AndreaBozzo/ceres-open-data-index huggingface dataset:
MARS EXPRESS SUN MRS 1/2/3                                     EXTENDED MISSION 8 4389 V1.0

This is a Mars Express                                     Radio Science data set, collected                                     during the extended mission phase                                     2023-01-01 to 2023-12-31.                                     It is a Solar Conjunction                                     measurement and covers the time                                     2023-12-12T08:33:17.000 to                                     2023-12-12T09:45:05.000.

Tags: __
Organization: National Aeronautics and Space Administration
LANL 1994 Geosynchronous Orbit Particle Analyzer (SOPA) at 60 sec Resolution in Spacecraft Coordinates

The LANL 1994-084 SOPA data set contains various parameters in a variety of coordinates systems including GEI, spacecraft, polar geographic, and polar magnetic coordinates at about 60 s resolution. These parameters include universal time, spacecraft location, electron and on density, electron and on temperature, electron and ion particle flux, electron and ion energies, electron and ion rangies, and data quality flags.

Tags: energeticparticles-60-sec, geosynchronous, lanl, sopa, synchronous-orbit-particle-analyzer
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSINAC 4 EXT1-MTP027 RDR V1.0

This CODMAC level 4 data set contains radiometric calibrated and geometric distortion corrected (resampled) image data in W/m^2/sr/nm acquired by the OSIRIS Narrow Angle Camera during the ROSETTA EXTENSION 1 phase of the Rosetta mission, covering the period from 2016-03-08T23:25:00.000 to 2016-04-05T23:24:59.000.

Tags: __
Organization: National Aeronautics and Space Administration
EPOXI INFLIGHT LUNAR CALS - HRII CALIBRATED SPECTRA V1.0

This dataset contains calibrated, 1.05- to 4.8-micron spectral images of the Moon acquired the High Resolution Infrared Spectrometer (HRII) from 29 December 2007 through 18 December 2009 during several in-flight instrument calibrations for the EPOXI mission.

Tags: __
Organization: National Aeronautics and Space Administration
LANL 1997 Geosynchronous Orbit Particle Analyzer (SOPA) at 60 sec Resolution in Spacecraft Coordinates

The LANL 1997-97A SOPA data set contains various parameters in a variety of coordinates systems including GEI, spacecraft, polar geographic, and polar magnetic coordinates at about 60 s resolution. These parameters include universal time, spacecraft location, electron and on density, electron and on temperature, electron and ion particle flux, electron and ion energies, electron and ion rangies, and data quality flags.

Tags: energeticparticles-60-sec, geosynchronous, geosynchronous-orbit-particle-analyzer, lanl, sopa
Organization: National Aeronautics and Space Administration
LISIRD supplied Composite Lyman Alpha

This data product contains daily irradiance levels \n(photons/s/cm**2) of solar Lyman alpha (121.5 nm) radiation from multiple \nspacecraft and modelling sources, including AE-E/ESUM, SME/SUVM, \nUARS/SOLSTICE, TIMED/SEE and SORCE/SOLSTICE spacecraft and F10.7 and Mg \nmodels.  Data are available from 1947 to near-current, both graphically \nand, in txt/csv format, digitally, from the LISIRD interface at \nU.Colorado/LASP.

Tags: irradiance
Organization: National Aeronautics and Space Administration
MAVEN SEP Calibrated Ion and Electron Spectra Data Collection (Sensor 2)

Calibrated MAVEN Solar Energetic Particle (SEP) Instrument Sensor 2 ion and electron spectra. The data include total (integrated) and differential (as a function of 28 energy windows) ion and electron number fluxes in forward and reverse look directions. Description of the SEP instrument can be found on the SEP home page https://lasp.colorado.edu/maven/science/instrument-package/sep/ and in the SEP instrument publication https://doi.org/10.1007/s11214-015-0218-z.

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
MARS EXPRESS ASPERA-3 RAW EDR ION MASS ANALYZER EXT1 V1.0

This data set contains Mars Express ASPERA-3 Ion Mass         Analyzer (IMA) data for the first mission extention         (January 1, 2006 - September 30, 2007).  These data are         provided in raw units of counts/accumulation.

Tags: __
Organization: National Aeronautics and Space Administration
MARS EXPRESS SUN MRS 1/2/3                                     EXTENDED MISSION 8 4354 V1.0

This is a Mars Express                                     Radio Science data set, collected                                     during the extended mission phase                                     2023-01-01 to 2023-12-31.                                     It is a Solar Conjunction                                     measurement and covers the time                                     2023-10-29T00:25:02.200 to                                     2023-10-29T04:07:40.000.

Tags: __
Organization: National Aeronautics and Space Administration
MAVEN STATIC Event Rate Selected Channel Data Collection

MAVEN Supra-Thermal And Thermal Ion Composition (STATIC) Particle Distributions. This collection contains files with time-ordered event rate data from a selected rate channel. Data are derived from APID da. Description of the STATIC instrument can be found on the STATIC home page https://lasp.colorado.edu/maven/science/instrument-package/static/ and in the STATIC instrument publication https://doi.org/10.1007/s11214-015-0175-6.

Tags: energeticparticles, ioncomposition, thermalplasma
Organization: National Aeronautics and Space Administration
IBEX-Lo TOF Histograms

Each table (CSV file) captures the numbers \nof counts of arriving energetic neutral atoms, as integrated \nover a full 8-day orbit, for a single IBEX-Lo energy step, \nfor one of three categories of species (hydrogen, oxygen plus\ncarbon, and hydrogen plus oxygen plus carbon, the latter \ntwo being labelled "Oxygen" and "All," respectively in file\nnames).  Numbers of counts are given in 1024 0.33-nanosecond \nTOF bins ranging from 0-0.33 ns to 339.67-340 ns.  Each table \nis CSV-formatted Excel.  Each subdirectory is for a given \nenergy band and has the tables (files) for each of several \norbits for each of the three species categories.

Tags: neutralatomimages
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 3 0884 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 2015-07-09T14:50:00.000 to 2015-07-09T17:44:02.000.

Tags: __
Organization: National Aeronautics and Space Administration
LANL Daily-averaged electron fluxes from the Synchronous Orbit Particle Spectrometer (SOPA)

Daily-averaged electron fluxes from the Los Alamos\n    National Laboratory (LANL) Synchronous Orbit Particle Spectrometer\n    (SOPA) Daily averages from each geosynchronous satellite available\n    on any given day were merged into a single, uniform daily average.\n    Data span 22 September, 1989 through 31 December, 2009. Data are\n    log(flux) with flux in units of electrons /(cm^2.s.sr.keV). The\n    original SOPA data channels have been fit to a bi-Maxwelian spectra.\n    Fluxes are evaluated at virtual "channels" for fixed energies (i.e.\n    not for an energy passband or integral thresholds) [see 2010JA015735\n    _LANL_Data_and_Processing for details] (2010ja015735-readme.txt)

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
MAVEN SWEA Survey Rate 3D Electron Distributions Data Collection

MAVEN Solar Wind Electron Analyzer (SWEA) electron energy/angle (3D) distributions in units of differential energy flux (eV/cm^2 sec ster eV) at the MAVEN survey telemetry rate. Description of the SWEA instrument can be found on the SWEA home page https://lasp.colorado.edu/maven/science/instrument-package/swea/ and in the SWEA instrument publication https://doi.org/10.1007/s11214-015-0232-1.

Tags: thermalplasma
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RPCMIP 3 ESC1 V1.0

This archive contains data from the RPC-MIP instrument onboard ROSETTA Orbiter, acquired during the comet escort part 1 phase at the vicinity of comet 67P/CG. It also contains documentation which describes the 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
MAVEN SWIA Calibrated Coarse Archive 3D Data Collection

MAVEN Solar Wind Ion Analyzer (SWIA) coarse archive 3d files with time-ordered fully calibrated ion distributions in units of differential energy flux derived from the SWIA Coarse distribution Archive telemetry, as well as a header of ancillary information needed to interpret the data. Description of the SWIA instrument can be found on the SWIA home page https://lasp.colorado.edu/maven/science/instrument-package/swia/ and in the SWIA instrument publication https://doi.org/10.1007/s11214-013-0029-z.

Tags: thermalplasma
Organization: National Aeronautics and Space Administration
MAVEN SWEA Survey Rate Electron Pitch Angle Distributions Data Collection

MAVEN Solar Wind Electron Analyzer (SWEA) electron pitch angle distributions in units of differential energy flux (eV/cm^2 sec ster eV) at the MAVEN survey telemetry rate. Description of the SWEA instrument can be found on the SWEA home page https://lasp.colorado.edu/maven/science/instrument-package/swea/ and in the SWEA instrument publication https://doi.org/10.1007/s11214-015-0232-1.

Tags: thermalplasma
Organization: National Aeronautics and Space Administration
MAVEN SWIA Calibrated Onboard Survey Moment Data Collection

SWIA onboard moment files with time-ordered ion moments converted to physical units and coordinates, as computed onboard from Coarse and Fine ion distributions, as well as a header with ancillary information needed to interpret the moments. Description of the SWIA instrument can be found on the SWIA home page https://lasp.colorado.edu/maven/science/instrument-package/swia/ and in the SWIA instrument publication https://doi.org/10.1007/s11214-013-0029-z.

Tags: thermalplasma
Organization: National Aeronautics and Space Administration
MMS 1 Energetic Particle Detector, Energetic Ion Spectrometer (EPD-EIS) Energy by Time of Flight, Level 2 (L2), Burst Mode, 0.605 s Data

Energetic Particle Detector (EPD), Energetic Ion Spectrometer (EIS) Energy by Time of Flight, Level 2, Burst Survey, 0.605 s Data. The EIS provides ion composition measurements (protons versus oxygen ions) and angular distributions over the energy range from approximately 45 to 500 keV.

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
MARS EXPRESS SUN MRS 1/2/3                                     EXTENDED MISSION 8 4400 V1.0

This is a Mars Express                                     Radio Science data set, collected                                     during the extended mission phase                                     2023-01-01 to 2023-12-31.                                     It is a Solar Conjunction                                     measurement and covers the time                                     2023-12-20T03:25:42.000 to                                     2023-12-20T07:46:56.000.

Tags: __
Organization: National Aeronautics and Space Administration
MMS 1 Energetic Particle Detector, Energetic Ion Spectrometer (EPD-EIS) Pulse Height by Time of Flight, Level 2 (L2), Burst Mode, 0.605 s Data

Energetic Particle Detector (EPD), Energetic Ion Spectrometer (EIS) Pulse Height by Time of Flight, Level 2, Burst Survey, 0.605 s Data. The EIS provides ion composition measurements (protons versus oxygen ions) and angular distributions over the energy range from approximately 45 to 500 keV.

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MARSIS EXPERIMENT DATA RECORD EXT 5 V1.0

This dataset contains the                    scientific telemetry produced by the MARSIS                    instrument after editing for duplicated and                    corrupted packets, together with geometric                    information computed on ground to locate                    observations in space and time. Both subsurface                    and ionosphere sounding data are included in                    the dataset.

Tags: __
Organization: National Aeronautics and Space Administration
LANL 2001 Magnetospheric Plasma Analyzer (MPA) at 87 sec Resolution in Spacecraft Coordinates

The LANL 01A MPA data set contains numerical moments computed from measurements of the Los Alamos Magnetospheric Plasma Analyzer (MPA) [Bame et al., Rev. Sci. Inst., in press 1993]. The moments are presented in s/c coordinates: the z-axis is aligned with the spin axis, which points radially toward the center of the Earth; the x-axis is in the plane containing the spacecraft spin axis and the spin axis of the Earth, with +X generally northward; and the y-axis points generally eastward. Polar angles are measured relative to the spin axis (+Z), and azimuthal angles are measured around the z-axis, with zero along the +X direction. The moments are computed for three 'species': lop (low-ener. ions, ~1eV/e-~130eV/e); hip (hi-ener. ions, ~130eV/e-~45keV/e); alle (electrons, ~30eV - ~45keV ). The electron measurements are obtained 21.5 secs after the ion measurements. Epoch is the measurement time appropriate for the ions. The moments are computed after the fluxes are corrected for background and s/c potential. Algorithms for these corrections are relatively unsophisticated, so the moments are suspect during times of high background and/or high spacecraft potential. Because the determined spacecraft potential is not very precise, the magnitude of the low-energy ion flow velocity is probably not accurate, but the flow direction is well determined. Tperp and Tpara are obtained from diagonalization of the 3-dimensional temperature matrix, with the parallel direction assigned to the eigenvalue which is most different from the other two. The corresponding eigenvector is the symmetry axis of the distribution and should be equivalent to the magnetic field direction. The eigenvalue ratio Tperp/Tmid, which is provided for each species, is a measure of the symmetry of the distribution and should be ~1.0 for a good determination. Several of the parameters have a fairly high daily dynamic range and for survey purposes are best displayed logarithmically. These parameters are indicated by non-zero 'SCALEMIN' values in this file. A quality flag value of 1 indicates that the values are suspect because of unreliable location info.

Tags: energeticparticles-87-sec, geosynchronous, lanl, magnetospheric-plasma-analyzer, mpa
Organization: National Aeronautics and Space Administration
IBEX-Lo Release-3 Counts for flow longitude analysis

This product contains counts accumulated in \neach of 30 6-deg spin phase bins over some variable time span\nindicated in each record.  The time spans are selected to support\nanalysis of the flow longitude of the interstellar medium (ISM).\nThe data are specifically as used in the analyses reported in\nBzowski et al (2012) and Mobius et al (2012).  A companion product\nhas the counting data used in the ISM flow latitude analyses of\nthe same papers.  Data are organized into orbit-specific arrays\nwherein the columns contain the counts for a given time span\nwithin the orbit and the rows contain the counts for a given one\nof the 30 spin-phase angles for the multiple time spans of the orbit.\nArrays are available for orbits 12-19, 60, 61, and 63-67.  The number\nof time spans used in an orbit varies from 5 to 45. \n

Tags: neutralatomimages
Organization: National Aeronautics and Space Administration
VG2 NEP LECP RESAMPLED SUMMARY SCAN                                      AVERAGED 24SEC V1.0

This data consists of resampled data from the Low EnergyCharged Particle (LECP) Experiment on the Voyager 2 Spacecraftfor the period when Voyager 2 was in the vicinity of the planetNeptune.  The period covered is 1989-08-24T00:00:00.000 SCET  to1989-08-27T00:00:00.000 SCET.  This data approximates a time seriesof charged particle fluxes from a selection of channels availablefrom the instrument.  The word approximates is used becausethe angle scanning modes of the instrument complicates thenature of the data.  At times the instrument mechanically scans,and at times it is fixed to look at a specific direction.With the type of data given here, the fluxes are angle averagedfor those time periods when the instrument is scanning, and aretime averaged over an arbitrary period (12 or 24 sec, see below)for the periods when the detectors are stationary.

Tags: __
Organization: National Aeronautics and Space Administration
MARS EXPRESS SUN MRS 1/2/3                                     EXTENDED MISSION 8 4390 V1.0

This is a Mars Express                                     Radio Science data set, collected                                     during the extended mission phase                                     2023-01-01 to 2023-12-31.                                     It is a Solar Conjunction                                     measurement and covers the time                                     2023-12-14T04:13:14.000 to                                     2023-12-14T08:22:56.000.

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

Heliocentric trajectories for Juno in Heliographic, HG, Heliographic Inertial, HGI, and Solar Ecliptic, SE, Coordinates The 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. The 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: +---------------------------------------------------------------------+   Method Name   FPA Longitude Definition    ---------------------------------------------------------------------    B1950.0   the actual FPA at 22:09 UT on December 31, 1949     J2000.0   the smoothed FPA at 12:00 UT on January 1, 2000     True of Date   the actual FPA at 00:00 UT on the date of interest     Mean of Date   the smoothed FPA at 00:00 UT on the date of interest   +---------------------------------------------------------------------+ The heliocentric trajectory data included in this data product have been calculated by using the Equinox Epoch: defined via the "Mean of Date" method. More 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
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 7 4166 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 2020-12-13T15:22:58.100 to 2020-12-13T15:45:06.750.

Tags: __
Organization: National Aeronautics and Space Administration
MMS 1 Active Spacecraft Potential Control (ASPOC), Sensors 1 and 2, Level 2 (L2), Survey Mode, 1 s Data

MMS 1 Active Spacecraft Potential Control (ASPOC) - Sensors 1 and 2 Ion Beam Current Rates, Beam Energies, and Instrument Status variables. In tenuous plasma regions, the floating potential of a sunlit spacecraft is positively charged, reaching up to tens of Volts. The corresponding electric field disturbs the ambient plasma measurements obtained from electron and ion sensors and the large fluxes of attracted photo-electrons can significantly reduce the lifetime of the micro-channel plate. The electric field measurements can be also contaminated by the high spacecraft potential values. The Active Spacecraft Potential Control neutralizes the spacecraft potential by releasing positively charged Indium ions. The ASPOCs neutralize the electrical potential of the spacecraft, limiting or eliminating spurious electric fields that can contaminate measurements. This allows observations of the more scientifically important low-energy ions and electrons.

Tags: instrumentstatus
Organization: National Aeronautics and Space Administration
DAWN FC1 RAW (EDR) CERES IMAGES V1.0

Abstract  :  This dataset contains raw Framing Camera 1 (FC1) images sometimes  called level-1a or EDR data. It includes images from the Dawn Ceres  eXtended Mission 1 Orbit 3 (XMO3, aka Ceres Extended GRaND - CXG) phase  on 2017-02-19 and the Ceres eXtended Mission Orbit 4 (XMO4, aka Ceres  Extended Opposition - CXO) phase on 2017-04-29. In addition, there are  images from eXtended Mission 2 (XM2), orbits XMO6 (C2I - intermediate),  and XMO7 (C2E - elliptical) as well as some checkout and end-of-mission  star calibration images.FC1 is one of two identical units flying  on the Dawn spacecraft. It was designated as the backup system to be  used only in the event of a failure of the primary system, FC2. Prior to the Ceres extended mission, FC1 had only been used for in-flight  calibration and to periodically exercise its various mechanisms (door,  filter wheel, etc.). This is the only science dataset generated by FC1.

Tags: __
Organization: National Aeronautics and Space Administration
MMS 1 Electric Particle Detector, Fly's Eye Energetic Particle Sensor (EPD, FEEPS) Electrons, Level 2 (L2), Burst Mode, 0.3025 s Data

Fly's Eye Electron Proton Spectrometer (FEEPS) Burst Data. The Energetic Particle Detector (EPD) investigation aboard the four MMS spacecraft consists of two instrument designs, the FEEPS and the EIS (Energetic Ion Spectrometer). A FEEPS consists of six Heads, each composed of two Eyes. Each eye is a particle telescope with a single silicon detector. There are nine electron eyes and three ion eyes per FEEPS. The energy coverage is from 25 keV to 650 keV for electrons and 45 keV to 650 keV for ions. Each eye has sixteen energy channels, the spacing of which can be modified by command. The fields of view and pointing of each eye are designed to provide a broad, instantaneous field of view for the twelve eyes per FEEPS.

Tags: energeticparticles, magneticfield
Organization: National Aeronautics and Space Administration
ICON The Far Ultra Violet Imaging Spectrograph Day Limb Images

The FUV instrument takes 2D images of the Earth’s horizon in the Far ultraviolet. \n   The imager is pointing approximately 90 degrees to the spacecraft motion, similar to looking out \n   of the side window of a car as it drives down the road. Onboard electronics read the CCD detectors 8 times per\n   second and collect the data into radiance profiles every 12 seconds. The calibrated level 1 radiances\n   and Level 1 ancillary spacecraft data are combined in a limb retrieval to produce the level 2.4 O/N2 limb product.

Tags: imageintensity
Organization: National Aeronautics and Space Administration