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101
datasets available to search
ShareScore release 0.9.0
Dataset results
101 results for “Spectral imaging”
CH1-ORB MOON M3 4 L1B RADIANCE NEAR-IR SPECTRAL IMAGES V3.0
This dataset contains pixel located, radiometrically-calibrated data collected by M3 instrument on Chandrayaan-1.
GALILEO NIMS SPECTRAL IMAGE CUBES: JUPITER OPERATIONS
The natural form of imaging spectrometer data is the spectral image cube. It is normally in band sequential format, but has a dual nature. It is a series of 'images' of the target, each in a different wavelength, in ascending order. It is also a set of spectra, each at a particular line and sample, over the target area. Each spectrum describes a small portion of the area. When transformed into cubes, the data may be analyzed spatially, an image at a time, or spectrally, a spectrum at a time, or in more complex spatial-spectral fashion.
CASSINI ORBITER SATURN UVIS SPATIAL SPECTRAL IMAGE CUBE 1.0
Spectrographic observations of Jupiter, Saturnian rings, satellites, atmospheres and the interplanetary medium in the far and extreme ultraviolet.
CH1-ORB MOON M3 4 L1B RADIANCE NEAR-IR SPECTRAL IMAGES V1.0
This dataset contains pixel located, radiometrically-calibrated data collected by M3 instrument on Chandrayaan-1.
HIRES NIMS GASPRA SPECTRAL IMAGE CUBE
This data volume contains a 17 channel spectral image cube of asteroid 951 Gaspra ranging from 0.7 to 5.2 micrometers in wavelength in cgs units of radiance. The spatial resolution of this data is 1.28 km/pixel. This data set was obtained by the Galileo spacecraft Near Infrared Mapping Spectrometer on October 29, 1991. It was radiometrically calibrated using calibration measurements obtained by the Near Infrared Mapping Spectrometer during its observations of Earth on December 9, 1990.
CH1-ORB MOON M3 4 L1B RADIANCE NEAR-IR SPECTRAL IMAGES V2.0
This dataset contains pixel located, radiometrically-calibrated data collected by M3 instrument on Chandrayaan-1.
GALILEO NIMS SPECTRAL IMAGE TUBES: JUPITER OPERATIONS
The natural form of imaging spectrometer data is the spectral image cube. It is normally in band sequential format, but has a dual nature. It is a series of 'images' of the target, each in a different wavelength, in ascending order. It is also a set of spectra, each at a particular line and sample, over the target area. Each spectrum describes a small portion of the area. When transformed into cubes, the data may be analyzed spatially, an image at a time, or spectrally, a spectrum at a time, or in more complex spatial-spectral fashion.
CONTOUR REMOTE IMAGING SPEC. GROUND OCF SPECTRAL DATA
This dataset contains raw counts from the the spectrograph of the CONTOUR Remote Imaging Spectrograph (CRISP) instrument during ground calibration in the Optical Calibration Facility (OCF) at JHU/APL in 2002.
CASSINI ORBITER JUPITER UVIS SPATIAL SPECTRAL IMAGE CUBE 1.0
Spectrographic observations of Jupiter, Saturnian rings, satellites, atmospheres and the interplanetary medium in the far and extreme ultraviolet.
CH1-ORB MOON M3 2 L0 RAW NEAR-IR SPECTRAL IMAGES V1.0
This data set contains raw near-IR spectral image cubes acquired from November 2008 through August 2009 by the Moon Mineralogy Mapper (M3) instrument during the Chandrayaan-1 mission to the Moon.
CASSINI ORBITER SATURN UVIS SPATIAL SPECTRAL IMAGE CUBE V1.3
Spectrographic observations of Jupiter, Saturnian rings, satellites, atmospheres and the interplanetary medium in the far and extreme ultraviolet.
CASSINI ORBITER SATURN UVIS SPATIAL SPECTRAL IMAGE CUBE V1.4
Spectrographic observations of Jupiter, Saturnian rings, satellites, atmospheres and the interplanetary medium in the far and extreme ultraviolet.
CASSINI ORBITER SATURN UVIS SPATIAL SPECTRAL IMAGE CUBE 1.1
Spectrographic observations of Jupiter, Saturnian rings, satellites, atmospheres and the interplanetary medium in the far and extreme ultraviolet.
HIRES NIMS IDA SPECTRAL IMAGE CUBES
This data volume contains 17 channel spectral image cubes of asteroid 243 Ida ranging from 0.7 to 5.2 micrometers in wavelength in cgs units of radiance. These data were obtained by the Galileo spacecraft Near Infrared Mapping Spectrometer on August 28, 1993. They were radiometrically calibrated using calibration measurements obtained by the Near Infrared Mapping Spectrometer during its observations of Europa on June 28, 1996.
CASSINI ORBITER N/A UVIS SPATIAL SPECTRAL IMAGE CUBE 1.0
Spectrographic observations of Jupiter, Saturnian rings, satellites, atmospheres and the interplanetary medium in the far and extreme ultraviolet.
TW Hya STIS Spectral Imaging
<p>2-D spectral image from HST PID 11607 (PI: T. Bethell)</p>
NIMS SPECTRAL IMAGE CUBES OF THE EARTH: E1 & E2 ENCOUNTERS
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NIMS SPECTRAL IMAGE CUBES OF THE EARTH: E1 & E2 ENCOUNTERS
Unknown
NIMS SPECTRAL IMAGE TUBES OF THE MOON: E1 & E2 ENCOUNTERS
Unknown
NIMS SPECTRAL IMAGE CUBES OF VENUS
Unknown
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.