AndreaBozzo/ceres-open-data-index huggingface dataset:
Ulysses Cosmic Ray and Solar Particle Investigation (COSPIN) High Energy Telescope (HET) Full Resolution Proton and Electron Counts and Accumulation Times for Spin-Averaged Counting Rates, OMNI1 H1-H9, 12 s Data

A Directory containing Daily FTP downloadable Files containing Readout-by-Readout Listings of the Counts accumulated in the H1-H9 Spin-Averaged Counting Rates. These Counting Rates respond primarily to Protons (H1-H5, H9) in the approximate Energy Ranges 5.4-14, 14-19, 24-31, 34-68, 68-92, and >92 MeV, respectively, and to Electrons (H6-8) in the very approximate Energy Ranges 1-3, 5-10, and 3-5 MeV, respectively. The Naming Convention for the Daily Files is uly_het_full_rat_omni1_YYYDDD.txt, where YYY indicates the three digit Year since 1900 (e.g. YYY=090 for 1990, and YYY=102 for 2002) and DDD indicates the three digit Day of Year (January 1 = 1). In each File, following a detailed Description of the Format, the Data consist of a Listing of Counts accumulated in the H1-H9 Spin-Averaged Counting Rates during the Intervals between successive Readouts, organized into Columns as described below. The first four Columns give the Start Time of the Counting Rate Accumulation Period as Fractional Year (to 12 Decimal Places) and as Year since 1900, Day of Year, and Milliseconds of Day at the Start of the Accumulation, followed by one Column giving the Duration of the Accumulation Period in Milliseconds (it is the same for all nine Rates), and nine Columns giving the Counts accumulated in that Period for each Rate. All Fields except for the Fractional Year are in Integer Format. Each Line contains Data for one single Readout of the Rates H1-H9, and all Readouts where at least one of the Rates has a Non-fill Value are included. Where Fill does occur it is indicated by -1. Since the Accumulation Period for each Readout is forced to include an Integral Number of Spacecraft Spins in order to produce pure Spin-Averaged Measurements, the Lengths of the Accumulation Periods vary in a Cyclic Manner as the Period of the Telemetry Cycle beats with the Spacecraft Spin Period. All Counting Rates in this File are read out twice per Spacecraft Format. At the most common Science Telemetry Bit Rate (2048 bps) this corresponds to an Average Interval between Readouts of 16 s. Thus, with a typical 5 rpm Spacecraft Spin Rate the Accumulation Intervals vary in a repeating Cycle of 12, 12, 24, 12, 12, 24, 12, etc., seconds. At lower Bit Rates the Average Interval is equal to 16 times (2048/BR) seconds and the Cycle automatically adjusts to produce this Average Accumulation. No Noise Removal or Despiking has been done, so Caution must be used in interpreting isolated large Increases or Decreases in the Counting Rates.

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
Pioneer 10 Charged Particle Composition (CPC) 15-min Count Rates

This data set contains coincidence mode counts and \naccumulation times, plus "box counts" based on pulse height analysis (PHA), \nat 15-min resolution. There are 11 coincidence mode counts and 27 "box \ncounts."  Taken together, the parameters included allow computation of \naverage counting rates and of fluxes of protons, electrons, helium and \nCNO nuclei in selected energy windows corresponding to the PHA boxes.\nThere are 12 proton boxes spanning 3-67 MeV, 5 helium boxes spanning\n3-67 MeV/n, 5 electron boxes, 2 Z>2 boxes, 1 box each for CNO, Z>5, and \nE>67 MeV/n.

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
Ulysses Heliosphere Instrument for Spectral, Composition, and Anisotropy at Low Energies (HISCALE) CA60-Z Count Rates, Daily Averages

Daily-averaged sectored count rates from CA60 - Channels Z2, Z2A, Z3, and Z4. The HISCALE instrument contains the Low-Energy Magnetic Spectrometers (LEMS), the Low-Energy Foil Spectrometers (LEFS) and the Composition Aperture (CA). There is a LEMS detector at 30 degrees from the spacecraft spin axis and a second at 120 degrees. LEFS is positioned at 60 degrees from the spacecraft spin axis with a second LEFS detector at 150 degrees. The CA detector is positioned at 60 degrees from the spacecraft spin axis. The parameter descriptions of this document reference the detectors by their acronyms and angle from the spacecraft spin axis, i.e. LEMS30, LEMS120, LEFS60, LEFS150, and CA60.

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSINAC 4 ESC2-MTP014 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 COMET ESCORT 2 mission phase, covering the period  from 2015-03-10T23:25:00.000 to 2015-04-08T11:24:59.000. 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
Ulysses Heliosphere Instrument for Spectral, Composition, and Anisotropy at Low Energies (HISCALE) CA60-W Count Rates, 5 min Averages

5min-averaged sectored count rates from CA60 - Channels W1, W2, W3, W4, W5, W6, W7, and W8. The HISCALE instrument contains the Low-Energy Magnetic Spectrometers (LEMS), the Low-Energy Foil Spectrometers (LEFS) and the Composition Aperture (CA). There is a LEMS detector at 30 degrees from the spacecraft spin axis and a second at 120 degrees. LEFS is positioned at 60 degrees from the spacecraft spin axis with a second LEFS detector at 150 degrees. The CA detector is positioned at 60 degrees from the spacecraft spin axis. The parameter descriptions of this document reference the detectors by their acronyms and angle from the spacecraft spin axis, i.e. LEMS30, LEMS120, LEFS60, LEFS150, and CA60.

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
Pioneer 10 Charged Particle Composition (CPC)  1-Hour Count Rates

Hourly count rates from U. Chicago Charged Particle Composition\nInvestigation (CPC) carried on Pioneer 10.  There are four rates each, for protons \nand alpha particles, at 11-20, 20-24, 24-29, 29-67 MeV/n.  There are four additional \ncount rates, corresponding to 7-17 MeV electrons, Z>=1 ions with E>67 MeV/n, Z>5 ions\nwith E>67 MeV/n, and 2 x minimizing ionizing particles. The data are ftp-accessible \nin annual ASCII files and via FTPBrowser.  The hourly averages were computed \nfrom 15-min data (counts, accumulation times, PHA-based box counts, etc.) that are\nalso available via ftp from nssdcftp.gsfc.nasa.gov.

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
Ulysses HISCALE LEFS150 ion and electron counts

This data set contains 1-hour spin averaged count rates of the ion and electron from the Ulysses Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies (HI-SCALE) Low Energy Foil Spectrometer at 150 degrees to the spacecraft spin axis. Count rate units are /s.  For references, see Astron. Astrophys. Suppl. Ser., 92(2), 349-363, 1992.

Tags: energeticparticles, ioncomposition
Organization: National Aeronautics and Space Administration
Ulysses HISCALE LEMSDE deflected electron counts

This data set contains 1-hour spin averaged count rates of the deflected electron from the Ulysses Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies (HI-SCALE) Low Energy Foil Spectrometer at 30 degrees to the spacecraft spin axis. Count rate units are /s.  For references, see Astron. Astrophys. Suppl. Ser., 92(2), 349-363, 1992.

Tags: energeticparticles, ioncomposition
Organization: National Aeronautics and Space Administration
Pioneer 10 Cosmic-Ray Telescope (CRT) 6-hr fluxes and rates

This data set has eight 6-hour fluxes (3.45-5.15, 30.55-56.47 and 120.7-227.3 MeV protons, 3.44-4.97, 10.03-21.7, 30.67-56.7 and 112.7-413 MeV/n alpha particles, and 2-6 MeV electrons), 28 count rates, and Poisson uncertainties in the fluxes and rates, as determined from the Cosmic Ray Telescope (CRT) on the Pioneer 10 spacecraft.  Data are in annual files with consistent end-of-record marks.  Spacecraft position data are not given in the data records but are accessible from Helioweb at http://cohoweb.gsfc.nasa.gov/helios/heli.html

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
MARS EXPRESS SUN MRS 1/2/3 EXTENDED MISSION 3 2755 V1.0

This is a Mars Express Radio Science data set, collected during the extended mission phase 2010-01-01 to 2012-12-31. It is a Solar Conjunction measurement and covers the time 2011-02-03T09:00:39 to 2011-02-03T10:59:56.500.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER CHECKOUT OSINAC 4 RVM1 RDR-REFLECT V1.0

This CODMAC level 4 data set contains radiometric calibrated and geometric distortion corrected (resampled)  image data in reflectance units (normalized and thus without unit),  acquired by the OSIRIS Narrow Angle Camera on the Rosetta spacecraft  during the RENDEZVOUS MANOEUVRE 1 mission phase, covering the period  from 2010-09-04T00:00:00.000 to 2011-07-13T23:59:59.000. The prime objective was commissioning / calibration. Several targets of opportunity were observed, but none of them is identifiable as prime target. This version V1.0 is the first version of this dataset.

Tags: __
Organization: National Aeronautics and Space Administration
CDDIS MEaSUREs SESES products weekly displacement grids time series

Making Earth System Data Records for Use in Research Environments (MEaSUREs) empowers the research community to participate in developing and generating data products that complement and augment NASA produced and distributed Earth science data products. NASA’s Enhanced Solid Earth Science Earth Science Data Record (ESDR) System (ESESES) continues and extends mature geodetic data product generation and archival as part of the MEaSUREs SESES project providing new, multi-decade, calibrated and validated geodetic-derived ESDRs obtained by the Scripps Institution of Oceanography (SIO) and NASA's Jet Propulsion Laboratory (JPL). These data-derived products include continuous multi-year high-rate GNSS, seismogeodetic, and meteorological time series, a catalog of transient deformation in tectonically active areas known for aseismic motion such as ETS with focus in Cascadia, and continuous estimation and cataloging of total near-surface water content derived from continuous GNSS time series over the continental U.S.

Tags: earth-science-geodetics-solid-earth-techniques-gnss-global-navigation-satellite-systems, earth-science-tectonics-solid-earth-earthquakes
Organization: National Aeronautics and Space Administration
Pioneer 10 Geiger Tube Telescope (GTT) 1-Hour Count Rates

Hourly count rates from U. Iowa Geiger Tube Telescope (GTT)\ncarried on Pioneer 10.  There are five rates: electrons > 0.06 MeV plus protons\n> 25 MeV; e > 5 MeV plus p > 30 MeV; e >0.55 MeV plus p > 6.6 MeV; e > 21 MeV\nplus p > 80 MeV; e > 31 MeV plus p > 80 MeV.  The data are ftp-accessible in\nannual ASCII files and via FTPBrowser.  The hourly averages were computed at\nNSSDC from 15-min data still offline (as of Feb. 2009).

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
Ulysses HISCALE LEMS30 ion and electron counts

This data set contains 1-hour spin averaged count rates of the ion and electron from the Ulysses Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies (HI-SCALE) Low Energy Foil Spectrometer at 30 degrees to the spacecraft spin axis. Count rate units are /s.  For references, see Astron. Astrophys. Suppl. Ser., 92(2), 349-363, 1992.

Tags: energeticparticles, ioncomposition
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 4 1231 V1.0

This is a Rosetta Radio Science data set, collected during the COMET ESCORT 4 phase 2015-10-22 to 2015-12-31. It is a Global Gravity measurement at the comet 67P and covers the time 2015-12-03T02:37:05.000 to 2015-12-03T04:06:28.500.

Tags: __
Organization: National Aeronautics and Space Administration
CDDIS MEaSUREs SESES products Change in Water Storage Time Series

Making Earth System Data Records for Use in Research Environments (MEaSUREs) empowers the research community to participate in developing and generating data products that complement and augment NASA produced and distributed Earth science data products. NASA’s Enhanced Solid Earth Science Earth Science Data Record (ESDR) System (ESESES) continues and extends mature geodetic data product generation and archival as part of the MEaSUREs SESES project providing new, multi-decade, calibrated and validated geodetic-derived ESDRs obtained by the Scripps Institution of Oceanography (SIO) and NASA's Jet Propulsion Laboratory (JPL). These data-derived products include continuous multi-year high-rate GNSS, seismogeodetic, and meteorological time series, a catalog of transient deformation in tectonically active areas known for aseismic motion such as ETS with focus in Cascadia, and continuous estimation and cataloging of total near-surface water content derived from continuous GNSS time series over the continental U.S. These data products are grids of changes in total water storage over the continental U.S.; continuous estimation and cataloging of total near-surface water content derived from continuous GNSS time series over the continental U.S.

Tags: earth-science-atmospheric-water-vapor-atmosphere, earth-science-geodetics-solid-earth-techniques-gnss-global-navigation-satellite-systems
Organization: National Aeronautics and Space Administration
Ulysses HISCALE 1-hour ion counts

This data set contains 1-hour spin averaged count rates of the ion data from the Ulysses Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies (HI-SCALE) Composition Aperture Telescope at 60 degrees to the spacecraft spin axis. Count rate units are /s.  For references, see Astron. Astrophys. Suppl. Ser., 92(2), 349-363, 1992.

Tags: energeticparticles, ioncomposition
Organization: National Aeronautics and Space Administration
LRO MOON CRATER EDR RAWDATA VERSION 1.0

This data set comprises the raw binary data from                             from the LRO Cosmic Ray Telescope for the                             Effects of Radiation (CRaTER) instrument. The                             data consists of the unconverted primary                             science, secondary science, and housekeeping                             CCSDS-formatted data packets and data headers.

Tags: __
Organization: National Aeronautics and Space Administration
Pioneer 10 Hourly Plasma Version 3.1 Data

This data set contains Version 3.1 final archival set of hourly averaged solar wind data from the Plasma Analyzer of the Pioneer 10 mission. It includes plasma bulk parameters in ASCII format: bulk velocity, proton number density, proton temperature, and flow angles. This is the same data set as NSSDC ID SPHE-00066 or 72-012A-13L, which is in binary format.

Tags: thermalplasma
Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 3 3428 V1.0

This is a Mars Express Radio Science data set, collected during the extended mission phase 2010-01-01 to 2012-12-31. It is a Global Gravity measurement and covers the time 2012-12-10T02:44:36.000 to 2012-12-10T05:32:27.500.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 2 0780 V1.0

This is a Rosetta Radio Science data set, collected during the COMET ESCORT 2 phase 2015-03-11 to 2015-06-30. It is a Global Gravity measurement at the comet 67P and covers the time 2015-05-16T07:16:10.000 to 2015-05-16T09:12:33.000.

Tags: __
Organization: National Aeronautics and Space Administration
Pioneer 10 Trapped Radiation Detector (TRD) 1-Hour Count Rates

Hourly count rates from UCSD Trapped Radiation Detector \n(TRD) carried on Pioneer 10.  Included are four rates, C1 and C3 from the \nCerenkov counter and M1L and M3L from the Minimum Ionizing Particle Counter.  \nC1 corresponds to >480 MeV/n ions (typically 80% protons and 20% Z>1 nuclei).  \nC3 corresponds to >650 MeV/n ions (typically 30% protons and 70% Z>1 nuclei).  \nM1L corresponds to >80 MeV/n ions (typically 90% protons and 10% Z>1 nuclei). \nM3L corresponds to 80-300 MeV protons (50%) and >80 MeV/n Z>1 nuclei (50%).  \nThe data are ftp-accessible in annual ASCII files and via FTPBrowser.  \nThe hourly averages were computed at NSSDC from 30-min data still offline \n(as of Feb. 2009).

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
Pioneer 11 Cosmic-Ray Telescope (CRT) 6-hr fluxes and rates

This data set has eight 6-hour fluxes (3.45-5.15, 30.55-56.47 and 120.7-227.3 MeV protons, 3.44-4.97, 10.03-21.7, 30.67-56.7 and 112.7-413 MeV/n alpha particles, and 2-6 MeV electrons), 28 count rates, and Poisson uncertainties in the fluxes and rates, as determined from the Cosmic Ray Telescope (CRT) on the Pioneer 11 spacecraft.  Data are in annual files with consistent end-of-record marks.  Spacecraft position data are not given in the data records but are accessible from Helioweb at http://cohoweb.gsfc.nasa.gov/helios/heli.html

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
ROSETTA NAVIGATION CAMERA  ENGINEERING DATA

This CODMAC level 3 data set contains the key parameters of the two  Navigation Cameras.   In particular, it provides information on operating modes of the  prime and backup cameras. The NAVCAM images are provided in a different  science dataset to the HK.   The Navigation cameras were used continuously during the comet phase  but on an irregular basis during the cruise e.g. asteroid flyby.  Similarly they were turned on much later than other instruments and  subsystems on board after launch.   It covers the period from launch in 2004, through the 3 Earth and  1 Mars flyby, plus the hibernation phases, plus the asteroid flybys  and finally covers the Prelanding, comet escort & Extension phases  of the prime target of the mission.   The prime target is comet 67P/Churyumov-Gerasimenko 1 (1969 R1).   This version V1.0 is the first version of this dataset.

Tags: __
Organization: National Aeronautics and Space Administration
Ulysses Heliosphere Instrument for Spectral, Composition, and Anisotropy at Low Energies (HISCALE) MFSA, Spacecraft Frame, Spin-Averaged Z>1 Ion Fluxes, Hourly Averages

Hourly-averaged ion fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the spacecraft rest frame.

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
MARS EXPRESS SUN MRS 1/2/3 EXTENDED MISSION 7 4057 V1.0

This is a Mars Express Radio Science data set, collected during the extended mission phase 2019-01-01 to 2020-12-31. It is a Solar Conjunction measurement and covers the time 2019-09-13T23:52:12.000 to 2019-09-14T03:43:10.500.

Tags: __
Organization: National Aeronautics and Space Administration
Phobos 2 Ephemeris, Heliocentric Trajectories, Heliographic, Heliographic Inertial, and Solar Ecliptic Coordinates, HelioWeb, Daily Data

Heliocentric trajectories for Phobos 2 in Heliographic, HG, Heliographic Inertial, HGI, and Solar Ecliptic, SE, Coordinates\n\nThe original trajectory data are taken from http://ssd.jpl.nasa.gov/horizons.cgi where users can find many more objects. In the case of orbit data for planets, the orbit data can be used as a proxy for spacecraft ephemeris that are in orbit about the planets. On a heliospheric scale, differences between the planet orbital tarjectory and that of the spacecraft are very small. For instance, the heliocentric longitudes differ by only 0.25° for a spacecraft stationed near the L1 Lagrange point at approximately 100 Earth radii upstream of the Earth.\n\nThe production of the HG, HGI, and SE trajectory data requires a values for the "Equinox Epoch", which is defined as the epoch time when the direction from the Earth to the sun at the time of the vernal equinox when the sun seems to cross equatorial plane of the Earth from below. This direction is called the First Point of Aries, FPA and it is not a fixed direction but drifts by about 1.4° per century or 50.26" per year. In addition, there are tiny irregularities in FPA drift that are on the order of 1" per year or less. The Equinox Epoch can be determined by using a variety of methods for calculating the instantaneous FPA longitudinal direction and whether the tiny irregularities have been smoothed or averaged out. Four methods for determining the Equinox Epoch are in common usage:\n\n+---------------------------------------------------------------------+\n| Method Name  | FPA Longitude Definition                             |\n|---------------------------------------------------------------------|\n| B1950.0      | the actual FPA at 22:09 UT on December 31, 1949      |\n| J2000.0      | the smoothed FPA at 12:00 UT on January 1, 2000      |\n| True of Date | the actual FPA at 00:00 UT on the date of interest   |\n| Mean of Date | the smoothed FPA at 00:00 UT on the date of interest |\n+---------------------------------------------------------------------+\n\nThe heliocentric trajectory data included in this data product have been calculated by using the Equinox Epoch: defined via the "Mean of Date" method.\n\nMore precise coordinates, and some planet-centered coordinates, are found in the "traj" subdirectories of spacecraft specific directories at https://spdf.gsfc.nasa.gov/pub/data/ and http://ssd.jpl.nasa.gov/horizons.cgi.

Tags: ephemeris
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 1 0554 V1.0

This is a Rosetta Radio Science data set, collected during the COMET ESCORT 1 phase 2014-11-20 to 2015-03-10. It is a Global Gravity measurement at the comet 67P and covers the time 2015-01-29T12:51:10.000 to 2015-01-29T22:52:12.000.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 1 0511 V1.0

This is a Rosetta Radio Science data set, collected during the COMET ESCORT 1 phase 2014-11-20 to 2015-03-10. It is a Global Gravity measurement at the comet 67P and covers the time 2014-12-28T01:42:05.000 to 2014-12-28T12:10:12.000.

Tags: __
Organization: National Aeronautics and Space Administration