AndreaBozzo/ceres-open-data-index huggingface dataset:
MESS MDIS MAP PROJ HIGH-INCIDENCE BASEMAP WEST RDR V1.0

Abstract : The Mercury Dual Imaging System (MDIS) consists of two cameras, a Wide Angle Camera (WAC) and a Narrow Angle Camera (NAC), mounted on a common pivot platform. This dataset includes Map Projected High- Incidence Angle Basemap Illuminated from the West RDRs (HIWs) which comprise a global map of I/F measured by the NAC or WAC filter 7 (both centered near 750 nm) during the the Extended Mission at high incidence angles to accentuate subtle topography, photometrically normalized to a solar incidence angle (i) : 30 degrees, emission angle (e) : 0 degrees, and phase angle (g) : 30 degrees at a spatial sampling of 256 pixels per degree. The HIW data set is a companion to the Map Projected High-Incidence Angle Basemap Illuminated from the East RDR (HIE) data set. Together the two data sets are intended to detect and allow the mapping of subtle topography. They complement a Basemap Data Record (BDR) data set also composed of WAC filter 7 and NAC images acquired at moderate/high solar incidence angles centered near 68 degrees (changed to 74 degrees in the find end-of-mission data delivery), and an Low Incidence Angle (LOI) data set also composed of WAC filter 7 and NAC images acquired at lower incidence centered near 45 degrees, analogous to the geometry used for color imaging. The map is divided into 54 'tiles', each representing the NW, NE, SW, or SE quadrant of one of the 13 non-polar or one of the 2 polar quadrangles or 'Mercury charts' already defined by the USGS. Each tile also contains 5 backplanes: observation ID; BDR metric, a metric used to determine the stacking order of component images, modified for the higher incidence angle centered near 78 degrees; solar incidence angle; emission angle; and phase angle.

Tags: __
Organization: National Aeronautics and Space Administration
STEREO-B SWAVES new one minute averages of the high (hfr) frequency receiver data.

The two STEREO radio receivers measure wave intensity, source direction and angular size in the frequency \n   range 40 kHz to 16 MHz, corresponding to heliocentric source distances of about 1 Rs to 1 AU. One 10-40 kHz \n   receiver measures radio and plasma waves near the 1 AU electron plasma frequency. One receiver makes high \n   time resolution measurements at 50 MHz. Time Domain Samplers make simultaneous wideband waveform measurements \n   on three electric components. Antenna systems include three mutually orthogonal 6-meter monopoles. \n

Tags: stereo-b, swaves, waves-high-frequency-receiver
Organization: National Aeronautics and Space Administration
STEREO-B PLASTIC Small Transients List

Small Transients (ST) are identified by the following criteria: 1. The STs have durations between 0.5 and 12 hours. 2. Magnetic field strength is higher than the yearly average (> 1.3 times yearly average). 3. Low proton beta (less than 0.7 times yearly average) or low proton temperature (Tp/Texp < 0.7). 4. Low Alfvén Mach Number (less than 0.7 yearly average), or large rotations of magnetic field components (we used the minimum variance analysis on the magnetic field, Sonnerup and Cahill Jr. [1967], Sonnerup and Scheible [1998]; and we require that the intermediate-to-minimum eigenvalue ratio be > 5). 5. Checking the Aflvénic fluctuations. We remove all three correlations (Rx, Ry, Rz) greater than 0.5, or two greater than 0.6 and the other greater than 0.3 from our list, which is similar to the criterion in Cartwright and Moldwin [2008].

Tags: thermalplasma
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 PRELANDING 0317 V1.0

This is a Rosetta Radio Science data set, collected during the PRELANDING phase 2014-01-21 to 2014-11-18. It is a Global Gravity measurement at the comet 67P and covers the time 2014-09-25T16:32:50.000 to 2014-09-26T00:25:10.000.

Tags: __
Organization: National Aeronautics and Space Administration
STEREO-B SWAVES One minute averages of the high (hfr) frequency receiver data.

The two STEREO radio receivers measure wave intensity, source direction and angular size in the frequency \n   range 40 kHz to 16 MHz, corresponding to heliocentric source distances of about 1 Rs to 1 AU. One 10-40 kHz \n   receiver measures radio and plasma waves near the 1 AU electron plasma frequency. One receiver makes high \n   time resolution measurements at 50 MHz. Time Domain Samplers make simultaneous wideband waveform measurements \n   on three electric components. Antenna systems include three mutually orthogonal 6-meter monopoles. \n

Tags: stereo-b, swaves, waves-high-frequency-receiver
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 2 0713 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 2015-04-17T12:28:15.000 to 2015-04-17T15:27:31.500.

Tags: __
Organization: National Aeronautics and Space Administration
Circum-Arctic Map of Permafrost and Ground-Ice Conditions, Version 2

The Circum-Arctic permafrost and ground ice map is available via ftp in ESRI Shapefile format and Equal-Area Scalable Earth Grid (EASE-Grid) format. See the Format section for an explanation of the files provided via FTP. The circumpolar permafrost and ground ice data contribute to a unified international data set that depicts the distribution and properties of permafrost and ground ice in the Northern Hemisphere (20°N to 90°N). The re-gridded data set shows discontinuous, sporadic, or isolated permafrost boundaries. Permafrost extent is estimated in percent area (90-100 percent, 50-90 percent, 10-50 percent, <10 percent, and no permafrost). Relative abundance of ground ice in the upper 20 m is estimated in percent volume (>20 percent, 10-20 percent, <10 percent, and 0 percent). The data set also contains the location of subsea and relict permafrost. the gridded data are gridded at 12.5 km, 25 km, and 0.5 degree resolution. The shapefiles were derived from the original 1:10,000,000 paper map (Brown et al. 1997) Permafrost, or permanently frozen ground, is ground (soil, sediment, or rock) that remains at or below 0°C for at least two years (Permafrost Subcommittee, 1988). It occurs both on land and beneath offshore arctic continental shelves, and underlies about 22 percent of the Earth's land surface. For more information on the creation of the original map, see Heginbottom et al. (1993). The original paper map also includes information on the relative abundance of ice wedges, massive ice bodies and Pingos, ranges of permafrost temperature and thickness (Brown et al. 1997).

Tags: earth-science-frozen-ground-cryosphere-ground-ice-ground-ice, earth-science-frozen-ground-cryosphere-permafrost-permafrost, earth-science-frozen-ground-land-surface-ground-ice-ground-ice, earth-science-frozen-ground-land-surface-permafrost-permafrost
Organization: National Aeronautics and Space Administration
AIM/CDE dust grain impact data

AIM/CDE (Cosmic Dust Experiment) data are available\nas Levels 1 and 2 daily netCDF files.  L1 data contains, for each dust \ngrain impact, a time tag, pulse height data, a number of electrons released \nby the impact, and engineering and housekeeping data.  L2 data adds the mass \nof the impacting particle and spacecraft location at time of impact.  \nFuture L3 and L4 products will add total mass impacting per orbit and \nimpact rates (L3) and mass correlation with CIPS total particle mass and \nPolar Mesospheric Cloud brightness.\n

Tags: dust
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 3 1039 V1.0

This is a Rosetta Radio Science data set, collected during the COMET ESCORT 3 phase 2015-07-01 to 2015-10-21. It is a Global Gravity measurement at the comet 67P and covers the time 2015-09-17T09:41:30.000 to 2015-09-17T15:39:26.500.

Tags: __
Organization: National Aeronautics and Space Administration
STEREO-B/SECCHI/EUVI FITS data

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 spacecraft are identical suites of remote sensing instruments designed to observe coronal mass ejections (CMEs) at the Sun and in transit outwards to 1 AU.\n\nEUVI measured emission lines at 30.4 nm (He II), 17.1 nm (Fe IX), 19.5 nm (Fe XII), and 21.1 nm (Fe XIV). The EUVI's 2048 x 2048 pixel detectors have a field of view out to 1.7 solar radii, and observe in four spectral channels that span the 0.1 to 20 MK temperature range. In addition to its view from two vantage points, the EUVI will provide a substantial improvement in image resolution and image cadence over its predecessor SOHO-EIT, while complying with the more restricted mass, power, and volume allocations on the STEREO mission.

Tags: imageintensity
Organization: National Aeronautics and Space Administration
STEREO-B PLASTIC Suprathermal Event List

This data product contains a list of automatically identified suprathermal proton events measured on the Wide Angle Partition without a Solid State Detector (WAP non-SSD) portion of the STEREO/PLASTIC instrument. This list in conjunction with the IMPACT magnetic field information and PLASTIC solar wind data can aid a user in identifying energetic proton events related to Stream Interaction Regions (SIRs), shocks, upstream events, magnetospheric events, etc.

Tags: thermalplasma
Organization: National Aeronautics and Space Administration
CLAMS-Chesapeake Lighthouse and Aircraft Measurements for Satellites Un. Washington Convair-580 aircraft measurements

Un. Washington Convair-580 Aerosol, radiation, chemical, and meteorological data products for the Chesapeake Lighthouse and Aircraft Measurements for Satellites (CLAMS) field campaign in ASCII format

Tags: earth-science-aerosols-atmosphere, earth-science-aerosols-atmosphere-aerosol-backscatter, earth-science-aerosols-atmosphere-aerosol-optical-depth-thickness, earth-science-atmospheric-radiation-atmosphere-solar-radiation, earth-science-clouds-atmosphere
Organization: National Aeronautics and Space Administration
THEMIS-A (P5), Electric Field Instrument (EFI) Spacecraft measured Electric Field

THEMIS-A: Electric Field Instrument, EFI, Electric Field Measurements. The L2 Product is a 3D Estimate of the perpnedicular Electric Field, Eperp, derived from the Spin Plane E-Field Measurements assuming E ⋅ B = 0, using relevant Flux-Gate Magnetometer, FGM, Data. This Data Product includes Spin-Averaged, and Fast Survey Field Data. The Spin-Averaged Data, EFS_DOT0, has approximately 3 s Time Resolution. Fast Survey, EFF_DOT0, Data has 0.125 s Time Resolution.

Tags: electricfield
Organization: National Aeronautics and Space Administration
MGS SAMPLER MAGNETOMETER/ELECTRON REFLECTOMETER DATA

MAG/ER data included on this volume consist of a suite of GIF files thatare plots of derived electron and magnetic field observations acquired during the assessment orbits [see: Acuna et al., 1998]. The plots include electron fluxes at 10, 50, 130, 300, and 1000 eV, a color spectrogram of the same data, and magnetic field amplitude and rms, and spacecraft altitude. The numerical data will be released later on MAG/ER archive volumes, after further validation and calibration procedures have been applied.

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Organization: National Aeronautics and Space Administration
AIM/SOFIE mixing ratios, extinction profiles, etc.

The daily netCDF files at GATS, Inc., hold level 2 SOFIE (Solar Occultation for Ice Experiment) data. These include primary absorber mixing ratios (CO2, CH4, NO,H2O, O3), 10 aerosol extinction profiles, uncertainity profiles for mixing ratios and extinctions, 83 km measurement lat./long., Temperatures, Pressures, Time, [0.150 km sampling, 150km to 3.0km, 30 profiles/day]. Vertical resolutions are 1km for gases and for polar mesospheric clouds, and .LT.3.5 km for temperatures and pressures.

Tags: profile
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P VIRTIS 2 ESCORT 3 MTP018 V2.0

This release contains the digital numbers (DN) contained in the telemetry (TM) packages of the VIRTIS instrument on board of the spacecraft Rosetta. This volume contains data at the vicinity of comet 67P, from the ESCORT 3 MTP018 phase, which occurred from 2015-07-01 to 2015-07-29. This version of the dataset (2.0) is produced by a fixed EGSE software. The old version of the software produced incomplete products, reduced by one line

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Organization: National Aeronautics and Space Administration
AeroCube-6B Dosimeter Data, 1 s and 0.1 s Data

Each AeroCube-6 vehicle carries three dosimeters measuring electrons with energies from about 43 keV to about 830 keV and protons with energies ranging from 370 keV to 12 MeV. The dataset manager, Dr. Paul O Brien, can be reached at paul.obrien@aero.org. The data are described in AeroCube-6 Dosimeter Data README (v3.0), Aerospace Report No. TOR-2016-01155, The Aerospace Corporation, March 4, 2016, El Segundo, CA. Also see AeroCube-6 Dosimeter Equivalent Energy Thresholds and Flux Conversion Factors, Aerospace Report No. TOR-2017-02598, The Aerospace Corporation, July 1, 2019, El Segundo, CA.

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
THEMIS-A Level 1 Probe State Data

The L1 STATE files contain the following data, sampled at one-minute intervals:\n\n               * probe position and velocity in GEI, GSE, and GSM coordinates;\n               * flags to indicate regions of interest and maneuver status;\n               * RA and declination of spin axis;\n               * spin period and spin phase;\n               * spin model parameters for high-precision interpolation of spin phase between one-minute data points.\n\n               Version number indicates data source as follows:\n\n               * V00: predicted ephemeris and attitude, no spin period or spin phase;\n               * V01: predicted ephemeris and attitude, spin period and spin phase derived from probe telemetry;\n               * V02: predicted attitude, definitive ephemeris from magnetometer and Doppler tracking data;\n               * V03: corrected attitude and spin phase derived from fully calibrated magnetometer data (added science attitude determination using perigee data post-processing).\n\n               Produced by Mission Ops, Science Ops and Science Team.

Tags: ephemeris
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 2 0792 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 2015-05-19T14:09:30.000 to 2015-05-19T15:16:14.500.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSINAC 4 EXT3-MTP032 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 ROSETTA EXTENSION 3 mission phase, covering the period from 2016-07-26T23:25:00.000 to 2016-08-09T23:24:59.000. 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 October 2018 PSA/PDS external peer review.

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Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 3 3410 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 2012-09-25T09:18:16.000 to 2012-09-25T12:56:49.500.

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Organization: National Aeronautics and Space Administration
ARTEMIS P1 field-plasma merged data, near moon

This data set contains 96s and 384s resolution magnetic field and plasma ion data from the THEMIS-B ESA and FGM instruments during the near moon (ARTEMIS) phase of the spacecraft life (>~September 1, 2010). The data are at each resolution for several mutually exclusive, contiguous hours during most days. The field-plasma-merged data set was created at GSFC/Space Physics Data Facility (SPDF) as part of the LunaSOX effort, from CDAWeb data sets THB_L2_ESA (good quality, high angular resolution mode only) and THB_L2_FGM. Geocentric spacecraft and moon orbit data from SSCWeb were used to add geocentric and selenocentric spacecraft position data to the merged data set records.

Tags: magneticfield, thermalplasma
Organization: National Aeronautics and Space Administration
THEMIS-B (P1/ARTEMIS-P1) Electron and Ion Moments (GMOM) Ground-Calculated Particle Energy Fluxes and Moments: Density, Velocity, Pressure and Temperature

THEMIS-B Electrostatic Analyzer (ESA) and Solid State Telescope (SST) Ground-Calculated Particle Energy Fluxes and Moments: Density, Velocity, Pressure, and Temperature. Generated from ESA and SST Combined Distributions. Data include Electron/Ion Ground-Calculated Fluxes and Spectrograms for Ions from 5 eV to 4 MeV and Electrons from 6 eV to 700 keV.

Tags: electricfield, energeticparticles, instrumentstatus, magneticfield, thermalplasma
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSIWAC 4 ESC3-MTP021 RDR-INF-REFL 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 reflectance units (normalized  and thus without unit),  acquired by the OSIRIS Wide Angle Camera on the Rosetta spacecraft  during the COMET ESCORT 3 mission phase, covering the period  from 2015-09-22T23:25:00.000 to 2015-10-20T23:24:59.000. 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.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 3 0875 V1.0

This is a Rosetta Radio Science data set, collected during the COMET ESCORT 3 phase 2015-07-01 to 2015-10-21. It is a Global Gravity measurement at the comet 67P and covers the time 2015-07-04T04:57:45.000 to 2015-07-04T05:41:36.500.

Tags: __
Organization: National Aeronautics and Space Administration
ACE Solar Wind Ion Composition Spectrometer (SWICS) Solar Wind Plasma Elemental Charge State Distributions with Statistical Uncertainties and Data Quality Flags, Level 2 (L2), 2 h Data

This ACE SWICS/SWIMS Data Set contains actual Charge State, Q, Distributions of Carbon, Oxygen, Neon, Magnesium, Silicon and Iron as opposed to the averaged Charge States that have been available on CDAWeb for some time. The Solar Wind Ion Composition Spectrometer (SWICS), prior to August 23, 2011 and denoted as SWICS Version 1.1, determines uniquely the Chemical and Ionic Charge State Composition of the Solar Wind, the Temperatures and Mean Speeds of major Solar Wind Ions at all Speeds above 300 km/s for Protons and 170 km/s for Fe+16, and resolves Protons and Helium Isotopes of Solar and Interstellar Sources. SWICS 1.1 measures the Distribution Functions of Interstellar Cloud Pick-Up Ions and Interplanetary Dust Cloud Pick-Up Ions up to Energies of 100 keV/e. The ACE SWICS 1.1 Data Products represent a new Release of the Data with significantly improved Time Series Measurements for the Elemental Abundance, Charge State Composition, and Kinetic Properties of Heavy Ions in the Solar Wind. It is a major new Update produced with completely redesigned Analysis Methods to account more rigorously for Instrumental and Statistical Effects (Shearer et al., 2014). Rare Elements are now identified more reliably and Estimates of Statistical Error are provided. Release Notes are available that describe the Data, the Methods used to determine the Data Values, and Issues concerning Data Quality and Measurement Uncertainty. The Quality of ACE Level 2 Data is such that it is suitable for serious Scientific Study. However, to avoid Confusion and Misunderstanding, it is recommended that Users consult with the appropriate ACE Team Members before publishing Work derived from the Data. The ACE Team has worked hard to ensure that the Level 2 Data are free from Errors, but the Team cannot accept Responsibility for Erroneous Data, or for Misunderstandings about how the Data may be used. This is especially true if the appropriate ACE Team Members are not consulted before Publication. At the very least, Preprints should be forwarded to the ACE Team before Publication. For more Information about the SWICS Instrument, visit the SWICS Home Page at http://solar-heliospheric.engin.umich.edu/ace.

Tags: energeticparticles, ioncomposition
Organization: National Aeronautics and Space Administration
STEREO WAVES (SWAVES) Radio Intensity Spectra, both Ahead and Behind s/c

The CDF file contains 1 minute averaged radio intensity data from both the Ahead and Behind s/c. A description of the STEREO/WAVES instrument is provided in: Bougeret, J.L, et al. (2008), S/WAVES: The Radio and Plasma Wave Investigation on the STEREO Mission, Space Science Reviews, 136, 487-528. The STEREO / WAVES (SWAVES) instruments provide unique and critical observations for all primary science objectives of the STEREO mission, the generation of CMEs, their evolution, and their interaction with Earth's magnetosphere. SWAVES can probe a CME from lift-off to Earth by detecting the coronal and interplanetary (IP) shock of the most powerful CMEs, providing a radial profile through spectral imaging, determining the radial velocity from ~2 RS (from center of sun) to Earth, measuring the density of the volume of the heliosphere between the sun and Earth, and measuring important in situ properties of the IP shock, magnetic cloud, and density compression in the fast solar wind stream that follows. SWAVES measures the fluctuation electric field present on three orthogonal monopole antennas mounted on the back (anti-sunward) surface of the spacecraft. Each monopole antenna unit is a 6 m long Beryllium-Copper (BeCu) "stacer" spring. The three units deploy from a common baseplate that also accommodates the preamplifier housing. The 6 m length was chosen to put the antenna quarter-wave resonance near the top of the SWAVES HFR2 frequency band. These data consist of output from the SWAVES HFR and LFR receivers. - the High Frequency Receivers (HFR) - for spectral analysis and direction finding of radio noise generated from a few solar radii (16 MHz) to about half an Astronomical Unit (125 kHz) - the Low Frequency Receiver (LFR) - for spectral analysis and direction finding from about half an Astronomical Unit (160 kHz) to one AU (2.5 kHz).

Tags: jovian-decametric-radiation, jupiter-dam, solar-radio-burst, spectrogram, spectrum-dynamic-spectrogram, type-ii-solar-radio-burst, type-iii-solar-radio-burst, waves-passive
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSINAC 5 ESC4-MTP024 DDR-GEO V1.0

This CODMAC level 5 data set contains derived data products that include pixel-precise georeferencing information, acquired by the OSIRIS Narrow Angle Camera on the Rosetta spacecraft during the COMET ESCORT 4 mission phase, covering the period from 2015-12-15T23:25:00.000 to 2016-01-12T23:24:59.000. 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
ROSETTA-ORBITER X SREM 5 STEINS V1.0

This data set contains derived electron and proton flux energies in MeV from the Standard Radiation Environment Monitor (SREM) instrument on the Rosetta spacecraft. These are CODMAC Level 5 derived data, and measure the radiation in the spacecraft environment during the AST1 (STEINS) mission phase.

Tags: __
Organization: National Aeronautics and Space Administration