AndreaBozzo/ceres-open-data-index huggingface dataset:
NEW HORIZONS SPICE KERNELS V1.0

This data set includes the complete set of New Horizons (NH) SPICE      data files (``kernel files''), which can be accessed using SPICE      software. The SPICE data contain geometric and other ancillary      information needed to recover the full value of the science      instrument data. In particular SPICE kernels provide spacecraft      and planetary ephemerides, instrument mounting alignments,      spacecraft orientation, and data needed for relevant time      conversions.

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Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 7 4013 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 Occultation measurement and covers the time 2019-05-24T18:50:00.000 to 2019-05-24T20:45:00.000.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P VIRTIS 2 ESCORT 1 MTP012 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 1 MTP012 phase, which occurred from 2015-01-14 to 2015-02-11. 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
Wind Weimer Propagated 60 s Resolution Tri-axial Fluxgate Magnetometer in GSE Coordinates

Wind Weimer propagated solar wind data and linearly interpolated to have the measurements on the minute at 60 s resolution tri-axial fluxgate magnetometer data in GSE coordinates. This data set consists of propagated solar wind data that has first been propagated to a position just outside of the nominal bow shock (about 17, 0, 0 Re) and then linearly interpolated to 1 min resolution using the interp1.m function in MATLAB. The input data for this data set is a 1 min resolution processed solar wind data constructed by Dr. J.M. Weygand. The method of propagation is similar to the minimum variance technique and is outlined in Dan Weimer et al. [2003; 2004]. The basic method is to find the minimum variance direction of the magnetic field in the plane orthogonal to the mean magnetic field direction. This minimum variance direction is then dotted with the difference between final position vector minus the original position vector and the quantity is divided by the minimum variance dotted with the solar wind velocity vector, which gives the propagation time. This method does not work well for shocks and minimum variance directions with tilts greater than 70 degrees of the sun-earth line. This data set was originally constructed by Dr. J.M. Weygand for Prof. R.L. McPherron, who was the principle investigator of two National Science Foundation studies: GEM Grant ATM 02-1798 and a Space Weather Grant ATM 02-08501. These data were primarily used in superposed epoch studies. References: Weimer, D. R. (2004), Correction to ‘‘Predicting interplanetary magnetic field (IMF) propagation delay times using the minimum variance technique,’’ J. Geophys. Res., 109, A12104, doi:10.1029/2004JA010691. Weimer, D.R., D.M. Ober, N.C. Maynard, M.R. Collier, D.J. McComas, N.F. Ness, C. W. Smith, and J. Watermann (2003), Predicting interplanetary magnetic field (IMF) propagation delay times using the minimum variance technique, J. Geophys. Res., 108, 1026, doi:10.1029/2002JA009405. There are now two version of this data set. An off set has been found in the Wind MFI Bz component that is present after November 2004. Version 2 has this offset removed. Prof. R.L. McPherron determined the correction to be Bz = Bz - (-0.000000130406219.*odoy.*odoy + 0.000576303146.*odoy + 0.679940509 + 0.3215*cos(2*pi*(doy-171)/366)) where doy is the day of the year in units of days and odoy is the days sinces Jan 1, 1999 00:00:00 UT in units of days.

Tags: bow-shock, magnetic-fields, magneticfield-1-min, magnetometer, magnetopause, magnetotail, propagated-solar-wind-data, solar-wind, wind
Organization: National Aeronautics and Space Administration
MARS EXPRESS SUN MRS 1/2/3 EXTENDED MISSION 7 4033 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 2019-08-16T23:30:00.000 to 2019-08-17T05:15:00.000.

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Organization: National Aeronautics and Space Administration
Wind Magnetic Field Investigation (MFI) Data at full resolution

This data product contains Wind MFI full resolution magnetic field magnitude and GSE and GSM Cartesian components. Time resolution is typically 0.046s or 0.092s from launch through 1997, and is 0.092s thereafter. Final Version 5 data are accessible to within about 3 months of current date, newly defined Version 4 data (with final Bz offsets and not-yet-final spacecraft position vectors) between 3 months and about 2 weeks of current date, and newly defined Version 3 data (with the most recently determined Bz offset value, not yet final for the Version 3 interval) from 2 weeks to about 2 days of current.

Tags: magneticfield
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 1 0550 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 2015-01-26T11:29:25.000 to 2015-01-26T20:29:11.000.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 PRELANDING 0432 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 2014-11-14T14:38:25.000 to 2014-11-15T02:38:24.000.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 4 1284 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 2015-12-25T17:31:45.000 to 2015-12-25T19:00:15.000.

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Organization: National Aeronautics and Space Administration
Wind Magnetic Field Investigation (MFI) Composite Data

Wind MFI composite data in GSE and GSM coordinates. The files contain multiple time resolution data: 3-second, 1-minute, and 1-hour. Final Version 5 data are accessible to within about 3 months of current date, newly defined Version 4 data (with final Bz offsets and not-yet-final spacecraft position vectors) between 3 months and about 2 weeks of current date, and newly defined Version 3 data (with the most recently determined Bz offset value, not yet final for the Version 3 interval) from 2 weeks to about 2 days of current.

Tags: magneticfield
Organization: National Aeronautics and Space Administration
OPTICAL CONSTANTS AND LAB SPECTRA OF WATER ICE V1.1

Transmission spectra of amorphous and crystalline H2O-ice at temperatures from 20-150 K for a wavelength range from 1.11 to 2.63 microns. These spectra have not been continuum-corrected or had the infrared interference fringes removed. Optical constants (n and k values) were derived from these laboratory spectra and are included in the data set.

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Organization: National Aeronautics and Space Administration
Wind Suprathermal Ion Composition Spectrometer (STICS) Distribution Functions

Wind Suprathermal Ion Composition Spectrometer (STICS) phase-space distribution functions at 1-day time resolution for specified ions. Calibrated science quality data presented in the native spacecraft frame. The data files contain 3D phase space density distribution, A(v) (currently in arbitrary units) functions, for H+. There are 512 values for A(v) for each time step, corresponding to each directional sector (16 total directions) and each Deflection Voltage Step (DVS) corresponding to a set E/q value (32 total voltage steps per sector). Only proton distribution functions are currently released at the production level.

Tags: ioncomposition
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 4 1182 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 2015-11-15T02:25:40.000 to 2015-11-15T07:16:26.000.

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Organization: National Aeronautics and Space Administration
Wind Solar Wind Experiment (SWE) Faraday Cup, Solar Wind Plasma Reduced Ion Distribution Functions, 92 s Data

WIND Solar Wind Experiment, SWE, Faraday cup data: this data set contains three-dimensional measurements of ions in the energy range 150 eV to 8 keV. Placed 15° above and below equatorial plane of the spacecraft, the Faraday Cups measure ion charge flux as a function of epoch, cup number, orientation angle, and bias grid potential. For each time point, a full spectrum is comprised of charge flux measurements at the two Faraday cup sensors at 20 azimuth angles for each of 31 energy-per-charge windows with 1240 data points per spectrum. Spectra are built up over approximately 92 s intervals. The effective area of the Faraday cup sensor as a function of incidence angle onto the cup is also provided.

Tags: electricfield, energeticparticles, instrumentstatus
Organization: National Aeronautics and Space Administration
Wind Solar Wind Experiment (SWE) 92-sec Definitive Solar Wind Proton Data

SWE is a comprehensive plasma instrument for the WIND spacecraft, see K.W.Ogilvie, et al., Space Sci. Rev., 71, 55-77, 1995. This product provides solar wind proton parameters, including anisotropic temperatures, derived by non-linear fitting of the measurements and with moment techniques. Data reported within this product do not exceed the limits of various parameters listed in the following section. There may be more valid data in the original dataset that requires additional work to interpret but were discarded due to the limits. In particular we have tried to exclude non-solar wind data from these files. We provide the one sigma uncertainty for each parameter produced by the non-linear curve fitting analysis either directly from the fitting or by propagating uncertainties for bulk speeds, flow angles or any other derived parameter. For the non-linear anisotropic proton analysis, a scalar thermal speed is produced by determining parallel and perpendicular temperatures, taking the trace, Tscalar = (2Tperp + Tpara)/3 and converting the result back to a thermal speed. The uncertainties are also propagated through.

Tags: thermalplasma
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RPCLAP 3EXT2 CALIB2 V1.0

This data set containsCALIBRATED data from Rosetta RPC-LAP, acquired during the ROSETTAEXTENSION 2 mission phase where the primary target was the comet67P/CHURYUMOV-GERASIMENKO 1 (1969 R1). It contains instrument outputs involts and amperes, calibrated and corrected for instrument offsets.

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Organization: National Aeronautics and Space Administration
JUNO JUPITER MWR ATMOSPHERIC BRIGHTNESS TEMPERATURE V1.0

The Juno MWR ATMOSPHERIC BRIGHTNESS TEMPERATURE dataset in this      volume is a nonaccumulating dataset derived from high-rate perijove      data. The atmospheric brightness temperature (and their angular      dependence) is provided as a function of planetocentric latitude.      The data is store is several product files separated by MWR channel      and perijove.

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Organization: National Aeronautics and Space Administration
Wind Energetic Particle Acceleration, Composition and Transport (EPACT)/LEMT 5-min Omnidirectional Fluxes

This dataset contains 5-min omnidirectional fluxes for He, C, O, Ne, Si, and Fe in particles/cm2-sr-s-MeV/nuc in seven energy bins (six for Ne) in the general range of 2-10 MeV/nucleon. The error bars are statistical only, that is, corresponding to sqrt(N), where N is the number of collected ions. For intervals in which zero ions were observed, the error bar corresponds to one ion. ASCII listing generated from this link provide the start-time of the averaging interval as YYYY DD HH, followed by pairs of numbers giving the flux and its uncertainty from the selected intervals. The available energy bins for the species are:\n\n+----------------------------------------------------------------------------------------------+\n| Species |  Band 1   |  Band 2   |  Band 3   |  Band 4   |  Band 5   |  Band 6   |  Band 7    |\n|----------------------------------------------------------------------------------------------|\n| He      | 2.00-2.40 | 2.40-3.00 | 3.00-3.70 | 3.70-4.53 | 4.53-6.00 | 6.00-7.40 | 7.40-9.64  |\n| C       | 2.57-3.19 | 3.19-3.85 | 3.85-4.80 | 4.80-5.80 | 5.80-7.20 | 7.20-9.10 | 9.10-13.70 |\n| O       | 2.56-3.17 | 3.17-3.88 | 3.88-4.68 | 4.68-6.00 | 6.00-7.40 | 7.40-9.20 | 9.20-13.40 |\n| Ne      | 3.27-3.98 | 3.98-4.72 | 4.72-5.92 | 5.92-7.87 | 7.87-9.96 | 9.96-12.7 |            |\n| Si      | 2.50-3.20 | 3.20-4.00 | 4.00-4.90 | 4.90-6.00 | 6.00-7.90 | 7.90-9.70 | 9.70-13.60 |\n| Fe      | 2.40-3.00 | 3.00-3.95 | 3.95-4.80 | 4.80-5.90 | 5.90-7.80 | 7.80-9.30 | 9.30-12.50 |\n+----------------------------------------------------------------------------------------------+

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
CLEM1 LUNAR GRAVITY V1.0

The gravitational signature of the Moon was determined from velocity perturbations of the Clementine spacecraft as measured from the Doppler shift of the S-band radio tracking signal. Clementine was tracked by NASA's Deep Space Network (DSN) at Goldstone, California, Canberra, Australia, Madrid, Spain, as well as by the Pomonkey, Maryland, tracking station operated by the Naval Research Laboratory. The tracking data were used to determine the Clementine orbit about the Moon, as well as the lunar gravity field [ZUBERETAL1994]. A detailed description of how the Clementine orbits were computed and an assessment of their quality can be found in [LEMOINEETAL1995B].

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Organization: National Aeronautics and Space Administration
HAYABUSA AMICA V1.0

The Asteroid Multi-band Imaging Camera (AMICA) of the Hayabusa mission to the asteroid 25143 Itokawa obtained 1662 images from May 11, 2003, shortly after launch, until November 19, 2005, after Itokawa encounter. This data set includes all images from the mission, plus pre-flight flat field images.

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Organization: National Aeronautics and Space Administration
VENUS CLIMATE ORBITER IR2 CALIBRATED DATA V1.0

The VCO IR2 CDR data set contains products acquired by the IR2 instrument onboard the Venus Climate Orbiter (VCO, also known as PLANET-C and AKATSUKI) spacecraft. The data files are provided in FITS format with an HDU as IMAGE extension, and it also contains metadata to the header of the HDU.

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Organization: National Aeronautics and Space Administration
Wind SMS Suite, SupraThermal Ion Composition Spectrometer (SMS/STICS) Alpha Particle Distribution Function and Differential Flux, Magnetosphere, Level 2 (L2), PT3M Data

The Suprathermal Ion Composition Spectrometer (STICS) is a Time of Flight (TOF) Plasma Mass Spectrometer, capable of identifying Mass and Mass per Charge for incident Ions up to 200 keV/q. It uses an Electrostatic Analyzer to admit Ions of a particular Energy per Charge (E/Q) into the TOF Chamber. The E/Q Voltage is stepped through 32 Values, sitting at each Value for approximately 24 s, to measure Ions over the full E/Q Range of 6 keV/q to 200 keV/q. Ions then pass through a Carbon Foil and TOF Chamber, before finally impacting on a Solid-State Detector (SSD) for Energy Measurement. STICS combines these three Measurements of E/Q, TOF and Residual Energy, producing PHA Words. This Triple-Coincidence Technique greatly improves the Signal to Noise Ratio in the Data. Measurements of E/Q and TOF without Residual Energy also produce PHA Words. These Double-Coincidence Measurements are characterized by better Statistics since Ions whose Energy does not allow them to be registered by the SSD can still be counted in Double-Coincidence Measurements. However, Ion Identification in Double-Coincidence Measurements are limited to a select Number of Ions that are well separated in E/Q - TOF Space. The STICS Instrument provides full 3D Velocity Distribution Functions, through a Combination of multiple Telescopes and Spacecraft Spin. The Instrument includes three separate TOF Telescopes that view three separate Latitude Sectors, as shown in Figure 1. In addition, the WIND Spacecraft Spins, allowing the three Telescopes to trace out a nearly 4π sr Viewing Area. The Longitudinal Sectors are shown in Figure 2. The Solar Direction is in Sectors 8-10 while the Earthward Direction is in Sectors 0-2.

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER COMET ESCORT OSINAC 2 EDR MTP 012 V1.0

This data set contains raw EDR images acquired by the OSIRIS Narrow AngleCamera during the escort phase of the Rosetta mission at the comet 67P,covering the period from 2015-01-13 to 2015-02-10.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER CHECK MIDAS 3 CR4A PC8 V3.0

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 set includes all data from theCRUISE 4-1 mission phase.This release supersedes version 1.0. Version 2.0 was never generatedfor pre-comet phases.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 2 0705 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 2015-04-12T08:28:35.000 to 2015-04-12T13:19:09.000.

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Organization: National Aeronautics and Space Administration
Wind SMS Suite, SupraThermal Ion Composition Spectrometer (SMS/STICS) Proton Distribution Function and Differential Flux, Magnetosphere, Level 2 (L2), PT3M Data

The Suprathermal Ion Composition Spectrometer (STICS) is a Time of Flight (TOF) Plasma Mass Spectrometer, capable of identifying Mass and Mass per Charge for incident Ions up to 200 keV/q. It uses an Electrostatic Analyzer to admit Ions of a particular Energy per Charge (E/Q) into the TOF Chamber. The E/Q Voltage is stepped through 32 Values, sitting at each Value for approximately 24 s, to measure Ions over the full E/Q Range of 6 keV/q to 200 keV/q. Ions then pass through a Carbon Foil and TOF Chamber, before finally impacting on a Solid-State Detector (SSD) for Energy Measurement. STICS combines these three Measurements of E/Q, TOF and Residual Energy, producing PHA Words. This Triple-Coincidence Technique greatly improves the Signal to Noise Ratio in the Data. Measurements of E/Q and TOF without Residual Energy also produce PHA Words. These Double-Coincidence Measurements are characterized by better Statistics since Ions whose Energy does not allow them to be registered by the SSD can still be counted in Double-Coincidence Measurements. However, Ion Identification in Double-Coincidence Measurements are limited to a select Number of Ions that are well separated in E/Q - TOF Space. The STICS Instrument provides full 3D Velocity Distribution Functions, through a Combination of multiple Telescopes and Spacecraft Spin. The Instrument includes three separate TOF Telescopes that view three separate Latitude Sectors, as shown in Figure 1. In addition, the WIND Spacecraft Spins, allowing the three Telescopes to trace out a nearly 4π sr Viewing Area. The Longitudinal Sectors are shown in Figure 2. The Solar Direction is in Sectors 8-10 while the Earthward Direction is in Sectors 0-2.

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
MER 1 MARS ALPHA PARTICLE X-RAY SPECTROMETER 2 XRAYSPEC V1.0

This archive contains Mars Exploration Rover x-ray data products fromthe APXS instrument and ancillary files. Each product has a detachedPDS label that describes the file structure and instrument parametersused for that product. The APXS x-ray products archived on this volume were generated by the APXS Science Team, Max Planck Institute, for the Mars Exploration Rover Project. Supporting documentation and label files conform to the Planetary Data System (PDS) Standards, Version 3.6, Jet PropulsionLaboratory (JPL) document number D-7669. This archive is designed tobe accessed as an online resource.

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Organization: National Aeronautics and Space Administration
PHOENIX MARS MET LIDAR ATMOSPHERIC PROFILES EDR V1.0

The PHX Atmospheric Lidar Profiles product contains unprocessed laser scattering atmospheric profiles for photon counting data at 532nm, and analog data at both 532 and 1064nm wavelengths (expressed in Dignal Numbers). The range data is provided as a time series of profiles between 5 and 90 min in total duration, with each profile representing an accumulation or average over 1.28-20.24 sec. Supplemental data of estimated laser power and inter-profile analog background skylight estimates are also provided.

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Organization: National Aeronautics and Space Administration
Wind Energetic Particle Acceleration, Composition and Transport (EPACT)/LEMT 1-Hr Omnidirectional Fluxes

This dataset contains hourly-averaged omnidirectional fluxes for He, C, O, Ne, Si, and Fe in particles/cm2-sr-s-MeV/nuc in seven energy bins (six for Ne) in the general range of 2-10 MeV/nucleon. The error bars are statistical only, that is, corresponding to sqrt(N), where N is the number of collected ions. For intervals in which zero ions were observed, the error bar corresponds to one ion. ASCII listing generated from this link provide the start-time of the averaging interval as YYYY DD HH, followed by pairs of numbers giving the flux and its uncertainty from the selected intervals. The available energy ranges for bins bby species are:\n\n+----------------------------------------------------------------------------------------------+\n| Species |  Band 1   |  Band 2   |  Band 3   |  Band 4   |  Band 5   |  Band 6   |  Band 7    |\n|----------------------------------------------------------------------------------------------|\n| He      | 2.00-2.40 | 2.40-3.00 | 3.00-3.70 | 3.70-4.53 | 4.53-6.00 | 6.00-7.40 | 7.40-9.64  |\n| C       | 2.57-3.19 | 3.19-3.85 | 3.85-4.80 | 4.80-5.80 | 5.80-7.20 | 7.20-9.10 | 9.10-13.70 |\n| O       | 2.56-3.17 | 3.17-3.88 | 3.88-4.68 | 4.68-6.00 | 6.00-7.40 | 7.40-9.20 | 9.20-13.40 |\n| Ne      | 3.27-3.98 | 3.98-4.72 | 4.72-5.92 | 5.92-7.87 | 7.87-9.96 | 9.96-12.7 |            |\n| Si      | 2.50-3.20 | 3.20-4.00 | 4.00-4.90 | 4.90-6.00 | 6.00-7.90 | 7.90-9.70 | 9.70-13.60 |\n| Fe      | 2.40-3.00 | 3.00-3.95 | 3.95-4.80 | 4.80-5.90 | 5.90-7.80 | 7.80-9.30 | 9.30-12.50 |\n+----------------------------------------------------------------------------------------------+

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P VIRTIS 2 ESCORT 2 MTP015 V1.0

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 2 MTP015 phase, which occurred from 2015-04-08 to 2015-05-06

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Organization: National Aeronautics and Space Administration