Found 106 datasets matching "imageintensity".
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THEMIS Ground All Sky Imager at Yellowknife (62.52 deg GLat, 245.69 deg GLong): 32 x 32 pixel thumbnails for full ASI images. The ASI stations monitor a 170 degree field of view imaging the...
Search relevance: 28.66 | Views last month: 1 -
THEMIS Ground All Sky Imager at Narsarsuaq (61.16 deg GLat, 314.56 deg GLong): 32 x 32 pixel thumbnails for full ASI images. The ASI stations monitor a 170 degree field of view imaging the...
Search relevance: 28.66 | Views last month: 1 -
Polar Visible Imaging System (VIS) Low Resolution Camera Images, Calibrated, Level 0 (L0), 12 s Data
Instrument Functional Description: The VIS Instrument is a Set of three Low Light Level Cameras. Two of these Cameras share primary and some secondary Optics and are designed to provide Images of...
Search relevance: 28.66 | Views last month: 1 -
THEMIS Ground All Sky Imager at Inuvik (68.41 deg GLat, 226.23 deg GLong): 32 x 32 pixel thumbnails for full ASI images. The ASI stations monitor a 170 degree field of view imaging the auroral...
Search relevance: 28.66 | Views last month: 1 -
THEMIS Ground All Sky Imager at Pinawa (50.20 deg GLat, 263.96 deg GLong): 256 x 256 pixel full resolution images of auroral oval. The ASI stations monitor a 170 degree field of view imaging the...
Search relevance: 28.66 | Views last month: 1 -
The LASCO C3 Raw FITS Data. LASCO (Large Angle Spectroscopic Coronagraph) is comprised of three nested coronagraphs (C1, C2, and C3) that image the solar corona from 1.1--30 solar radii (C1:...
Search relevance: 28.66 | Views last month: 1 -
THEMIS Ground All Sky Imager at McGrath (62.95 deg GLat, 204.40 deg GLong): 256 x 256 pixel full resolution images of auroral oval. The ASI stations monitor a 170 degree field of view imaging the...
Search relevance: 28.66 | Views last month: 1 -
The FUV instrument takes 2D images of the Earth’s horizon in the Far ultraviolet. The imager is pointing approximately 90 degrees to the spacecraft motion, similar to looking out of the side...
Search relevance: 28.66 | Views last month: 0 -
THEMIS Ground All Sky Imager at Gillam (56.35 deg GLat, 265.34 deg GLong) 32 x 32 pixel thumbnails for full ASI images. The ASI stations monitor a 170 degree field of view imaging the auroral...
Search relevance: 28.66 | Views last month: 0 -
TWINS, Two Wide-angle Imaging Neutral-atom Spectrometers, is a Mission of Opportunity under NASA's Small Explorer, SMEX, Program. TWINS-1 and TWINS-2 are the Designations for NASA-Sponsored...
Search relevance: 28.66 | Views last month: 0 -
THEMIS Ground All Sky Imager at White Horse (61.01 deg GLat, 224.78 deg GLong): 256 x 256 pixel full resolution images of auroral oval. The ASI stations monitor a 170 degree field of view imaging...
Search relevance: 28.66 | Views last month: 0 -
THEMIS Ground All Sky Imager at Gillam (56.35 deg GLat, 265.34 deg GLong): 256 x 256 pixel full resolution images of auroral oval. The ASI stations monitor a 170 degree field of view imaging the...
Search relevance: 28.66 | Views last month: 0 -
THEMIS Ground All Sky Imager at Kiana (66.97 deg GLat, 199.56 deg GLong): 256 x 256 pixel full resolution images of auroral oval. The ASI stations monitor a 170 degree field of view imaging the...
Search relevance: 28.66 | Views last month: 0 -
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...
Search relevance: 28.66 | Views last month: 0 -
THEMIS Ground All Sky Imager at Fort Smith (60.03 deg GLat, 248.07 deg GLong): 32 x 32 pixel thumbnails for full ASI images. The ASI stations monitor a 170 degree field of view imaging the...
Search relevance: 28.66 | Views last month: 0 -
Synoptic (or Carrington) Maps comprise an efficient method to summarize both short term and long term coronal evolution. This resource contains East and West limb maps from the Cor1 and Cor2...
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The IMAGE extreme ultraviolet (EUV) imager detects resonantly scattered solar EUV photons with a wavelength of 30.4 nm that have been resonantly scattered by singly ionized helium (Sandel et al.,...
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The Percent Polarized data from the LASCO C2 coronagraphLASCO (Large Angle Spectroscopic Coronagraph) is comprised of three nested coronagraphs (C1, C2, and C3) that image the solar corona from...
Search relevance: 28.66 | Views last month: 0 -
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...
Search relevance: 28.66 | Views last month: 0 -
The LASCO C3 Calibrated FITS Data. LASCO (Large Angle Spectroscopic Coronagraph) is comprised of three nested coronagraphs (C1, C2, and C3) that image the solar corona from 1.1--30 solar radii...
Search relevance: 28.56 | Views last month: 7
