AndreaBozzo/ceres-open-data-index huggingface dataset:
Polar Definitive Attitude, 10 min Data, Spin Axis Orientation Angles in GCI, GSE and GSM Coordinates

Polar Definitive Attitude Body Spin Rate and Spin Axis Orientation Right Ascension and Declination Angles in Geocentric Celestial Inertial, GCI, Geocentric Solar Ecliptic, GSE, and Geocentric Solar Magnetospheric, GSE, Coordinates

Tags: ephemeris
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RPCMIP/RPCLAP 5 ESC3 V1.0

This archive contains cross-calibrated data from the RPC-MIP and RPC-LAP instruments on-board ROSETTA Orbiter acquired during the COMET ESCORT 3 mission phase. Observations are performed in the vicinity of comet 67P/C-G. It also contains documentation which describes the RPC-MIP experiment. The data archived in this data set conform to the Planetary Data System Standards, Version 3.6.

Tags: __
Organization: National Aeronautics and Space Administration
STARDUST NAVCAM RAW IMAGES OF WILD 2 - VERSION 3.0

This data set contains EDR (raw) pre-encounter and encounter images taken by the Stardust Navigation Camera of comet 81P/Wild 2 (1978 A2). This is a new version of a subset of an existing data set, based on work done during the Stardust-NExT mission. The updated calibration from the Stardust-NExT mission was applied to these data in a separate data set (similar name: Level 3; RDR). Changes in the calibration of the NAVCAM instrument, between these prime mission data and those of the Stardust-NExT mission, are a possibility and are addressed in [KLAASENETAL2011B].

Tags: __
Organization: National Aeronautics and Space Administration
Biome-BGC: Terrestrial Ecosystem Process Model, Version 4.1.1

Biome-BGC is a computer program that estimates fluxes and storage of energy, water, carbon, and nitrogen for the vegetation and soil components of terrestrial ecosystems. The primary model purpose is to study global and regional interactions between climate, disturbance, and biogeochemical cycles.Biome-BGC represents physical and biological processes that control fluxes of energy and mass. These processes include: New leaf growth and old leaf litterfall Sunlight interception by leaves and penetration to the ground Precipitation routing to leaves and soil Snow accumulation and melting Drainage and runoff of soil water Evaporation of water from soil and wet leaves Transpiration of soil water through leaf stomata Photosynthetic fixation of carbon from CO2 in the air Uptake of nitrogen from the soil Distribution of carbon and nitrogen to growing plant parts Decomposition of fresh plant litter and old soil organic matter Plant mortality Fire The model uses a daily time-step. This means that each flux is estimated for a one-day period. Between days, the program updates its memory of the mass stored in different components of the vegetation, litter, and soil. Weather is the most important control on vegetation processes. Flux estimates in Biome-BGC depend strongly on daily weather conditions. Model behavior over time depends on climate--the history of these weather conditions.A companion file with more information about Biome-BGC and its components is available at ftp://daac.ornl.gov/data/model_archive/BIOME_BGC/biome_bgc_4.1.1/comp/BiomeBGC_v411_release.pdf .Biome-BGC, Version 4.1.1 was developed and is maintained by the Numerical Terradynamic Simulation Group, School of Forestry, The University of Montana, Missoula, Montana, USA. Additional information can be found on there web site at: http://www.ntsg.umt.edu/.

Tags: earth-science-ecological-dynamics-biosphere-ecosystem-functions-biogeochemical-cycles, earth-science-soils-land-surface-carbon, earth-science-soils-land-surface-nitrogen, earth-science-soils-land-surface-soil-heat-budget, earth-science-soils-land-surface-soil-moisture-water-content
Organization: National Aeronautics and Space Administration
CSSWE REPTile Level 1 6-s Counts and Position

This data set contains Level 1 corrected count rates from the Relativistic Electron and Proton Telescope integrated little experiment (REPTile)on board the Colorado Student Space Weather Experiment (CSSWE) CubeSat. Electron counts are provided for 0.5-1.7 MeV, 1.7-3.3 MeV, and >3.3 MeV. Proton counts are provided for 9-18 MeV, 19-30 MeV, and 30-40 MeV. All counts, in units of number per 6 seconds, have been corrected for transmission and temperature noise. L is calculated using the IGRF magnetic field model. Geographic latitude, longitude and altitude (km) are provided.

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P SREM 2 EXTENSION 3 MTP031 V1.0

This data set contains count rates (1/s) as measured by the Standard Radiation Environment Monitor (SREM) instrument on the Rosetta spacecraft, along with their standard deviations. The primary target is comet 67P/Churyumov-Gerasimenko. These are CODMAC Level 2 Experiment Data Record data, and provide a measure of the radiation in the spacecraft environment during the Medium Term Plan 31 period of the EXTENSION 3 mission phase.

Tags: __
Organization: National Aeronautics and Space Administration
MARS EXPLORATION ROVER 1 RADIO SCIENCE SUBSYSTEM EDR V1.0

The Mars Exploration Rover 2 (MER1) Radio Science (RS) data archive contains raw radio tracking data collected during the surface lifetime of the MER1 Rover. The data contain potentially valuable information on the rotation dynamics of Mars, extending the previous data available from the Viking and Mars Pathfinder landers. For more information on the earlier investigations see [FOLKNERETAL1997A].

Tags: __
Organization: National Aeronautics and Space Administration
MARS EXPRESS ASPERA-3 RAW-CAL NTRL PARTICLE IMAGER EXT4 V1.0

This data set contains Mars Express ASPERA-3 Neutral         Particle Imager (NPI) data for the fourth mission extension         (January 1, 2013 - Dec. 31, 2014).  These data are provided         in units of count rate (counts/second).

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSIWAC 4 EXT3-MTP031 RDR-STR-REFL V1.0

This CODMAC level 4 data set contains solar stray light corrected, radiometric calibrated and geometric distortion corrected (resampled) image data in in reflectance units (normalized and thus without unit), acquired by the OSIRIS Wide Angle Camera on the Rosetta spacecraft during the ROSETTA EXTENSION 3 mission phase, covering the period from 2016-06-28T23:25:00.000 to 2016-07-26T23:24:59.000. The prime target is comet 67P/Churyumov-Gerasimenko 1 (1969 R1). This version V1.0 is the first version of this dataset: Lien corrected dataset after October 2018 PSA/PDS external peer review.

Tags: __
Organization: National Aeronautics and Space Administration
DE 1 Energetic Ion Composition Spectrometer (EICS) Validated Summary Data

This Validated Summary (VS) data set from the DE 1 Energetic Ion Composition Spectrometer (EICS) contains 96-second averaged fluxes (in units of 1/(cm^2-sec-sr-keV) ) for H+, O+, and He+ ions in 15 energy (~0.01 to ~20 keV) and 14 pitch angle bins. It also includes data uncertainties, data quality indicators, and spacecraft position. Data are in CDF format from CDAWeb.

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
Borehole locations and permafrost depths, Alaska, USA, Version 1

The methods utilized by the U.S. Geological Survey to measure subsurface temperatures have evolved considerably over the years. Although some of the early measurements were obtained using thermistor strings frozen into permafrost, the vast majority of the measurements were made in fluid-filled holes using a custom temperature sensor. A typical sensor used in Alaska prior to 1989 consisted of a series-parallel network of 20 thermistors; see Sass et al. [1971] for a more detailed description. During a logging experiment, the resistance of the thermistor network was determined using a Wheatstone bridge prior to 1967. After that time, a 4-wire resistance measurement was made using a commercial 5.5-digit multimeter (DMM). Before 1984, boreholes were logged in the 'incremental' or 'stop-and-go' modes; the vertical spacing of the measurements was typically 3-15 m. Beginning in 1984, the depth/resistance measurements were automatically stored on magnetic tape, allowing boreholes to be logged in the 'continuous' mode; the typical data spacing for the continuous temperature logs was 0.3 m (1 ft). Many of the Alaskan boreholes were re-logged several times to quantify the thermal disturbance caused by drilling the holes (see Lachenbruch and Brewer [1959]). A review of current temperature measuring techniques used by the USGS in the polar regions is given by Clow et al. [1996]. Data from 1950-1989 are included on the CAPS CD-ROM Version 1.0, June 1998.

Tags: earth-science-frozen-ground-cryosphere-permafrost-permafrost, earth-science-frozen-ground-cryosphere-soil-temperature-soil-temperature, earth-science-frozen-ground-land-surface-permafrost-permafrost, earth-science-frozen-ground-land-surface-soil-temperature-soil-temperature
Organization: National Aeronautics and Space Administration
MGS MARS MAG PRE-MAP DETAIL WORD RESOLUTION V1.0

This data set contains vector magnetic field data acquired by the Fluxgate section of the Magnetometer / Electron Reflectometer instrument aboard the Mars Global Surveyor (MGS) spacecraft. The data are provided at a variable time resolution depending on the telemetry rate available to the investigation for the time period beginning with Aerobraking Phase 1A (1997-09-12). The data in the dataset cover the entire premapping period (ends 1999-03-08).

Tags: __
Organization: National Aeronautics and Space Administration
CRRES HEEF electron equatorial distributions vs.L

This data set holds half-orbit (~5 hour) resolution \nelectron distributions (19 5-deg equatorial pitch angles vs. 19 energies) \nfrom the High Energy Electron Fluxmeter (HEEF) on the CRRES spacecraft.  \nThe energy range covered is 0.3-7.5 MeV.  These data are developed from \nthe 1-min insitu pitch angle distributions by assigning each 5-deg bin \nin pitch angle a corresponding McIlwain L value and then by mapping the \ninsitu pitch angle distribution to the equator, into 0.05-wide L bins, \nassuming first adiabatic invariant conservation.  The mapping yields \nequivalent equatorial pitch angles.  Flux data are for a given half-orbit, \ngiven 0.05-wide L bin,  given equatorial pitch angle and given energy bin\nare then averaged.  Data records are for a given half-orbit and given\nL bin; each record contains averaged fluxes vs. equatorial pitch angle\nand energy.  The data are in SGI(UNIX) binary format.  Read software\nis contained within the companion documentation.

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
MARS EXPRESS SUN MRS 1/2/3 EXTENDED MISSION 4 3571 V1.0

This is a Mars Express Radio Science data set, collected during the extended mission phase 2013-01-01 to 2014-12-31. It is a Solar Conjunction measurement and covers the time 2013-04-22T12:32:34 to 2013-04-23T17:31:11.000.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P SREM 2 PRELANDING MTP006 V1.0

This data set contains count rates (1/s) as measured by the Standard Radiation Environment Monitor (SREM) instrument on the Rosetta spacecraft, along with their standard deviations. The primary target is comet 67P/Churyumov-Gerasimenko. These are CODMAC Level 2 Experiment Data Record data, and provide a measure of the radiation in the spacecraft environment during the Medium Term Plan 6 period of the PRELANDING mission phase.

Tags: __
Organization: National Aeronautics and Space Administration
DE 2 Combined Magnetic Field Vector Electric Field data Matrix

Dynamics Explorer 2 Magnetic Field and Vector Electric Field Instrument DC Matrix

Tags: auroral-region, cusp, dynamics-explorer, dynamics-explorer-1, electric-fields, electricfield-0-5-s, ionosphere, magnetic-fields, magneticfield, magnetosphere, matrix, plasmasphere, polar-cap, radiation-belt
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSINAC 4 EXT1-MTP025 RDR-INFLDSTR V1.0

This CODMAC level 4 data set contains solar stray-light corrected, in-field stray-light corrected,  radiometric calibrated and geometric distortion corrected  (resampled) image data in W/m^2/sr/nm,  acquired by the OSIRIS Narrow Angle Camera on the Rosetta spacecraft  during the ROSETTA EXTENSION 1 mission phase, covering the period  from 2016-01-12T23:25:00.000 to 2016-02-09T23:24:59.000. The prime target is comet 67P/Churyumov-Gerasimenko 1 (1969 R1). This version V1.0 is the first version of this dataset: Lien corrected dataset after September 2019 PSA/PDS external peer review.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P MIDAS 3 EXT3 SAMPLES V1.0

The Micro-Imaging Dust Analysis System (MIDAS) is an instrument on theROSETTA Orbiter that will provide 3D images and statistical parametersof pristine cometary particles, collected in the vicinity of comet67P/Churyumov-Gerasimenko. This data setincludes all data from the ROSETTA EXTENSION 3 mission phase.

Tags: __
Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 6 3914 V1.0

This is a Mars Express Radio Science data set, collected during the extended mission phase 2017-01-01 to 2018-12-31. It is a Occultation measurement and covers the time 2018-03-10T06:40:53.000 to 2018-03-10T07:08:31.949.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER COMET PRELANDING OSIWAC 2 EDR DATA MTP 003

This data set contains raw EDR images acquired by the OSIRIS Wide AngleCamera during the prelanding phase of the Rosetta mission at the comet 67P,covering the period from 2014-05-07 to 2014-06-04.

Tags: __
Organization: National Aeronautics and Space Administration
DE 1 Magnetic Field Observations Triaxial Fluxgate Magnetometer (MAG-A)

Dynamics Explorer 1 Magnetic Field Observations Triaxial Fluxgate Magnetometer at 6 second resolution.

Tags: auroral-region, cusp, dynamics-explorer, dynamics-explorer-1, magnetic-fields, magneticfield-6-s, magnetometer, magnetosphere, plasmasphere, polar-cap, radiation-belt, solar-wind
Organization: National Aeronautics and Space Administration
BOREAS RSS-14 GOES-8 Level-1 Visible, Infrared and Water Vapor Images

The BOREAS RSS-14 team collected and processed several GOES-7 and GOES-8 image data sets that covered the BOREAS study region. The level-1 BOREAS GOES-8 images are raw data values collected by RSS-14 personnel at FSU and delivered to BORIS. The data cover 14-Jul-1995 to 21-Sep-1995 and 01-Jan-1996 to 03-Oct-1996. The data start out containing three 8-bit spectral bands and end up containing five 10-bit spectral bands. No major problems with the data have been identified. The data are contained in binary image format files. Companion files include (1) an image inventory listing to inform users of the images that are available and (2) example thumbnail images.

Tags: earth-science-atmospheric-radiation-atmosphere-reflectance, earth-science-atmospheric-water-vapor-atmosphere-water-vapor-indicators-water-vapor, earth-science-surface-radiative-properties-land-surface-reflectance
Organization: National Aeronautics and Space Administration
Gold Level L2 Solar EUV proxy

The GOLD solar irradiance proxy (QEUV) is a proxy for the integrated solar EUV \n   irradiance below 45 nm, which can be derived directly from far ultraviolet (FUV) radiance \n   measurements. QEUV is a dayside disk data product, derived from the GOLD DAY measurement mode.\n   \n   Algorithm heritage\n   The disk QEUV retrieval algorithm was originally developed for use with GUVI and SSUSI images \n   (Strickland et al., [1995]).  The GOLD implementation of this algorithm takes advantage of GOLD’s \n   ability to transmit the full spectrum to maximize the signal-to-noise ratio and eliminate atomic \n   emission lines that contaminate the N2 LBH bands (e.g., N I 149.3 nm). This algorithm has been \n   extensively documented and applied (e.g., Strickland et al. [2004]; Evans et al., [1995]). The \n   associated GOLD Level 2 data product is called QEUV.\n   \n   References\n   -Evans, J. S., D. J. Strickland and R. E. Huffman (1995), Satellite remote sensing of thermospheric \n    O/N2 and solar EUV: 2. Data analysis, J. Geophys. Res., Vol. 100, NO. A7, pages 12,227-12,233.\n      -Strickland, D. J., J. S. Evans, and L. J. Paxton (1995), Satellite remote sensing of thermospheric  \n    O/N2 and solar EUV: 1. Theory, J. Geophys. Res., 110, A7, pages 12,217-12,226.\n      -Strickland, D. J., J. L. Lean, R. R. Meier, A. B. Christensen, L. J. Paxton, D. Morrison, J. D. \n    Craven, R. L. Walterscheid, D. L. Judge, and D. R. McMullin, (2004), Solar EUV irradiance variability \n    derived from terrestrial far ultraviolet dayglow observations, Vol. 31, L03801, doi:10.1029/2003GL018415.\n

Tags: gold, imageintensity-solar-euv-proxy, ses-14
Organization: National Aeronautics and Space Administration
DAWN FC2 RAW (EDR) VESTA IMAGES V1.0

Abstract : Framing Camera 2 is one of two identical units flying on Dawn spacecraft. This dataset includes the Experiment Data Record (EDR) version of all available images acquired during the Vesta Encounter (Approach, Survey, transfer to HAMO, HAMO, transfer to LAMO, LAMO, transfer to HAMO2, HAMO-2, and departure). In addition to the imagery, anciliary information is stored within the image headers. Calibration files needed for further processing are archived as a separate data set.

Tags: __
Organization: National Aeronautics and Space Administration
BOREAS AFM-04 Twin Otter Aircraft Flux Data

The BOREAS AFM-04 team used the NRC Twin Otter aircraft in 1994 and 1996 to make measurements in the boundary layer of the fluxes of sensible and latent heat, momentum, ozone, methane, and carbon dioxide, plus supporting meteorological parameters such as temperature, humidity, and wind speed and direction. Aircraft position, heading, and altitude were also recorded, as were several radiometric observations for use in interpretation of the data (greenness index, surface temperature, incoming and reflected radiation). Data were collected at both the NSA and SSA during the three 1994 IFCs and in July and August of 1996.

Tags: earth-science-atmospheric-chemistry-atmosphere-carbon-and-hydrocarbon-compounds-atmospheric-car, earth-science-atmospheric-chemistry-atmosphere-oxygen-compounds-atmospheric-ozone, earth-science-atmospheric-pressure-atmosphere-atmospheric-pressure-measurements, earth-science-atmospheric-radiation-atmosphere-reflectance, earth-science-atmospheric-radiation-atmosphere-solar-irradiance, earth-science-atmospheric-temperature-atmosphere-surface-temperature-air-temperature, earth-science-atmospheric-winds-atmosphere-upper-level-winds, earth-science-surface-thermal-properties-land-surface-land-surface-temperature
Organization: National Aeronautics and Space Administration
Polar Visible Imaging System (VIS) Earth Camera Images, Calibrated (E0), 4 min 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 the Nighttime Auroral Oval at Visible Wavelengths. A Third Camera is used to monitor the Directions of the Fields-of-View of the Auroral Cameras with respect to the sunlit Earth and return Global Images of the Auroral Oval at Ultraviolet Wavelengths. The VIS Instrumentation produces an Auroral Image of 256 × 256 Pixels approximately every 24 s dependent on the Integration Time and Filter selected. The Fields-of-View of the two Nighttime Auroral Cameras are 5.6 × 6.3° and 2.8 × 3.3° for the Low and Medium Resolution Cameras, respectively. The Medium Resolution Camera was never activated. One or more Earth Camera Images of 256 × 256 Pixels are produced every 5 min, depending on the commanded Mode. The Field-of-View of the Earth Camera is approximately 20 × 20°. See: http://vis.physics.uiowa.edu/vis/vis_description/vis_description.htmlx Reference: Frank, L.A., J.B. Sigwarth, J.D. Craven, J.P. Cravens, J.S. Dolan, M.R. Dvorsky, J.D. Harvey, P.K. Hardebeck, and D. Muller, The Visible Imaging System (VIS) for the Polar Spacecraft, Space Science Review, Vol. 71, pp. 297-328, 1995. Data Set Description: The VIS Earth Camera Data Set comprises all Earth Camera Images for the selected Time Period. Full Coordinate Information is included for Viewer Orientation. In addition, a Rotation Matrix and a Table of Distortion-correcting Look Direction Unit Vectors are provided for the Purpose of calculating Coordinates for every Pixel. To facilitate viewing of the Images, a Mapping of Pixel Value to a recommended Color Table based on the Characteristics of the selected Filter will be included with each Image. A Relative Intensity Scale is provided through an Uncompressed Count Table. Approximate Intensity Levels in kiloRayleighs are given in an Intensity Table. For detailed Information on Intensities, see Sensitivities_and_Intensities.txt at https://cdaweb.gsfc.nasa.gov/Polar_VIS_docs/SENSITIVITIES_AND_INTENSITIES.TXT. Supporting Software is available at: http://vis.physics.uiowa.edu/vis/software/ Included is an IDL Program that displays the Images with the recommended Color Bar, provides approximate Intensities, Coordinate Data for each Pixel, and includes multiple Options for Image Manipulation.

Tags: imageintensity
Organization: National Aeronautics and Space Administration
Helios 2 Magnetic Field Spectral Density, offline at NSSDC

This data set contains 8-sec averaged and peak spectral densities of magnetic field component variations in 8 spectral bands with center frequencies logarithmically equispaced between 6.8 Hz and 1470 Hz.  Data records also contain time, spacecraft position, spacecraft-sun-Earth angle, spin vector direction, data quality flags, etc.

Tags: magneticfield, spectrum
Organization: National Aeronautics and Space Administration
BUV/Nimbus-4 Level 1 Radiance Data V001 (BUVN4L1RUT) at GES DISC

The Nimbus-4 BUV Level-1 Radiance data collection was derived from the Primary Data Base (PDB) product and contains the calibrated and geolocated backscattered ultraviolet radiances measured every 32 seconds at 12 wavelengths between 250 and 340 nm during the daylit orbit portion. The data collection also contains quality flags, dark current analyses of the data, orbital information, and housekeeping data. The data were originally created on IBM 360 machines and archived on magnetic tapes. The data have been restored from the tapes and are now archived on disk in their original IBM binary file format. Each file contains about one orbit of data. The data files consist of 100 4-byte word records which are blocked with up to 25 records. The first record is the header record, followed by a series of data records, and ended with two trailer records. A typical orbit file is about 70 kB in size. The BUV instrument was operational from April 10, 1970 until May 6, 1977. In July 1972 the Nimbus-4 solar power array partially failed such that BUV operations were curtailed. Thus data collected in the later years was increasingly sparse, particularly in the equatorial region. This product was previously available from the NSSDC with the identifier ESAC-00055 (old ID 70-025A-05B).

Tags: earth-science-ultraviolet-wavelengths-spectral-engineering-ultraviolet-radiance
Organization: National Aeronautics and Space Administration