AndreaBozzo/ceres-open-data-index huggingface dataset:
Voyager 2 Spacecraft Positions

Voyager 2 spacecraft positions generated from data at HelioWeb (cohoweb.gsfc.nasa.gov/helios/heli.html) These data were obtained from running the program HELICOOR in the public directory NSSDCA::ANON_DIR:[ACTIVE.HELIO]. These data are based on predicted trajectories calculated with the GTDS code by the NSSDC Satellite Situation Center and converted to solar ecliptic and heliographic coordinates by the HELIOCOOR program. The HELICOOR code was written by R. Parthasarathy. The program GENTRJCON added the HILLON longitude. Note that the solar ecliptic coordinates are given with respect to true equinox and ecliptic of date. The solar ascending node was located at ecliptic longitude +74.367 degrees as of 1 Jan. 1900 at 1200 UT; this longitude increases by 1.4 degrees/century.

Tags: ephemeris
Organization: National Aeronautics and Space Administration
Voyager 2 Uranus Cosmic Ray Subsystem (CRS) Electron Telescope D2 Counting Rates, Version 1.0, 96 s Summary Data

* Data Set Overview\n* =================\n\nCounting Rate from the D2 Detector in the Cosmic Ray Subsystem (CRS) Electron Telescope (TET) on Voyager 2 during the Uranus Encounter. The D2 Detector nominally responds to Electrons with Kinetic Energies above approximately 2.5 MeV (see Detector Description for Details).\n\n+------------------------------------------------------+\n| Parameter Characteristics      | Value               |\n--------------------------------------------------------\n| Sampling Parameter Name        | TIME                |\n| Sampling Parameter Resolution  | 6.0 SECONDS         |\n| Minimum Sampling Parameter     | N/A                 |\n| Maximum Sampling Parameter     | N/A                 |\n| Sampling Parameter Interval    | 96.0 SECONDS        |\n| Minimum available Sampling Int | 96.0 SECONDS        |\n| Sampling Parameter Unit        | SECOND              |\n| Data Set Parameter Name        | D2 RATE             |\n| Noise Level                    | 0.000 COUNTS/SECOND |\n| Data Set Parameter Unit        | COUNTS/SECOND       |\n+------------------------------------------------------+

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
DAWN VIR CAL (RDR) CERES VISIBLE SPECTRA  V1.0

This data set contains the spectralradiance (W/(m**2*sr*micron)) data from the Dawn VIR instrumentvisible channel for all Ceres encounter mission phases. The datacover the time period between 2014-12-26 and 2018-09-29.

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Organization: National Aeronautics and Space Administration
MER ALPHA PARTICLE X-RAY SPECTROMETER 5 OXIDE ABUNDANCE V1.0

This archive contains oxide abundance dataderived from the APXS Reduced Data Record (RDR) products on the Mars Exploration Rovers.The data consist of one file for each rover. When new APXS RDR dataappear in a MER release, the oxide abundance data are revised in thefollowing release approximately three months later. Hence the oxidedata lag behind the EDR and RDR data by one release.

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Organization: National Aeronautics and Space Administration
VG2 J/S/U/N/SS PLASMA WAVE SPECTROMETER RAW WFRM 60MS V1.0

This data set consists of electric     field waveform samples from the Voyager 2 Plasma Wave Subsystem waveform     receiver obtained during the entire mission.  Data after 2006-03-07 will     be added to the archive on subsequent volumes.  The data set encompasses     all waveform observations obtained in the cruise mission phases before,     between, and after the Jupiter, Saturn, Uranus, and Neptune encounter     phases as well as those obtained during the four encounter phases.

Tags: __
Organization: National Aeronautics and Space Administration
Voyager 2 Heliosphere Ephemeris in Heliographic and Solar Ecliptic Coordinates, Daily Data

* Data Set Overview\n* =================\n\nThese Data were obtained from running the Program HELICOOR in the Public Directory NSSDCA::ANON_DIR:[ACTIVE.HELIO]. These Data are based on predicted Trajectories calculated with the GTDS Code by the NSSDC Satellite Situation Center and converted to Solar Ecliptic COordinates and Heliographic Coordinates by the HELIOCOOR Program. The HELICOOR Code was written by R. Parthasarathy. The Program GENTRJCON added the HILLON Longitude.\n\nNote that the Solar Ecliptic Coordinates are given with respect to True Equinox and Ecliptic of Date. The Solar Ascending Node was located at Ecliptic Longitude +74.367° as of January 1, 1900 at 1200 UT. This Longitude increases by 1.4° per Century.\n\n* Data Formats\n* ============\n\nField      Description\n1. Date    YYYY DDD.DD where YY=Year and DDD.DD=Decimal Day\n2. Range   Heliocentric Range in AU\n3. SE_Lat  Solar Ecliptic Latitude in Degrees\n4. SE_Lon  Solar Ecliptic Longitude in Degrees\n5. HG_Lat  Heliographic Latitude in Degrees\n6. HG_Lon  Heliographic Longitude in Degrees\n7. IHG_Lon Inertial Heliographic Longitude in Degrees with respect to the Ascending Node of the Solar Equator in the Ecliptic.\n\n* Contact Information\n* ===================\n\n- R. P. (Sardi) Parthasarathy\n- Hughes STX Corporation / Space Physics Data Facility\n- NASA Goddard Space Flight Center\n- Greenbelt, Maryland\n- sardi@nssdca.gsfc.nasa.gov\n- Phone: (301) 286-8105\n\n* Acknowledgement\n* ===============\n\nUse of these Data in Publications should be accompanied at minimum by Acknowledgements of the National Space Science Data Center and the responsible Principal Investigator defined in the Experiment Documentation provided here.

Tags: ephemeris
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSIWAC 4 ESC1-MTP013 RDR V2.0

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 Wide Angle Camera on the Rosetta spacecraft during the COMET ESCORT 1 mission phase, covering the period from 2015-02-10T23:25:00.000 to 2015-03-10T23:24:59.000. The prime target is comet 67P/Churyumov-Gerasimenko 1 (1969 R1). This version V2.0 supersedes previous deliveries of the same dataset with the following changes since the last version: Lien corrected dataset after October 2018 PSA/PDS external peer review. 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.

Tags: __
Organization: National Aeronautics and Space Administration
CLEMENTINE BASEMAP MOSAIC

The Clementine Basemap Mosaic is a full-resolution (100 meters per pixel) global mosaic produced by the U.S. Geological Survey from Clementine EDR Data. The 750 nanometer filter imaging data acquired by the Ultraviolet/Visible Camera were used to create the single-band basemap mosaic.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 3 0912 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 2015-07-22T15:03:05.000 to 2015-07-22T17:32:34.500.

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Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 7 4009 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 2019-05-19T07:34:56.399 to 2019-05-19T07:57:04.449.

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Organization: National Aeronautics and Space Administration
NEW HORIZONS  ALICE KEMCRUISE1  RAW V2.0

This data set contains Raw data taken by the  New Horizons Alice Ultraviolet Imaging Spectrograph instrument  during the CRUISE TO FIRST KBO ENCOUNTER mission phase.  This is VERSION 2.0 of this data set.   This data set contains data acquired by the spacecraft between  01/11/2017 and 08/13/2018. This is the complete dataset.

Tags: __
Organization: National Aeronautics and Space Administration
LP ELECTRON REFLECTOMETER HIGH RES.        ELECTRON FLUX 5SEC V1.1

Time ordered high resolution data from theLunar Prospector Electron Reflectometer, accumulated over 1/2spacecraft spin, in units of particles/cm**2/sec/steradian/eV, for dates1998-01-16 to 1999-07-29.

Tags: __
Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3                                     EXTENDED MISSION 9 4408 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                                     2024-02-17T23:11:30.000 to                                     2024-02-17T23:33:38.300.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSINAC 4 PRL-MTP007 RDR-STRLIGHT V1.0

This CODMAC level 4 data set contains solar stray light corrected, radiometric calibrated and geometric distortion corrected (resampled) image data in W/m^2/sr/nm, acquired by the OSIRIS Narrow Angle Camera on the Rosetta spacecraft during the PRELANDING mission phase, covering the period from 2014-09-02T10:00:00.000 to 2014-09-23T09:59:59.000. 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
ROSETTA-ORBITER 67P GIADA 3 EXT2 EXTENSION 2 V1.0

Rosetta Extension 2 Phase covers the period of time from 6 April 2016 until 30 June 2016. It started after Rosetta successfully completed the Extension 1 Phase. The present DataSet collects the GIADA data of EXT2 phase. The GIADA Scientific phase started on 7 May 2014 and was devoted to the characterization of the 67P environment.

Tags: __
Organization: National Aeronautics and Space Administration
MARS EXPRESS SUN MRS 1/2/3 EXTENDED MISSION 4 3568 V1.0

This is a Mars Express Radio Science data set, collected during the extended mission phase 2013-01-01 to 2014-12-31. It is a Solar Conjunction measurement and covers the time 2013-04-27T08:46:36 to 2013-04-28T15:43:01.000.

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Organization: National Aeronautics and Space Administration
NEW HORIZONS LORRI KEM1 RAW V6.0

This data set contains Raw data taken by the New Horizons Long Range Reconnaissance Imager instrument during the KEM1 ENCOUNTER mission phase. This is VERSION 6.0 of this data set. This version includes data acquired by the spacecraft between 08/14/2018 and 04/30/2022. It only includes data downlinked before 05/01/2022. Future datasets may include more data acquired by the spacecraft after 08/13/2018 but downlinked after 04/30/2022. This version includes DKBO observations of 2011 HF103, 2011 HK103, 2011 HZ102, 2011 JA32, 2011 JW31, 2011 JX31, 2011 JY31, 2014 OE394, 2014 OJ394, 2014 OS393, 2014 PN70, 2020 KP11, 2020 KR11, and 2020 KT11, plus data from a Cosmic Optical Background Demo and a Microlensing demo. There are also observations of 50000 QUAOAR (2002 LM60), ASTEROID 307261 (2002 MS4), ASTEROID 486958 (2014 MU69), HD 37962, INTERPLANETARY DUST, M7, NGC 3532, PROXIMA CENTAURI, TRITON, and WOLF 359. It includes images of the approach and departure field around Arrokoth. The data cover the actual Arrokoth encounter.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSIWAC 4 ESC1-MTP012 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 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 October 2018 PSA/PDS external peer review.

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

This archive contains Mars Exploration Rover Miniature Thermal EmissionSpectrometer (Mini-TES) Brightness Temperature Reduced Data Record (BTR) products and ancillary files. The Mini-TES BTR products archived on this volume are the original products used during mission operations by the MarsExploration Rover project. Supporting documentation and label filesconform to the Planetary Data System (PDS) Standards, Version 3.6, JetPropulsion Laboratory (JPL) document number D-7669.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSIWAC 2 ESC1-MTP011 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 1 mission phase, covering the period from 2014-12-19T23:25:00.000 to 2015-01-13T23:24:59.000. 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.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER MARS RPCMIP 3 MARS V1.0

This archive contains data from the RPC-MIP instrument onboard ROSETTA Orbiter acquired during the MARS SWING-BY mission phase. It also contains documentation which describes the RPC-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
ROSETTA-ORBITER 67P OSIWAC 5 EXT1-MTP025 DDR-GEO V1.0

This CODMAC level 5 data set contains derived data products that include pixel-precise georeferencing information, acquired by the OSIRIS Wide Angle Camera on the Rosetta spacecraft during the ROSETTA EXTENSION 1 mission phase, covering the period from 2016-01-12T23:25:00.000 to 2016-02-09T23:24:59.000. 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.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 3 1023 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 2015-09-10T03:07:35.000 to 2015-09-10T15:46:13.000.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-LANDER 67P MUPUS 3 SDL V1.0

This archive contains calibrated data from the MUPUS instrument onboard ROSETTA Lander, acquired during the SDL phase. The primary target is the comet 67P/CHURYUMOV-GERASIMENKO. It also contains documentation which describes the MUPUS 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
VG1 SAT PLS DERIVED ION MAGNETOSHEATH                                      96SEC V1.0

This data set contains Voyager 1 plasma fit data from Saturn's      magnetosphere. The fit parameters assume a convected isotropic      proton Maxwellian distribution. Use of fit parameters is recommended      as these are normally more accurate.  Since only the first 72 or last      72 energy/charge channels are telemetered to Earth from each M-mode      spectra, derived parameters change significantly only every other set      of spectra so the effective time resolution is 96 second.

Tags: __
Organization: National Aeronautics and Space Administration
MARS EXPRESS SUN MRS 1/2/3 EXTENDED MISSION 4 3565 V1.0

This is a Mars Express Radio Science data set, collected during the extended mission phase 2013-01-01 to 2014-12-31. It is a Solar Conjunction measurement and covers the time 2013-04-25T15:40:41 to 2013-04-26T15:40:27.000.

Tags: __
Organization: National Aeronautics and Space Administration
VOYAGER 2 SATURN MAGNETOMETER RESAMPLED DATA 1.92 SEC

This data set includes Voyager 2 Saturn encounter magnetometer data that have been resampled at a 1.92 second sample rate. The data set is composed of 6 columns: 1) ctime - this column contains the data acquisition time. The time is always output in the ISO standard spacecraft event time format (yyyy-mm-dd-Thh:mm:ss.sss) but is stored internally in Cline time which is measured in seconds after 00:00:00.000 Jan 01, 1966, 2) br - this column contains the radial component of the magnetic field, 3) bphi - this column contains the phi component of the magnetic field, 4) btheta - this column contains the theta component of the magnetic field, 5) bmag - this column contains the magnitude of the magnetic field, 6) flag - a flag value that indicates either software error or spacecraft hardware interference reduced confidence in this record (flag value of 1 is bad , 0 is good or unchecked). All magnetic field observations are measured in nanoTeslas. The coordinate system for this dataset is Minus Saturn Longitude System (-SLS). All of the magnetic field data are calibrated (see the instrument calibration description for more details). The SLS coordinate system is defined in Desch and Kaiser, 1981 and the reference documents for this dataset are: Ness et al, 1982 Acuna,Connerney,and Ness, 1983 Connerney,Acuna,and Ness, 1983 Behannon,Lepping,and Ness, 1983

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER X SREM 5 CRUISE 4B 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 CRUISE 4B mission phase.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSIWAC 4 ESC3-MTP018 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 2015-06-30T23:25:00.000 to 2015-07-28T23:24:59.000. 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
Voyager 2 48-s Triaxial Fluxgate Magnetometer (MAG) Magnetic Field Data in ASCII Format

The average magnetic field strength produced by the spacecraft at the location of the \n        outboard magnetometer, of the dual magnetometers system on V2, varies between 0.1 and 0.2 nT, comparable \n        to the most probable magnetic field strength in the inner heliosheath and significantly larger \n        than the most probable magnetic field strength in the distant supersonic solar wind. The spacecraft \n        magnetic field is a complex, time-dependent signal that must be removed from the measured magnetic \n        field signal in order to derive the ambient magnetic fields of the solar wind and heliosheath.  \n        Corrections must also be made for spurious magnetic signals and noise associated with the telemetry \n        system, ground tracking systems, and other factors. Extracting the signal describing the solar wind \n        and heliosheath from the many sources of uncertainty is a complex and partly subjective process that \n        requires understanding of the instrument and judgment based on experience in dealing with the \n        ever-changing extraneous signals. We estimate that the 1-sigma uncertainty in the 48 sec averages \n        in the components of the magnetic field is typically +/- 0.02 nT. The uncertainties in F1, BR, BT, \n        and BN can differ from one another and they may vary with time, but there is no practical way to \n        determine these uncertainties more precisely at present.  This descriptor, and the data\n        access path identified below, are specific to 48s Voyager 2 MAG data taken when the spacecraft\n        was in the vicinity of, and beyond, the heliospheric termination shock.\n        References \n        \n        Behannon, K.W., M.H. Acuna, L.F. Burlaga, R.P. Lepping, N.F. Ness, and F.M. Neubauer, \n        Magnetic-Field Experiment for Voyager-2 and Voyager-2, Space Science Reviews, 21 (3), 235-257, 1977. \n\n        Burlaga, L.F., Merged interaction regions and large-scale magnetic field fluctuations during 1991 - \n        Voyager-2 observations, J. Geophys. Res., 99 (A10), 19341-19350, 1994. \n\n        Burlaga, L.F., N.F. Ness, Y.-M. Wang, and N.R. Sheeley Jr., Heliospheric magnetic field strength and \n        polarity from 1 to 81 AU during the ascending phase of solar cycle 23, J. Geophys. Res., 107 (A11), 1410, 2002. \n\n        Ness, N., K.W. Behannon, R. Lepping, and K.H. Schatten, J. Geophys. Res., , 76, 3564, 1971.\n        \n

Tags: magneticfield
Organization: National Aeronautics and Space Administration
JUNO J ENERGETIC PARTICLE DETECTOR UNCALIBRATED V1.0

Abstract                                                                      ========                                                                        This data set consists of the JUNO JEDI (Jupiter Energetic-Particle           Detector) uncalibrated observations, also known as EDRs. The system           is made up of 3 instrument subsystems (pucks) aligned in three                directions on the spinning JUNO spacecraft. The pucks each have 6 look        directions (telescopes) with a time of flight (TOF) and a deposited           energy detection (SSD) system.  In addition, the pulse height of the          signal in the TOF system can be used for energy measurement. The              instruments can be operated in a variety of modes, differing in the           way they use and combine these measurements. More details are available       in the INSTRUMENT.CAT file and the JEDI SIS.                                                                                                                The EDRs are organized in files covering one day of spacecraft event          time (SCET). There are potentially 10 different files per puck,               corresponding to the available data gathering modes: HIERSESP,                HIERSISP, HIERSTOFXER, HIERSTOFXPHR, LOERSESP, LOERSISP, LOERSTOFXER,         LOERSTOFXPHR, NONPTOFXER, NONPTOFXPHR. Depending on how the pucks are         operated, not all data types will be available for all pucks for any          particular time range.

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Organization: National Aeronautics and Space Administration