Search datasets
-
The AIM Cloud Imaging and Particle Size instrument (CIPS) is a panoramic imager that measures solar ultraviolet radiation scattered by the atmosphere back to the satellite. The fundamental...
Search relevance: 1.00 | Views last month: 15 | Catalog Last Checked: August 12, 2026 at 12:57 AM -
The LASCO C2 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: 1.00 | Views last month: 13 | Catalog Last Checked: August 12, 2026 at 12:06 AM -
The SDO/AIA Level 1 FITS Data. The Atmospheric Imaging Assembly (AIA) onboard Solar Dynamics Observatory (SDO) focuses on the evolution of the magnetic environment in the Sun’s atmosphere, and...
Search relevance: 1.00 | Views last month: 11 | Catalog Last Checked: August 12, 2026 at 12:06 AM -
The SDO/AIA 94 Ã… Level 1 FITS Data. The 94 Ã… channel observes the Fe XVIII line from 6.3 MK flaring plasma. The Atmospheric Imaging Assembly (AIA) onboard Solar Dynamics Observatory (SDO)...
Search relevance: 1.00 | Views last month: 8 | Catalog Last Checked: August 12, 2026 at 12:06 AM -
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: 1.00 | Views last month: 7 | Catalog Last Checked: August 12, 2026 at 12:06 AM -
Parker Solar Probe Wide-Field (WISPR) Imager de-compressed, uncalibrated integer-value image data. The images are rectified so that the top right corner of the image corresponds to spacecraft +X,...
Search relevance: 1.00 | Views last month: 5 | Catalog Last Checked: August 12, 2026 at 12:08 AM -
The "AIA Active Region Patches" comprise an unbiased multi-wavelength set of FITS files of data extracted from SDO/AIA full-disk data. The spatial extractions are based on SDO/HMI "Active Region...
Search relevance: 1.00 | Views last month: 4 | Catalog Last Checked: August 12, 2026 at 12:36 AM -
The SDO/AIA 131 Ã… Level 1 FITS Data. The 131 Ã… channel observes the Fe xx and Fe xxiii lines from 10 MK and 16 MK flaring plasma, respectively. The Atmospheric Imaging Assembly (AIA) onboard...
Search relevance: 1.00 | Views last month: 4 | Catalog Last Checked: August 12, 2026 at 12:06 AM -
The HMI continuum data refers to map of the continuum intensity of the solar spectrum in the region of the Fe I absorption line at 6173 â„« on the surface of the sun. HMI samples the Fe I...
Search relevance: 1.00 | Views last month: 4 | Catalog Last Checked: August 12, 2026 at 12:36 AM -
The SDO/AIA 304 Ã… Level 1 FITS Data. The 304 Ã… channel observes the He ii line from chromosphere and transition region (0.50 MK). The Atmospheric Imaging Assembly (AIA) onboard Solar Dynamics...
Search relevance: 1.00 | Views last month: 4 | Catalog Last Checked: August 12, 2026 at 12:36 AM -
The Polarized Brightness data from the LASCO C2 coronagraph. LASCO (Large Angle Spectroscopic Coronagraph) is comprised of three nested coronagraphs (C1, C2, and C3) that image the solar corona...
Search relevance: 1.00 | Views last month: 4 | Catalog Last Checked: August 12, 2026 at 12:06 AM -
THEMIS Ground All Sky Imager at Sanikiluaq (56.54 deg GLat, 280.77 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: 1.00 | Views last month: 4 | Catalog Last Checked: August 12, 2026 at 12:33 AM -
The Heliospheric Imager-1 (HI-1) telescope is part of the Sun Earth Connection Coronal and Heliospheric Investigations (SECCHI) instrument suite on the NASA STEREO mission. The SECCHI on the two...
Search relevance: 1.00 | Views last month: 4 | Catalog Last Checked: August 12, 2026 at 12:35 AM -
The SDO/AIA Level 1.5 Synoptic FITS Data. The AIA Synoptic FITS data are reduced to 1024x1024 2.4 arc-sec pixels by summing with pixel value in DN per original 0.6 arc-sec pixel. The data...
Search relevance: 1.00 | Views last month: 4 | Catalog Last Checked: August 12, 2026 at 12:06 AM -
The Extreme Ultraviolet Imager (EUVI) is part of the Sun Earth Connection Coronal and Heliospheric Investigations (SECCHI) instrument suite on the NASA STEREO mission. The SECCHI on the two STEREO...
Search relevance: 1.00 | Views last month: 4 | Catalog Last Checked: August 12, 2026 at 12:36 AM -
SHARP Near Real Time data in the Cylindrical Equal Area (CEA) Cartesian coordinate. SHARP stands for Space-weather HMI Active Region Patch. A SHARP is a DRMS series that contains (1) various...
Search relevance: 1.00 | Views last month: 3 | Catalog Last Checked: August 12, 2026 at 12:36 AM -
This describes the data produce for ICON EUV Daytime O+ (DP 2.6), which is in NetCDF4 format. These files are named ICON_L2-6_EUV_YYYY-MM-DD_vXXrZZ.NC, where YYYY-MM-DD is the year month day and...
Search relevance: 1.00 | Views last month: 3 | Catalog Last Checked: August 12, 2026 at 12:46 AM -
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: 1.00 | Views last month: 3 | Catalog Last Checked: August 12, 2026 at 12:33 AM -
The Ultraviolet Imager (UVI) is a small camera that detected and produced images of the ultraviolet light of the aurora, day and night. Using any of five specially designed filters the UVI camera...
Search relevance: 1.00 | Views last month: 3 | Catalog Last Checked: August 12, 2026 at 12:40 AM -
The GOLD night disk scan (NI1) measurements are used to derive the peak electron density (NMAX, electrons/cm3) on the disk. GOLD performs NI1 scans in both hemispheres from 17:00 to 21:00 hours...
Search relevance: 1.00 | Views last month: 3 | Catalog Last Checked: August 12, 2026 at 12:12 AM