AndreaBozzo/ceres-open-data-index huggingface dataset:
GOES-R Series Level 1b EXIS X-Ray Sensor (XRS) Science-Quality Products

The GOES-R Extreme Ultraviolet and X-Ray Irradiance Sensors (EXIS) X-Ray Sensor (XRS) Level 1b science-quality data contain 1-second cadence soft X-Ray irradiance measurements covering 0.05nm - 0.4nm (Channel A) and 0.1-0.8 nm (Channel B) integrated passbands. Each channel has two irradiance sensors to capture the full dynamic range of the solar X-Ray irradiance.

This science-quality dataset is produced by NOAAâs National Centers for Environmental Information (NCEI) and utilizes code provided by LASP, and differs from the L1b operational product used at the NOAA Space Weather Prediction Center (SWPC) in that it incorporates retrospective fixes for issues in the operational product and uses the most recent calibrations. The science-quality data have been reprocessed from the start of the mission to the present date. Both the science-quality and the operational data sets contain recovered data due to spurious dropouts.

Tags: doc/noaa/nesdis/ncei, earth magnetic field, earth science, exis-xrs-goesr, geostationary operational environmental satellite 16, geostationary operational environmental satellite 17, geostationary operational environmental satellites, goes, goes (geostationary operational environmental satellite), goes-16, goes-17, magnetosphere (other), national centers for environmental information, nesdis, noaa, noaa geostationary operational environmental satellites, noaa onestop project, solar activity, solar x-ray emissions, solar/space observation satellites, solar/space observing instruments, space, sun-earth interactions, temporal resolution range: 1 second - < 1 minute, u.s. department of commerce, x-ray sensor, x-ray sensor on goes-r series, x-ray/gamma ray detectors, xrs
Organization: National Oceanic and Atmospheric Administration, Department of Commerce
Global Oscillation Network Group (GONG) H-alpha Outputs (oHA)

Originally constructed in 1995, the Global Oscillation Network Group (GONG) is a network of six identical ground-based solar telescopes distributed around the Earth in order to obtain continuous observations of the Sun.  Those sites are located in Big Bear, California (BB); Mauna Loa, Hawaii (ML); Learmonth, Australia (LE); Udaipur, India (UD); El Teide, Spain (TD); and Cerro Tololo, Chile (CT).  Additionally, there are three engineering/testbed sites in Boulder, Colorado (TC, TE, and TS).  Owned by the National Science Foundation, GONG is operated and maintained by the National Solar Observatory (NSO) with significant funding from NOAAâs Space Weather Prediction Center (SWPC).  Each minute, weather permitting, the GONG network observes the Sun at two spectral wavelengths: 676.78nm (a Ni I absorption line) and 656.28nm (the H-alpha absorption line).

Tags: doc/noaa/nesdis/ncei, earth science, global oscillation network group, global oscillation network group instrument, global oscillation network group network, gong, gong instrument, gong network, ionosphere/magnetosphere dynamics, magnetic fields/magnetic currents, national centers for environmental information, nesdis, noaa, solar activity, solar flares, sun-earth interactions, u.s. department of commerce
Organization: National Oceanic and Atmospheric Administration, Department of Commerce
GOES-R Series Level 1b SEISS Magnetospheric Particle Sensor High Energy (MPS-HI) Product in Daily Aggregations

The GOES-R Magnetospheric Electrons and Protons: Medium and High Energy (MPSH) Product consists of fluxes of medium and high energy electrons and protons derived from in situ measurements of electron and proton count rates. The Magnetospheric Particle Sensor High (MPS-HI) makes these measurements. MPS-HI consists of ten solid state telescopes, five for electrons and five for protons, that define a 170-degree fan-like field-of-regard in the north-south plane. Differential and integral electron fluxes are reported at eleven energy bands from each electron telescope. Ten of the energy bands are evenly spaced logarithmically spanning from 50 keV to 4 MeV with differential electron flux being reported. The eleventh energy band collects electrons with energies greater than 2 MeV with electron integral flux being reported. In addition, differential proton fluxes are reported at eleven energy bands from each proton telescope. The eleven proton energy bands are evenly spaced logarithmically and range from 80 keV to 12 MeV. In addition, the product contains ionizing radiation doses in two energy deposition ranges, 50 keV to 1 MeV (low linear energy transfer, LOLET) and 1 MeV to 50 MeV (high linear energy transfer, HILET). The product also contains processing and data quality metadata, satellite state and location information, and data required for the generation of level 2 products. Measurement resolution is one second. NOAA's National Centers for Environmental Information (NCEI) has created these daily files by aggregating the official L1b files produced by the GOES-R Ground System. The granular L1b files each span 30 seconds of observations.

Tags: earth magnetic field, earth science, geostationary operational environmental satellite 16, geostationary operational environmental satellite 17, geostationary operational environmental satellites, goes, goes (geostationary operational environmental satellite), goes-16, goes-17, ionosphere/magnetosphere dynamics, magnetosphere (other), noaa onestop project, particle detectors, proton flux, seiss-goesr, solar energetic particle flux, solar/space observation satellites, solar/space observing instruments, space, sun-earth interactions, temporal resolution range: 1 second - < 1 minute
Organization: National Oceanic and Atmospheric Administration, Department of Commerce
NOAA Space Environment Monitor (SEM) Science-Quality Extreme Ultraviolet (EUVS) Data from GOES 13 - 15

The Space Environment Monitor (SEM) Extreme Ultraviolet Sensor (EUVS) onboard the GOES satellite series measure the EUV in 5 GOES wavelength bands (A-E) from about 5-127 nm. This data is used to investigate solar activity and the associated impacts of extreme and middle ultraviolet absorption on the earth's atmosphere. This data collection includes Reprocessed Level-1b and Level-2 SEM/EUVS
               data from GOES 13-15, channels A-E. The data are enhanced to science quality from the original operational archive. Enhancements include corrected calibrations, updated quality flagging, full ephemeris information, and both high-cadence and averaged data. The data were produced by NOAAâs National Centers for Environmental Information (NCEI) and archived by NOAA's Comprehensive Large Array-Data Stewardship System (CLASS).

Tags: astrophysics and astronomy, atmosphere, atmosphere radiation, doc/noaa/nesdis/ncei, earth science, euvs, extreme ultraviolet sensor, geostationary operational environmental satellite - 13, geostationary operational environmental satellite - 14, geostationary operational environmental satellite - 15, goes-13, goes-14, goes-15, national centers for environmental information, nesdis, noaa, solar physics, u.s. department of commerce, ultraviolet emissions, ultraviolet radiation
Organization: National Oceanic and Atmospheric Administration, Department of Commerce
Solar/Space Environment Data (Satellites)

The National Oceanic and Atmospheric Administration (NOAA) monitors the geospace and solar environments using a variety of space weather sensors aboard its fleet of operational satellites.

Tags: doc/noaa/nesdis/ncei, doc/noaa/nesdis/ngdc, earth magnetic field, earth science, icsu-wds, international council for science - world data system, national centers for environmental information, national geophysical data center, nesdis, noaa, noaa - space weather program, solar activity, solar energetic particle flux, solar region, solar/space observing instruments, solar/space observing satellites, space, sun-earth interactions, u.s. department of commerce
Organization: National Oceanic and Atmospheric Administration, Department of Commerce
GOES-R Series Level 1b Solar Ultraviolet Imager (SUVI) Product in FITS Format

The Solar Ultraviolet Imager (SUVI) Level 1b Solar Imagery: X-Ray product contains an image of the Sun at one of six wavelengths with different exposure times, and metadata required for exploitation and higher level processing. This product also contains an array containing a quality flag for each pixel in the solar image.
            
            Files for Sept. 2017 are test files produced by NOAA's National Centers for Environmental Information in Boulder, Colorado. The currently available data are processed from Level-0 SUVI files in Boulder, and are not necessarily representative of what data SUVI users will encounter in GOES-R Rebroadcast (GRB) produced by the GOES-R Ground Segment. The file metadata are populated with as much information as possible for users to interpret these observations, but some fields may be missing. Users requiring assistance with these files can contact the NCEI SUVI team by emailing goesr.suvi@noaa.gov.

Tags: corona, corona holes, coronal mass ejections, earth science, geostationary operational environmental satellites, goes, goes (geostationary operational environmental satellite), solar active regions, solar activity, solar flares, solar imagery, solar prominences/solar filaments, solar ultraviolet emissions, solar/space observation satellites, solar/space observing instruments, spectral/engineering, sun-earth interactions, sunspots, suvi-goesr, ultraviolet instruments, ultraviolet radiance, ultraviolet wavelengths
Organization: National Oceanic and Atmospheric Administration, Department of Commerce
Wang-Sheeley-Arge (WSA)-Enlil Solar Wind Prediction

Wang-Sheeley-Arge (WSA)-Enlil is a large-scale, physics-based prediction model of the heliosphere, used by the Space Weather Forecast Office to provide 1-4 day advance warning of solar wind structures and Earth-directed coronal mass ejections (CMEs) that cause geomagnetic storms.  Solar disturbances have long been known to disrupt communications, wreak havoc with geomagnetic systems, and to pose dangers for satellite operations.

Tags: doc/noaa/nesdis/ncei, doc/noaa/nesdis/ngdc, fgm, icsu-wds, international council for science - world data system, magnetic field/electric field instruments, magnetographs, national centers for environmental information, national geophysical data center, nesdis, noaa, noaa - space weather program, solar/space observation satellites, solar/space observing instruments, space, sun-earth interactions, u.s. department of commerce
Organization: National Oceanic and Atmospheric Administration, Department of Commerce
GOES-R Series Level 1b EXIS  Extreme Ultraviolet Sensor (EUVS) Product in Daily Aggregations

The GOES-R Extreme Ultraviolet and X-Ray Irradiance Sensors (EXIS) Extreme Ultraviolet Sensor (EUVS) measures solar spectral irradiance at discrete wavelengths between 25 and 141 nm and in the vicinity of 280 nm. GOES-R EUVS makes extreme ultraviolet (EUV) and far ultraviolet (FUV) high-spectral-resolution measurements of distinct solar emission lines representative of different layers of the solar atmosphere. The L1b data products derived from EUVS observations are irradiances for seven solar lines, the Magnesium core-to-wing ratio (i.e., the Mg II index), and EUV proxy spectra from 5 to 127 nm. The nominal data cadence is 30-seconds.

Tags: and astronomy, astrophysics, atmosphere, atmospheric radiation, doc/noaa/nesdis/ncei, earth science, euvs, exis-euvs-goesr, extreme ultraviolet sensor on goes-r series, geostationary operational environmental satellite 16, geostationary operational environmental satellite 17, geostationary operational environmental satellites, goes, goes (geostationary operational environmental satellite), goes-16, goes-17, national centers for environmental information, nesdis, noaa, noaa geostationary operational environmental satellites, noaa onestop project, solar extreme ultraviolet spectrophotometer, solar physics, solar/space observation satellites, temporal resolution range: 1 second - < 1 minute, u.s. department of commerce, ultraviolet emissions, ultraviolet radiation
Organization: National Oceanic and Atmospheric Administration, Department of Commerce
NOAA Space Environment Monitor (SEM) Science-Quality Magnetometer (MAG) Data from GOES 8-15

The Space Environment Monitor (SEM) Magnetometer (MAG) instrument onboard the GOES satellite series measures the magnitude and direction of the Earth's ambient magnetic field in geosynchronous orbit. This data collection includes Reprocessed Level-1b and Level-2 SEM/MAG data from GOES 8-15. The data are enhanced to science quality from the original operational archive. Enhancements include the highest temporal cadence (2Hz), recomputed means, corrected calibration parameters, updated quality flagging, vector measurements in geophysically relevant coordinates, and full ephemeris information. The data were produced by NOAAâs National Centers for Environmental Information (NCEI) and archived by NOAA's Comprehensive Large Array-Data Stewardship System (CLASS).

Tags: doc/noaa/nesdis/ncei, earth science, geomagnetic forecasts, geomagnetic indices, geomagnetism, geostationary operational environmental satellite - 10, geostationary operational environmental satellite - 11, geostationary operational environmental satellite - 12, geostationary operational environmental satellite - 13, geostationary operational environmental satellite - 14, geostationary operational environmental satellite - 15, geostationary operational environmental satellite - 8, geostationary operational environmental satellite - 9, goes-10, goes-11, goes-12, goes-13, goes-14, goes-15, goes-8, goes-9, ionosphere/magnetosphere dynamics, mag, magnetic fields/magnetic currents, magnetic storms, magnetometer, national centers for environmental information, nesdis, noaa, solid earth, sun-earth interactions, u.s. department of commerce
Organization: National Oceanic and Atmospheric Administration, Department of Commerce
GOES-R Series Level 1b SEISS Magnetospheric Particle Sensor High Energy (MPS-HI) Product in Daily Aggregations

The GOES-R Magnetospheric Electrons and Protons: Medium and High Energy (MPSH) Product consists of fluxes of medium and high energy electrons and protons derived from in situ measurements of electron and proton count rates. The Magnetospheric Particle Sensor High (MPS-HI) makes these measurements. MPS-HI consists of ten solid state telescopes, five for electrons and five for protons, that define a 170-degree fan-like field-of-regard in the north-south plane. Differential and integral electron fluxes are reported at eleven energy bands from each electron telescope. Ten of the energy bands are evenly spaced logarithmically spanning from 50 keV to 4 MeV with differential electron flux being reported. The eleventh energy band collects electrons with energies greater than 2 MeV with electron integral flux being reported. In addition, differential proton fluxes are reported at eleven energy bands from each proton telescope. The eleven proton energy bands are evenly spaced logarithmically and range from 80 keV to 12 MeV. In addition, the product contains ionizing radiation doses in two energy deposition ranges, 50 keV to 1 MeV (low linear energy transfer, LOLET) and 1 MeV to 50 MeV (high linear energy transfer, HILET). The product also contains processing and data quality metadata, satellite state and location information, and data required for the generation of level 2 products. Measurement resolution is one second. NOAA's National Centers for Environmental Information (NCEI) has created these daily files by aggregating the official L1b files produced by the GOES-R Ground System. The granular L1b files each span 30 seconds of observations.

Tags: doc/noaa/nesdis/ncei, earth magnetic field, earth science, geostationary operational environmental satellites, goes, goes (geostationary operational environmental satellite), ionosphere/magnetosphere dynamics, magnetosphere (other), national centers for environmental information, nesdis, noaa, noaa onestop project, particle detectors, proton flux, seiss-goesr, solar energetic particle flux, solar/space observation satellites, solar/space observing instruments, space, sun-earth interactions, temporal resolution range: 1 second - < 1 minute, u.s. department of commerce
Organization: National Oceanic and Atmospheric Administration, Department of Commerce
Geostationary Operational Environmental Satellite, R-Series (GOES-R) Extreme Ultraviolet X-Ray Irradiance Sensors (EXIS) Level 2 Products

The EUV and X-Ray Irradiance Sensors (EXIS) measures solar irradiance at the very short wavelengths where the Sun's output varies the most. EXIS has two primary components, the X-Ray Sensor (XRS) and the Extreme Ultraviolet Sensor (EUVS). EXIS Level 2 data are used by NOAAâs Space Weather Prediction Center to produce warnings for radio blackouts when large flares occur. EXIS extreme ultraviolet data is used in models to help determine upper atmospheric densities which impact satellite orbits. EXIS Level 2 data products include measurements of irradiances in two X-ray bands, seven lines at extreme and far ultraviolet wavelengths, and the Magnesium II index, The EXIS products are at multiple cadences including high resolution data of 1 to several seconds as well as 1-minute and daily averages. Other products include flare summaries, flare locations and extreme ultraviolet spectra generated by a proxy model.  Data are in NetCDF-4 format.

Tags: earth magnetic field, earth science, exis-euvs-goesr, exis-xrs-goesr, geostationary operational environmental satellites, goes, goes (geostationary operational environmental satellite), magnetosphere (other), noaa onestop project, solar activity, solar irradiance, solar ultraviolet emissions, solar x-ray emissionsx, solar/space observation satellites, solar/space observing instruments, space, sun-earth interactions, ultraviolet instruments, x-ray/gamma ray detectors
Organization: National Oceanic and Atmospheric Administration, Department of Commerce
NOAA Space Environment Monitor (SEM) Science-Quality Solar X-Ray Sensor (XRS) Data from GOES 1-15

The Space Environment Monitor (SEM) Solar X-Ray Sensor (XRS) onboard the GOES satellite series provides solar X-ray irradiances for the wavelength bands of 0.5 to 4 Angstrom (short channel) and 1 to 8 Angstrom (long channel). This data is used to track solar activity including solar flares. Large solar X-ray flares can change the Earthâs ionosphere, which blocks high-frequency (HF) radio transmissions on the sunlit side of the Earth. Solar flares are also associated with Coronal Mass Ejections (CMEs) which can ultimately lead to geomagnetic storms. This data collection includes Reprocessed Level-2 SEM/XRS data from GOES 1-15. The data are enhanced to science quality from the original operational archive. Enhancements include corrected calibrations, updated quality flagging, full ephemeris information, high-cadence and averaged data, and summaries of flare events. The data were produced by NOAAâs National Centers for Environmental Information (NCEI) and archived by NOAA's Comprehensive Large Array-Data Stewardship System (CLASS).

Tags: doc/noaa/nesdis/ncei, earth science, geostationary operational environmental satellite - 1, geostationary operational environmental satellite - 10, geostationary operational environmental satellite - 11, geostationary operational environmental satellite - 12, geostationary operational environmental satellite - 13, geostationary operational environmental satellite - 14, geostationary operational environmental satellite - 15, geostationary operational environmental satellite - 2, geostationary operational environmental satellite - 3, geostationary operational environmental satellite - 4, geostationary operational environmental satellite - 5, geostationary operational environmental satellite - 6, geostationary operational environmental satellite - 7, geostationary operational environmental satellite - 8, geostationary operational environmental satellite - 9, goes-1, goes-10, goes-11, goes-12, goes-13, goes-14, goes-15, goes-2, goes-3, goes-4, goes-5, goes-6, goes-7, goes-8, goes-9, national centers for environmental information, nesdis, noaa, solar activity, solar events, solar flares, solar physics, solar x-ray emissions, spectral/engineering, sun-earth interactions, u.s. department of commerce, x-ray, x-ray flux, x-ray irradiance, x-ray sensor, xrs
Organization: National Oceanic and Atmospheric Administration, Department of Commerce
Space Weather Products

Collection includes a variety of space weather datasets from the National Oceanic and Atmospheric Administration and from the World Data Service for Geophysics, Boulder.

Tags: chromosphere, corona, doc/noaa/nesdis/ncei, doc/noaa/nesdis/ngdc, icsu-wds, international council for science - world data system, national centers for environmental information, national geophysical data center, nesdis, noaa, noaa - space weather program, photosphere, solar active regions, solar activity, solar imagery, solar observatory stations, solar region, solar synoptic maps, solar telescope, space, sun-earth interactions, sunspots, u.s. department of commerce
Organization: National Oceanic and Atmospheric Administration, Department of Commerce
Global Oscillation Network Group (GONG) Quick-Reduce Inputs (iQR)

Originally constructed in 1995, the Global Oscillation Network Group (GONG) is a network of six identical ground-based solar telescopes distributed around the Earth in order to obtain continuous observations of the Sun.  Those sites are located in Big Bear, California (BB); Mauna Loa, Hawaii (ML); Learmonth, Australia (LE); Udaipur, India (UD); El Teide, Spain (TD); and Cerro Tololo, Chile (CT).  Additionally, there are three engineering/testbed sites in Boulder, Colorado (TC, TE, and TS).  Owned by the National Science Foundation, GONG is operated and maintained by the National Solar Observatory (NSO) with significant funding from NOAAâs Space Weather Prediction Center (SWPC).  Each minute, weather permitting, the GONG network observes the Sun at two spectral wavelengths: 676.78nm (a Ni I absorption line) and 656.28nm (the H-alpha absorption line).

Tags: doc/noaa/nesdis/ncei, earth science, global oscillation network group, global oscillation network group instrument, global oscillation network group network, gong, gong instrument, gong network, ionosphere/magnetosphere dynamics, magnetic fields/magnetic currents, national centers for environmental information, nesdis, noaa, sun-earth interactions, u.s. department of commerce
Organization: National Oceanic and Atmospheric Administration, Department of Commerce