AndreaBozzo/ceres-open-data-index huggingface dataset:
LRO MOON LAMP 2 EXPERIMENT DATA RECORD V1.0

The Lunar Reconnaissance Orbiter (LRO) Lyman Alpha Mapping Project (LAMP) CODMAC Level 2 Experiment Data Record is a collection of the far ultraviolet photon detections obtained by the LAMP instrument, in raw form. As such, it constitutes the permanent record of the raw LAMP data. These data include both the instrument science and housekeeping data, organized into extensions within files formatted according to the Flexible Image Transport System (FITS) standard, version 2.1b. The LAMP EDR archive enables reprocessing of the raw science data as radiometric and geometric calibration processing routines improve. Investigators interested in applying advanced calibration methods or needing to understand the properties of the raw data will find the EDR products useful. Most investigators, however, will be interested in using either the LAMP data products contained in the CODMAC Level 3 Reduced Data Record, as radiometric and geometric calibration processing has already been done for these products, or the LAMP CODMAC Level 5 far ultraviolet map products.

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Organization: National Aeronautics and Space Administration
THEMIS-B (P1/ARTEMIS-P1), Electric Field Instrument (EFI) Spacecraft measured Electric Field

THEMIS-B: 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
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 1 0501 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 2014-12-23T00:21:45.000 to 2014-12-23T12:16:10.500.

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Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3                                     EXTENDED MISSION 9 4431 V1.0

This is a Mars Express                                     Radio Science data set, collected                                     during the extended mission phase                                     2023-01-01 to 2026-12-31.                                     It is a Occultation                                     measurement and covers the time                                     2024-03-16T07:31:33.000 to                                     2024-03-16T07:53:41.000.

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Organization: National Aeronautics and Space Administration
STEREO-B Ephemeris, Heliocentric Trajectories, Heliographic, Heliographic Inertial, and Solar Ecliptic Coordinates, HelioWeb, Daily Data

Heliocentric trajectories for STEREO-B 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
CASSINI JUPITER CIRS TIME-SEQUENTIAL DATA RECORDS V2.0

This data set comprises uncalibratedand calibrated data from the Cassini Composite Infrared Spectrometer(CIRS) instrument. The basic data is comprised of uncalibrated raw spectra,along with along with pointing and geometry information, andhousekeeping information. Also included are calibrated power spectra, and documentation.

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Organization: National Aeronautics and Space Administration
STARDUST NAVCAM RAW PREFLIGHT CALIBRATION IMAGES V2.0

This dataset contains the raw, preflight, thermal-vacuum calibration images collected by the Navigation Camera (NAVCAM) on 8-10 April 1998 for the Stardust mission. This is version 2.0 of the dataset, in which the original image data were converted from the standard PDS IMG format to the FITS format; no corrections were applied. The NExT mission to comet 9P/Tempel 1 used some of these preflight data to check the exposure time offsets due to shutter reversal and to determine dark current rates. This dataset supersedes version 1.0 which was safed by PDS because the data were not considered to be scientifically useful for the Stardust mission, due to problems encountered during the flight (stuck filter wheel, contamination on the instrument window, etc.) that changed the instrument characteristics.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RPCLAP 2 ESC2 MTP016 V1.0

This dataset contains EDITED data from Rosetta RPC-LAP, acquired during MTP16 of the COMET ESCORT 2 mission phase. The Rosetta s/c was on its journey to comet 67P/CG.

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Organization: National Aeronautics and Space Administration
STEREO-B SECCHI HI Level 2 produced by UK Solar System Data Centre

\nSTEREO-B SECCHI HI Level 2 FITS files produced by the UK Solar System Data Centre, calibrated and background subtracted.  Images stored in FITS files with filenames such as "20140101_180501_24h1A_br11.fts". The meaning of the different parts of this filename is as follows:\n\n* 20140101 is the observation date, 2014-01-01;\n* 180501 is the observation time, 18:05:01 UT;\n* 2 represents Level-2;\n* 4 is a code for the data units, where 4=Dn/Sec/Pixel, b=Mean Solar Brightness (MSB), and t=S10. MSB \& S10 have the diffuse source correction applied;\n* h1 or h2 for HI-1 or HI-2;\n* A or B for STEREO-A or STEREO-B;\n* br for Buffinton/RAL background subtracted--a full running window where the F-corona is computed as the mean of the lowest quartile of pixels;\n* 11 is the length of the running window in days, usually either 01 or 11 for HI-1, and 03 or 11 for HI-2.\n

Tags: imageintensity
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 2 0834 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 2015-06-08T20:58:40.000 to 2015-06-09T06:15:34.500.

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Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 3 3272 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 2012-04-30T08:54:31.000 to 2012-04-30T13:10:24.500.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSINAC 4 ESC3-MTP019 RDR-STR-REFL V1.0

This CODMAC level 4 data set contains solar stray light corrected, radiometric calibrated and geometric distortion corrected (resampled) image data in in reflectance units (normalized and thus without unit), acquired by the OSIRIS Narrow Angle Camera on the Rosetta spacecraft during the COMET ESCORT 3 mission phase, covering the period from 2015-07-28T23:25:00.000 to 2015-08-25T23:24:59.000. 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
THEMIS-A (P5) Electron and Ion Moments (GMOM) Ground-Calculated Particle Energy Fluxes and Moments: Density, Velocity, Pressure and Temperature

THEMIS-A 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 RPCIES 3 ESC4 V2.0

This dataset contains CALIBRATED DATA of the Rosetta RPCIES instrument taken during the comet escort 4 phase (ESC4). The target of this phase was comet 67P/CHURYUMOV-GERASIMENKO 1 (1969 R1). Included are the data taken between 22 Oct 2015 and 31 Dec 2015. This version of the data has been reprocessed to remove an error introduced in the previous version.

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Organization: National Aeronautics and Space Administration
MGN V RDRS 5 COMPOSITE DATA RECORD ALT/RAD V1.0

This data set contains the Magellan Altimetry/Radiometry Composite Data Record (ARCDR). Along track estimates of elevation, Fresnel Reflectivity, surface roughness, brightness temperature, emissivity derived from Magellan altimeter and radiometer data.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSIWAC 4 ESC1-MTP012 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 Wide Angle Camera on the Rosetta spacecraft  during the COMET ESCORT 1 mission phase, covering the period  from 2015-01-13T23:25:00.000 to 2015-02-10T23:24:59.000. 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
STEREO-B SWAVES One minute Time Domain Sampler 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 at 250,000 samples/second. Antenna systems include three mutually orthogonal 6-meter monopoles. \n

Tags: stereo-b, swaves, waves-time-domain-sampler
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSIWAC 2 ESC2-MTP014 EDR V3.0

This CODMAC level 2 data set contains uncalibrated image data in DN unit, acquired by the OSIRIS Wide 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 V3.0 supersedes previous deliveries of the same dataset with the following changes since the last version: Lien corrected dataset after the July and October 2018 PSA/PDS external peer reviews. Updated documentation and ancillary files, added document on bandpass filter. Updated SCIENCE_USER_GUIDE_V03.PDF to include one section about FAQ and one section about image data quality. Added shutter backtravel and readout issues to image quality map. Updated DATA_QUALITY_ID keyword in image header. Improved handling of images with missing packets. Included FITs files. Browse products changed to the same size as the original image.

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Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 5 3856 V1.0

This is a Mars Express Radio Science data set, collected during the extended mission phase 2015-01-01 to 2016-12-31. It is a Occultation measurement and covers the time 2016-11-12T03:22:01 to 2016-11-12T04:07:00.

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Organization: National Aeronautics and Space Administration
STEREO-B SWAVES new one minute averages of the low (lfr) 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-low-frequency-receiver
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 3 1014 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 2015-09-04T21:27:30.000 to 2015-09-05T00:17:14.000.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER COMET ESCORT1 OSIWAC 2 EDR MTP 010 V1.0

This data set contains raw EDR images acquired by the OSIRIS Wide AngleCamera during the escort phase of the Rosetta mission at the comet 67P,covering the period from 2014-11-21 to 2014-12-19.

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Organization: National Aeronautics and Space Administration
MER2 MARS MINIATURE THERMAL EMISSION SPECTROMETER RDR V1.0

This archive contains Mars Exploration Rover Miniature Thermal EmissionSpectrometer (Mini-TES) Reduced Data Record (RDR) products and ancillary files. The Mini-TES RDR products archived on this volume are theoriginal products used during mission operations by the MarsExploration Rover project.

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Organization: National Aeronautics and Space Administration
STEREO-B/WAVES Low Frequency Receiver, Data

Radio measurements of power spectral density,radio flux density, Stokes Q, U, V parameters and angular half width of source measured by the STEREO-B/WAVES instrument. There a 48 linearly spaced frequency channels from 2.61 to 153 kHz. Time resolution varies with instrument mode ranging from 15 seconds to 1 minute.

Tags: electricfield, waves
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER COMET ESCORT OSIWAC 3 RDR MTP 016 V1.0

This data set contains calibrated images acquired by the OSIRIS Wide AngleCamera during the escort phase of the Rosetta mission at the comet 67P,covering the period from 2015-05-05 to 2015-06-02.

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Organization: National Aeronautics and Space Administration
THEMIS-A: On Board spin fits (FIT) of Electric (EFI) and Magnetic (FGM) field. On-Board Spin-fit electric and magnetic field data

THEMIS-A: On Board spin fits of Electric (EFI) and Magnetic (FGM) fields. This file contains data EFI and FGM that has been despun on-board to 3 second resolution. It stores meta information like the number of points that contributed to each spin and the standard deviation of those points. For the EFI data it also stores variables with the Z component of the EFI data zeroed and the Z component of the EFI estimated using the E.B=0 equality. The need to use an estimated Z axis for the EFI is due to error in measurements from the EFI axial booms. These data are provided in DSL (despun spacecraft L-Z vector), GSM, and GSE coordinates.

Tags: electricfield, magneticfield
Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 8 4184 V1.0

This is a Mars Express Radio Science data set, collected during the extended mission phase 2021-01-01 to 2022-12-31. It is a Occultation measurement and covers the time 2021-02-01T10:04:28.100 to 2021-02-01T10:26:36.649.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 ROSETTA EXTENSION 1 1315 V1.0

This is a Rosetta Radio Science data set, collected during the ROSETTA EXTENSION 1 phase 2016-01-01 to 2016-04-05. It is a Global Gravity measurement at the comet 67P and covers the time 2016-01-06T05:00:15.000 to 2016-01-06T09:37:19.500.

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Organization: National Aeronautics and Space Administration
THEMIS-A: ESA electron/ion energy fluxes and moments

THEMIS-A: Electrostatic Analyzers (ESA): Electron/Ion Ground-Calculated Energy Fluxes (5eV - 25 keV for Ions and 6eV - 30 KeV for Electrons) and Moments (density, velocity, pressure, and temperature). The satellite has 2 modes Fast and Slow survey and 3 data types: FULL, REDUCED and BURST. FULL: 88 angles x 32 energies, time resolution of 128 spins(395 seconds) in slow survey and 32 spins(98 seconds) in fast survey. REDUCED: spin time resolution(3 sec) but angles averaged into 1 angular spectra x 32 energies in slow survey or 6 angular spectra(90 degree x 90 degree window) x 32 energies in fast survey. BURST: 88 angles x 32 energies and spin time resolution(3 sec) but only available sporadically and for short duration. Note that angular resolution affects moments since they are obtained integrating over the mode-specific angular distribution. These moments are processed on the ground. They should be regarded as approximations but will improve in quality as our processing routines are improved over the course of the mission to account for additional sources of variance.

Tags: thermalplasma
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 2 0824 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 2015-06-03T09:28:35.000 to 2015-06-03T13:14:11.000.

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Organization: National Aeronautics and Space Administration
THEMIS-A: Solid State Telescope (SST): Energy flux spectrogram, electron/ion ground-calculated fluxes (30 keV - 300 keV).

THEMIS-A: The Solid State Telescope (SST) measures the incoming intensity (flux per solid angle) of superthermal electrons and ions. The spacecraft is fitted with two units (heads), each SST unit has two pairs of opposing ion and electron sensors. Each single sensor covers an angle of 36 degrees. The units are oriented such that one pair is always centered in the rotation plane, the other oriented at a maximum angle of 54 degrees off the plane. Each pair of units are oriented opposite each other allowing both ion and electron sensors to sweep out a maximum of 92% of the sky (45x45 degree required Elevation by Azimuth FOV, 108x22 raw) . The ion and electron sensors primarily measure particles between 30-300 keV and 30-100 keV respectively with a maximum capability of 20-6000 keV and 25-1000 keV. Full distribution data is measured over 128 angles and 16 energy bins, reduced distribution uses 6 angles and 16 energy bins, and burst mode data has 64 angles in 16 energy bins. Matched and paired electron broom magnets produce quadrapole fields reducing magnetic contamination. A mechanical attenuator is used to increase the instruments dynamical range avoiding oversaturation near the plasma sheet edge.

Tags: energeticparticles, ioncomposition, spectrum
Organization: National Aeronautics and Space Administration
MSL MARS SAMPLE ANALYSIS AT MARS 5 RDR LEVEL 2 V1.0

This archive contains Reduced Data Record (RDR) instrument data acquired by the Sample Analysis at Mars (SAM) instrument suite on the Mars Science Laboratory rover. SAM includes the Quadrupole Mass Spectrometer (QMS), the Gas Chromatograph (GC), and the Tunable Laser Spectrometer (TLS).

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 3 1009 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 2015-09-03T10:08:40.000 to 2015-09-03T17:29:51.500.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSIWAC 4 EXT3-MTP032 RDR-STR-REFL V1.0

This CODMAC level 4 data set contains solar stray light corrected, radiometric calibrated and geometric distortion corrected (resampled) image data in in reflectance units (normalized and thus without unit), acquired by the OSIRIS Wide Angle Camera on the Rosetta spacecraft during the ROSETTA EXTENSION 3 mission phase, covering the period from 2016-07-26T23:25:00.000 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
THEMIS-B 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
IHW COMET HALLEY INFRARED IMAGE DATA, V2.0

This data set contains the infrared images collected and archived by the International Halley Watch (IHW) Infrared Studies Network (IRSN). Raw and calibrated data are included, as well as calibration observations of standard stars. These data have been reformatted and the accompanying documentation updated in this revised version.

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Organization: National Aeronautics and Space Administration