost‐effective seascape scale direct measurements of open‐access coastal human use such as recreational fisheries
Open the record for dataset details and reuse information.
supplyment movie of "The modulation of coherent structures by the near-wall motions of particles"
<p><span>The particle trajectories on the erodible wall recorded by the high-speed photography. </span></p>
movie_BH_xy
Open the record for dataset details and reuse information.
Supporting Movie for "Connecting the Low to High Corona: Propagating Disturbances as Tracers of the Near-Sun Solar Wind" by Alzate et al. (2024)
<p>High-resolution movie of Figure 2 of Alzate et al. (2024).</p>
Movies for Figure 1 in "In LIGO's Sight? Vigorous Coherent Gravitational Waves from Cooled Collapsar Disks, (#AAS56281R1)"
Open the record for dataset details and reuse information.
MD Simulation movies 1,2,3
<p>MD Simulation movies 1,2,3</p>
1930's Movie Camera
High poly model. .zip folder including PBR materials (diffuse, smoothness, metallic) and original .blend file. Adjustable crank handle and switches. Model broken up into various parts (Film, Handle, Lense, Handle, Eyepiece). Adjustable lenses. Modelled accurately to existing products. Ready for use in a game/animation scene. [My Portfolio](http://hogandarren01.wixsite.com/portfolio) Source: Objaverse 1.0 / Sketchfab
Cinema Movie Projector AP5 - 1961
Raw scan made on cinema movie projector that is standing in Kijów Centrum Cimena in Kraków, Poland It was used for 35mm tape. Produced in the 1961 by Łódzkie Zakłady Kinotechniczne in Poland. The projector was designed for cinemas with rooms up to 1000 seats. It was then one of the most popular models used in Polish cinemas The projector was equipped with an aspherical mirror with a diameter of 356 mm and a focal length of 120 mm. The standard lens provided by the manufacturer was Polkinar 1.8 / 100 The basic equipment of the projector was an optical sound reading system with two exposure bulbs - one in the working position, the other one in reserve (both fixed in the rotating holder, which allowed for exchange without interrupting the projection). In addition, the projector could be equipped with a 4-channel magnetic sound pickup The projector was powered by a three-phase asynchronous motor. The engine was started using an automatic starter. https://youtu.be/-xr1BMyKNWI MusicInfo: Piano by AShamaluevMusic Source: Objaverse 1.0 / Sketchfab
Simulated Radiotherapy Treatment Assisted With Pediatric Radiation Oncology With Movie Induced Sedation Effect Technique
ClinicalTrials.gov study NCT03556930. IPD Sharing: Not stated. Countries: 0. Publications: 0.
TIMED Global Ultraviolet Imager (GUVI) Airglow Flux 14-day Movies, at Wavelength 1216 Å in North Polar Projection
GUVI measures FUV Airglow in five Spectral Bands: the atomic HI Lyman-alpha Band, 121.6 nm, two atomic Oxygen OI Bands, 130.4 nm and 135.6 nm, and the molecular Nitrogen Lyman-Birge-Hopfield Short, LBHS, 141 to 152.8 nm, and Lyman-Birge-Hopfield Long, LBHL, 167.2 to 181.2 nm, Bands. The Cross-Track Scanning Spectrograph images a Ground Swath of 3000 km Width providing nearly Contiguous Global Coverage with 15 Orbits per Day. This L1CDisk, Level 1C Disk, Version 3, File provides the calibrated, geolocated, and rectified Intensities for the first H Ly-alpha, 1216 Å, Wavelength Band. This is a Movie with mapped Images of the Log Intensities by Orbit by using a North Polar Projection.
TIMED Global Ultraviolet Imager (GUVI) Airglow Flux 14-day Movies, at Wavelength LBH1 in South Polar Projection
GUVI measures FUV Airglow in five Spectral Bands: the atomic HI Lyman-alpha Band, 121.6 nm, two atomic Oxygen OI Bands, 130.4 nm and 135.6 nm, and the molecular Nitrogen Lyman-Birge-Hopfield Short, LBHS, 141 to 152.8 nm, and Lyman-Birge-Hopfield Long, LBHL, 167.2 to 181.2 nm, Bands. The Cross-Track Scanning Spectrograph images a Ground Swath of 3000 km Width providing nearly Contiguous Global Coverage with 15 Orbits per Day. This L1CDisk, Level 1C Disk, Version 3, File provides the calibrated, geolocated, and rectified Intensities for the fourth LBH1, 1400-1500 Å, Wavelength Band. This is a Movie with mapped Images of the Log Intensities by Orbit by using a South Polar Projection.
TIMED Global Ultraviolet Imager (GUVI) Airglow Flux 14-day Movies, at Wavelength 1356 Å in North Polar Projection
GUVI measures FUV Airglow in five Spectral Bands: the atomic HI Lyman-alpha Band, 121.6 nm, two atomic Oxygen OI Bands, 130.4 nm and 135.6 nm, and the molecular Nitrogen Lyman-Birge-Hopfield Short, LBHS, 141 to 152.8 nm, and Lyman-Birge-Hopfield Long, LBHL, 167.2 to 181.2 nm, Bands. The Cross-Track Scanning Spectrograph images a Ground Swath of 3000 km Width providing nearly Contiguous Global Coverage with 15 Orbits per Day. This L1CDisk, Level 1C Disk, Version 3, File provides the calibrated, geolocated, and rectified Intensities for the third OI, 1356 Å, Wavelength Band. This is a Movie with mapped Images of the Log Intensities by Orbit by using a North Polar Projection.
TIMED Global Ultraviolet Imager (GUVI) Airglow Flux 14-day Movies, at Wavelength LBH2 in South Polar Projection
GUVI measures FUV Airglow in five Spectral Bands: the atomic HI Lyman-alpha Band, 121.6 nm, two atomic Oxygen OI Bands, 130.4 nm and 135.6 nm, and the molecular Nitrogen Lyman-Birge-Hopfield Short, LBHS, 141 to 152.8 nm, and Lyman-Birge-Hopfield Long, LBHL, 167.2 to 181.2 nm, Bands. The Cross-Track Scanning Spectrograph images a Ground Swath of 3000 km Width providing nearly Contiguous Global Coverage with 15 Orbits per Day. This L1CDisk, Level 1C Disk, Version 3, File provides the calibrated, geolocated, and rectified Intensities for the fifth LBH2, 1650-1800 Å, Wavelength Band. This is a Movie with mapped Images of the Log Intensities by Orbit by using a South Polar Projection.
TIMED Global Ultraviolet Imager (GUVI) Airglow Flux 14-day Movies, at Wavelength 1304 Å in South Polar Projection
GUVI measures FUV Airglow in five Spectral Bands: the atomic HI Lyman-alpha Band, 121.6 nm, two atomic Oxygen OI Bands, 130.4 nm and 135.6 nm, and the molecular Nitrogen Lyman-Birge-Hopfield Short, LBHS, 141 to 152.8 nm, and Lyman-Birge-Hopfield Long, LBHL, 167.2 to 181.2 nm, Bands. The Cross-Track Scanning Spectrograph images a Ground Swath of 3000 km Width providing nearly Contiguous Global Coverage with 15 Orbits per Day. This L1CDisk, Level 1C Disk, Version 3, File provides the calibrated, geolocated, and rectified Intensities for the second OI, 1304 Å, Wavelength Band. This is a Movie with mapped Images of the Log Intensities by Orbit by using a South Polar Projection.
DEEP IMPACT INSTRUMENT MOVIES OF 9P/TEMPEL 1, V1.0
This data set comprises a collection of movies of comet 9P/Tempel 1, created from observations made by the High Resolution (visual mode) and Medium Resolution Instruments aboard the flyby craft, and the Impactor Tracking Sensor aboard the impactor craft.
TIMED Global Ultraviolet Imager (GUVI) Airglow Flux 14-day Movies, at Wavelength 1304 Å in Mercator Projection
GUVI measures FUV Airglow in five Spectral Bands: the atomic HI Lyman-alpha Band, 121.6 nm, two atomic Oxygen OI Bands, 130.4 nm and 135.6 nm, and the molecular Nitrogen Lyman-Birge-Hopfield Short, LBHS, 141 to 152.8 nm, and Lyman-Birge-Hopfield Long, LBHL, 167.2 to 181.2 nm, Bands. The Cross-Track Scanning Spectrograph images a Ground Swath of 3000 km Width providing nearly Contiguous Global Coverage with 15 Orbits per Day. This L1CDisk, Level 1C Disk, Version 3, File provides the calibrated, geolocated, and rectified Intensities for the second OI, 1304 Å, Wavelength Band. This is a Movie with mapped Images of the Log Intensities by Orbit by using a Transverse Mercator Projection.
TIMED Global Ultraviolet Imager (GUVI) Airglow Flux 14-day Movies, at Wavelength 1304 Å in North Polar Projection
GUVI measures FUV Airglow in five Spectral Bands: the atomic HI Lyman-alpha Band, 121.6 nm, two atomic Oxygen OI Bands, 130.4 nm and 135.6 nm, and the molecular Nitrogen Lyman-Birge-Hopfield Short, LBHS, 141 to 152.8 nm, and Lyman-Birge-Hopfield Long, LBHL, 167.2 to 181.2 nm, Bands. The Cross-Track Scanning Spectrograph images a Ground Swath of 3000 km Width providing nearly Contiguous Global Coverage with 15 Orbits per Day. This L1CDisk, Level 1C Disk, Version 3, File provides the calibrated, geolocated, and rectified Intensities for the second OI, 1304 Å, Wavelength Band. This is a Movie with mapped Images of the Log Intensities by Orbit by using a North Polar Projection.
TIMED Global Ultraviolet Imager (GUVI) Airglow Flux 14-day Movies, at Wavelength 1216 Å in South Polar Projection
GUVI measures FUV Airglow in five Spectral Bands: the atomic HI Lyman-alpha Band, 121.6 nm, two atomic Oxygen OI Bands, 130.4 nm and 135.6 nm, and the molecular Nitrogen Lyman-Birge-Hopfield Short, LBHS, 141 to 152.8 nm, and Lyman-Birge-Hopfield Long, LBHL, 167.2 to 181.2 nm, Bands. The Cross-Track Scanning Spectrograph images a Ground Swath of 3000 km Width providing nearly Contiguous Global Coverage with 15 Orbits per Day. This L1CDisk, Level 1C Disk, Version 3, File provides the calibrated, geolocated, and rectified Intensities for the first H Ly-alpha, 1216 Å, Wavelength Band. This is a Movie with mapped Images of the Log Intensities by Orbit by using a South Polar Projection.
TIMED Global Ultraviolet Imager (GUVI) Airglow Flux 14-day Movies, at Wavelength LBH2 in Mercator Projection
GUVI measures FUV Airglow in five Spectral Bands: the atomic HI Lyman-alpha Band, 121.6 nm, two atomic Oxygen OI Bands, 130.4 nm and 135.6 nm, and the molecular Nitrogen Lyman-Birge-Hopfield Short, LBHS, 141 to 152.8 nm, and Lyman-Birge-Hopfield Long, LBHL, 167.2 to 181.2 nm, Bands. The Cross-Track Scanning Spectrograph images a Ground Swath of 3000 km Width providing nearly Contiguous Global Coverage with 15 Orbits per Day. This L1CDisk, Level 1C Disk, Version 3, File provides the calibrated, geolocated, and rectified Intensities for the fifth LBH2, 1650-1800 Å, Wavelength Band. This is a Movie with mapped Images of the Log Intensities by Orbit by using a Transverse Mercator Projection.
TIMED Global Ultraviolet Imager (GUVI) Airglow Flux 14-day Movies, at Wavelength 1216 Å in Mercator Projection
GUVI measures FUV Airglow in five Spectral Bands: the atomic HI Lyman-alpha Band, 121.6 nm, two atomic Oxygen OI Bands, 130.4 nm and 135.6 nm, and the molecular Nitrogen Lyman-Birge-Hopfield Short, LBHS, 141 to 152.8 nm, and Lyman-Birge-Hopfield Long, LBHL, 167.2 to 181.2 nm, Bands. The Cross-Track Scanning Spectrograph images a Ground Swath of 3000 km Width providing nearly Contiguous Global Coverage with 15 Orbits per Day. This L1CDisk, Level 1C Disk, Version 3, File provides the calibrated, geolocated, and rectified Intensities for the first H Ly-alpha, 1216 Å Wavelength Band. This is a Movie with mapped Images of the Log Intensities by Orbit by using a Transverse Mercator Projection.
ScienceDex guides
Understand access before you commit
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.