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Solar Terrestrial Relations Observatory-A (STEREO-A), Hourly Data
The NSSDC Coordinated Heliospheric Observations Web, COHOWeb, hourly and daily Solar-Terrestrial Relations Observatory-A, STEREO-B, data were made by using high resolution data... -
STEREO-A In-Situ Measurements of Particles and CME Transients (IMPACT) Solar...
The file contains Level 1 3D electron distributions from the In-situ Measurements of Particles and CME Transients, IMPACT, SWEA instrument on the STEREO Ahead spacecraft. For... -
STEREO-A In-Situ Measurements of Particles and CME Transients (IMPACT) Solar...
The file contains Level 1 3D electron distributions in burst mode from the In-situ Measurements of Particles and CME Transients, IMPACT, SWEA instrument on the STEREO Ahead... -
STEREO-A IMPACT (In-Situ Measurements of Particles and CME Transients)...
The IMPACT Suprathermal Ion Telescope (SIT) data consist of 1-min resolution ion fluxes of the following species (and numbers of energy bands, typically spanning ~0.04-9 MeV/n):... -
STEREO-A multi-instrument Level 1 IMPACT data from UCB
Level 1 data from each of the several IMPACT instruments, in CDF. Time resolutions range from 0.125s (MAG) to 1m (SEPT, LET, HET). Full spectral and directional resolution is... -
STEREO-A IMPACT (In-Situ Measurements of Particles and CME Transients) Low...
The IMPACT Low Energy Telescope (LET) data consist of 1-min resolution unsectored fluxes and counts for each of 15 single-Z ionic species at each of a species-dependent number... -
STEREO-A Ephemeris, Heliocentric Trajectories, Heliographic, Heliographic...
STEREO-A Heliocentric orbit in Heliographic Inertial, Heliographic rotating, and Solar Ecliptic coordinates at a 1 hourly cadence. For coordinate definitions see... -
STEREO-A Ephemeris, Heliocentric Trajectories, Heliographic, Heliographic...
STEREO-A Heliocentric orbit in Heliographic Inertial, Heliographic rotating, and Solar Ecliptic coordinates at a daily cadence. For coordinate definitions see... -
STEREO-A Ephemeris in the HEEQ Coordinate System
STEREO atttitude and orbit data are distributed as SPICE kernels. Since most SEP investigators would rather not deal with SPICE kernels, Caltech provides text files containing... -
STEREO-A Ephemeris in the HEE Coordinate System
STEREO atttitude and orbit data are distributed as SPICE kernels. Since most SEP investigators would rather not deal with SPICE kernels, Caltech provides text files containing... -
STEREO-A Ephemeris in the HCI Coordinate System
STEREO atttitude and orbit data are distributed as SPICE kernels. Since most SEP investigators would rather not deal with SPICE kernels, Caltech provides text files containing... -
STEREO-A Ephemeris in the GSM Coordinate System
STEREO atttitude and orbit data are distributed as SPICE kernels. Since most SEP investigators would rather not deal with SPICE kernels, Caltech provides text files containing... -
STEREO-A Ephemeris
STEREO atttitude and orbit data are distributed as SPICE kernels. Since most SEP investigators would rather not deal with SPICE kernels, Caltech provides text files containing... -
STEREO-A Ephemeris in the GEI Coordinate System
STEREO atttitude and orbit data are distributed as SPICE kernels. Since most SEP investigators would rather not deal with SPICE kernels, Caltech provides text files containing... -
SOHO UVCS Data
The primary scientific goals of the UVCS (UltraViolet Coronagraph Spectrometer) are to: (1) locate and characterize the coronal source regions of the solar wind; (2) identify... -
SOHO MDI Line Of Sight (LOS) Velocity Data
Line of sight magnetic field inferred from the frequency/wavelength Zeeman splitting between opposite circular polarizations of a magnetically-sensitive line. -
SOHO/MDI Line Of Sight (LOS) Magnetic Field Data
Line of sight magnetic field inferred from the frequency/wavelength Zeeman splitting between opposite circular polarizations of a magnetically-sensitive line. -
SOHO LASCO C3 Polarized Brightness FITS Data
The Polarized Brightness data from the LASCO C3 coronagraph. LASCO (Large Angle Spectroscopic Coronagraph) is comprised of three nested coronagraphs (C1, C2, and C3) that image... -
SOHO LASCO C3 Level 1.0 FITS Data
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... -
SOHO LASCO C3 Percent Polarized FITS Data
The Percent Polarized data from the LASCO C3 coronagraph. LASCO (Large Angle Spectroscopic Coronagraph) is comprised of three nested coronagraphs (C1, C2, and C3) that image the...