AndreaBozzo/ceres-open-data-index huggingface dataset:
ISIS-2 Topside Sounder Average Ionogram over Santiago, Chile: SNT, Latitude -33, Longitude 298

These Ionograms were digitized from the original ISIS-2 7-Track Analog Telemetry Tapes using the Facilities of the former Data Evaluation Laboratory at the NASA/GSFC. This Data Restoration Project is headed by Dr. R.F. Benson (NASA/GSFC). Ionograms were digitized at the Rate of 40,000 16-bit samples/s. This Sample Rate is higher than the Nyquist Frequency of 30 kHz. The Sample Frequency of 40 kHz provides a Measurement every 25 &#181;s corresponding to an Apparent Range Interval equal to 3.75 km from c*t/2, where c is the Speed of Light. Ionograms with this Sample Rate are designated as &apos;Full&apos; Ionograms because they have the full 3.75 km Apparent-Range Resolution. The Ionograms used for most Analyses, and those available from CDAWeb, were produced by averaging every four Samples of the Sounder-Receiver Video Amplitude Output to yield an average Value every 100 &#181;s corresponding to an Apparent-Range Resolution of 15 km. These Ionogram Files are referred to as &apos;Average&apos; Files with Standard Resolution. Each Ionogram consists of a Fixed-Frequency Portion and a Swept-Frequency Portion. The Time Resolution between Ionograms is typically 14 or 22 s depending on the Frequency Sweep Range.

Tags: auroral-kilometric-radiation-akr, ducted-echoes, field-aligned-irregularities-fai, ground-echoes, ground-reflections, ionospheric-echoes, ionospheric-reflections, plasma-resonance, plasma-waves, solar-type-iii-bursts, spectrum, swept-frequency-sounder, topside-ionosphere, topside-sounder, upper-hybrid-noise-band, wave-scattering, waves-active-ionogram
Organization: National Aeronautics and Space Administration
MARS EXPRESS SUN MRS 1/2/3 EXTENDED MISSION 5 3780 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 Solar Conjunction measurement and covers the time 2015-06-26T23:23:01 to 2015-06-27T05:09:00.

Tags: __
Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3                                     EXTENDED MISSION 8 4318 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 Occultation                                     measurement and covers the time                                     2023-08-07T07:17:00.300 to                                     2023-08-07T07:39:08.000.

Tags: __
Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 6 3892 V1.0

This is a Mars Express Radio Science data set, collected during the extended mission phase 2017-01-01 to 2018-12-31. It is a Occultation measurement and covers the time 2017-01-30T03:34:01 to 2017-01-30T04:19:00.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER EARTH OSINAC 4 EAR1 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 EARTH SWING-BY 1 mission phase, covering the period  from 2004-10-17T00:00:00.000 to 2005-04-04T23:59:59.000. The prime target is planet Earth. This version V1.0 is the first version of this dataset.

Tags: __
Organization: National Aeronautics and Space Administration
LANL 1989 Magnetospheric Plasma Analyzer (MPA) at 87 sec Resolution in Spacecraft Coordinates

The LANL 1989-046 MPA data set contains various parameters in a variety of coordinates systems including GEI, spacecraft, polar geographic, and polar magnetic coordinates at about 87 s resolution. These parameters include universal time, denisty, velocity, and temperature for both low and high energy ions and electrons as well as position information and instrument status flags.

Tags: energeticparticles-87-sec, geosynchronous, lanl, magnetospheric-plasma-analyzer, mpa
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P MIDAS 3 ESC4 SAMPLES 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 theCOMET ESCORT 4 mission phase.This release supersedes version 2.0.

Tags: __
Organization: National Aeronautics and Space Administration
ISIS-2 Topside Sounder Average Ionogram over Sodankyla, Finland: SOD, Latitude 67, Longitude 27

These Ionograms were digitized from the original ISIS-2 7-Track Analog Telemetry Tapes using the Facilities of the former Data Evaluation Laboratory at the NASA/GSFC. This Data Restoration Project is headed by Dr. R.F. Benson (NASA/GSFC). Ionograms were digitized at the Rate of 40,000 16-bit samples/s. This Sample Rate is higher than the Nyquist Frequency of 30 kHz. The Sample Frequency of 40 kHz provides a Measurement every 25 &#181;s corresponding to an Apparent Range Interval equal to 3.75 km from c*t/2, where c is the Speed of Light. Ionograms with this Sample Rate are designated as &apos;Full&apos; Ionograms because they have the full 3.75 km Apparent-Range Resolution. The Ionograms used for most Analyses, and those available from CDAWeb, were produced by averaging every four Samples of the Sounder-Receiver Video Amplitude Output to yield an average Value every 100 &#181;s corresponding to an Apparent-Range Resolution of 15 km. These Ionogram Files are referred to as &apos;Average&apos; Files with Standard Resolution. Each Ionogram consists of a Fixed-Frequency Portion and a Swept-Frequency Portion. The Time Resolution between Ionograms is typically 14 or 22 s depending on the Frequency Sweep Range.

Tags: auroral-kilometric-radiation-akr, ducted-echoes, field-aligned-irregularities-fai, ground-echoes, ground-reflections, ionospheric-echoes, ionospheric-reflections, plasma-resonance, plasma-waves, solar-type-iii-bursts, spectrum, swept-frequency-sounder, topside-ionosphere, topside-sounder, upper-hybrid-noise-band, wave-scattering, waves-active-ionogram
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 1 0540 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 2015-01-17T03:34:45.000 to 2015-01-17T11:33:30.000.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 4 1167 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 2015-11-09T08:13:10.000 to 2015-11-09T11:03:25.000.

Tags: __
Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 5 3861 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 2016-11-19T03:17:01 to 2016-11-19T04:02:00.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER MARS OSIWAC 2 MARS EDR V2.0

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 MARS SWING-BY mission phase, covering the period  from 2006-07-29T00:00:00.000 to 2007-05-28T23:59:59.000. The prime target is planet Mars. This version V2.0 supersedes previous deliveries of the same dataset with the following changes since the last version: Reprocessed 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 2 0799 V1.0

This is a Rosetta Radio Science data set, collected during the COMET ESCORT 2 phase 2015-03-11 to 2015-06-30. It is a Global Gravity measurement at the comet 67P and covers the time 2015-05-22T04:48:05.000 to 2015-05-22T06:47:42.500.

Tags: __
Organization: National Aeronautics and Space Administration
ISIS-2 Topside Sounder Average Ionogram over Tromso, Norway: TRO, Latitude 70, Longitude 19

These Ionograms were digitized from the original ISIS-2 7-Track Analog Telemetry Tapes using the Facilities of the former Data Evaluation Laboratory at the NASA/GSFC. This Data Restoration Project is headed by Dr. R.F. Benson (NASA/GSFC). Ionograms were digitized at the Rate of 40,000 16-bit samples/s. This Sample Rate is higher than the Nyquist Frequency of 30 kHz. The Sample Frequency of 40 kHz provides a Measurement every 25 &#181;s corresponding to an Apparent Range Interval equal to 3.75 km from c*t/2, where c is the Speed of Light. Ionograms with this Sample Rate are designated as &apos;Full&apos; Ionograms because they have the full 3.75 km Apparent-Range Resolution. The Ionograms used for most Analyses, and those available from CDAWeb, were produced by averaging every four Samples of the Sounder-Receiver Video Amplitude Output to yield an average Value every 100 &#181;s corresponding to an Apparent-Range Resolution of 15 km. These Ionogram Files are referred to as &apos;Average&apos; Files with Standard Resolution. Each Ionogram consists of a Fixed-Frequency Portion and a Swept-Frequency Portion. The Time Resolution between Ionograms is typically 14 or 22 s depending on the Frequency Sweep Range.

Tags: auroral-kilometric-radiation-akr, ducted-echoes, field-aligned-irregularities-fai, ground-echoes, ground-reflections, ionospheric-echoes, ionospheric-reflections, plasma-resonance, plasma-waves, solar-type-iii-bursts, spectrum, swept-frequency-sounder, topside-ionosphere, topside-sounder, upper-hybrid-noise-band, wave-scattering, waves-active-ionogram
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P NAVCAM 2 ROSETTA EXTENSION 3 MTP035 V1.1

This dataset contains ROSETTA NAVCAM RAW DATA of the Extension 3 Phase from 26th Sep 2016 to 30th Sep 2016 when at the vicinity of target 67P/CG. 30th Sep 2016 is the end of the Rosetta mission. This data set V1.1 supersedes the V1.0. It includes document updates and resolve other outstanding errata.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSINAC 4 EXT3-MTP034 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 ROSETTA EXTENSION 3 mission phase, covering the period from 2016-09-02T06:40:00.000 to 2016-09-26T06:39:59.000. 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
LANL 1990 Geosynchronous Orbit Particle Analyzer (SOPA) at 60 sec Resolution in Spacecraft Coordinates

The LANL 1990-095 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
DERIVED GEOPHYSICAL ARROKOTH ENCOUNTER DATA V1.0

This data set contains higher level products derived from data taken by the LOng-Range Reconnaissance Imager (LORRI) and the Multispectral Visible Imaging Camera (MVIC) instruments during the Arrokoth encounter phase of the New Horizons Kuiper Belt Extended Mission. Arrokoth shape models, Arrokoth surface and subsurface temperature simulations, and Arrokoth albedo and normal reflectance maps are included. The simulation results predict temperatures at various sub- surface depths on dates as Arrokoth orbits the Sun. This is VERSION 1.0 of this data set.

Tags: __
Organization: National Aeronautics and Space Administration
IBEX-Hi digital maps every 6 months

As of this writing (11/5/2010), this product \nhad been issued by the IBEX team in two releases. \nRelease 1 IBEX-Hi map data are superseded by Release 2\ndata which are more time-extensive (12 months vs. 6 months)\nand are richer in content.  While Release 1 IBEX-Hi map data \nand their documentation remain accessible at\nftp://nssdcftp.gsfc.nasa.gov/spacecraft_data/ibex/hi/maps/digital_data/release_1/\nand\nftp://nssdcftp.gsfc.nasa.gov/spacecraft_data/ibex/hi/maps/images/release_1/,\nthis description supports the retrieval and use of Release 2 data only.\n\nThe Release_2 IBEX-Hi map data contain all-sky 6 deg x 6 deg \nresolution maps in J2000 ecliptic coordinates of energetic \nneutral fluxes reaching the near-Earth IBEX spacecraft from \nthe distant heliosphere and heliosheath.  Maps \nare in both a spacecraft frame and, via Compton-Getting \ncorrections, a heliospheric frame.  Basic maps are each \naccumulated over 6-months duration, so far for epochs 1 \n(12/2008-06/2009) and 2 (06/2009-12/2009).  Maps are available \nfor five of the energy bands of IBEX-Hi (0.52-0.95, 0.84-1.55, \n1.36-2.50, 1.99-3.75, 3.13-6.00 keV) and, for the heliospheric \nframe only, also for six monoenergetic points (0.71, 1.11, 1.74, \n2.73, 3.0, 4.29 keV).  In addition, monoenergetic maps are available\nas summed over the data collected during epochs 1 and 2 combined.\nAll maps are available in digital text format and in PNG image format\n(considered as separate data sets within VEPO).\n\nGiven that VHO/VEPO typically displays clickable granule (file)\nnames for any given specification of data product and time span,\nand given that IBEX-Hi digital maps and PNG-formatted display\nmaps are each considered single data products, a request for data\nfrom either product will yield .GE.20 names of files containing data\nspanning or within the requested time span.  For IBEX, the names\nshown by VHO/VEPO actually have the form subdirectory/filename.\nThe subdirectories are named map1, map1cg, map2, map2cg, and\nmap-combined.  Maps involving "1" ("2") are from the first (second)\n6-month epoch, while "combined" means composed of data taken\nduring epochs 1 and 2.  Maps involving (not involving) "cg" means\nheliospheric frame (spacecraft frame).  In the first four subdirectories,\nfile names are of the forms ha60.hide-trp-flux100-hi-N-flux.ext and\nha60.hide-trp-mono_80-P.PP-flux.ext, where "ext" is "png" or "txt"\naccording to which product is requested,  N is the energy step\nnumber for the IBEX-Hi instrument (2-6), P.PP is the energy level,\nin keV, of a monoenergetic flux.  Files in the "combined"\nsubdirectories are named "combined-P.PP-flux.ext, where P.PP\nhas the same meaning as above.\n\nIn addition to the flux maps to which VEPO provides access, \nseveral map files whose data support the determination of the \nfluxes are also available in the underlying nssdcftp directories \nand are described by aareadme files there (and by IBEX web pages \nat SWRI: http://ibex.swri.edu/ibexpublicdata/Data_Release_2/)

Tags: neutralatomimages
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 3 0975 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 2015-08-20T21:32:25.000 to 2015-08-21T05:23:01.000.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 2 0778 V1.0

This is a Rosetta Radio Science data set, collected during the COMET ESCORT 2 phase 2015-03-11 to 2015-06-30. It is a Global Gravity measurement at the comet 67P and covers the time 2015-05-15T12:25:35.000 to 2015-05-15T15:16:47.000.

Tags: __
Organization: National Aeronautics and Space Administration
PVO VENUS MAG RESAMPLED SC COORDS 24SEC AVGS V1.0

This dataset contains vectors collectedby the Pioneer Venus Orbiter (previously Pioneer 12) Magnetometer which havebeen averaged over 24 seconds on 12 second centers. The data are provided inspacecraft coordinates whose system has it Z axis antiparallel to thespacecraft spin axis during orbit.  This choice maintained the Z axisalong roughly the Earth's ecliptic north pole. Late in the missionwhen it was believed that the shadowing of the solar panels bythe booms was causing a problem, the spin axis was moved to thepole of the Venus orbital plane.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 2 0722 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 2015-04-21T21:18:30.000 to 2015-04-22T00:14:05.000.

Tags: __
Organization: National Aeronautics and Space Administration
LANL1994Magnetospheric Plasma Analyzer (MPA) at 87 sec Resolution in Spacecraft Coordinates

The LANL 1994-084 MPA data set contains various parameters in a variety of coordinates systems including GEI, spacecraft, polar geographic, and polar magnetic coordinates at about 87 s resolution. These parameters include universal time, denisty, velocity, and temperature for both low and high energy ions and electrons as well as position information and instrument status flags.

Tags: energeticparticles-87-sec, geosynchronosus, lanl, magnetospheric-plasma-analyzer, mpa
Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3                                     EXTENDED MISSION 8 4347 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 Occultation                                     measurement and covers the time                                     2023-10-08T22:28:05.000 to                                     2023-10-09T04:55:01.000.

Tags: __
Organization: National Aeronautics and Space Administration
GALILEO ORBITER AT JUPITER CALIBRATED MAG HIGH RES V1.0

This data set contains high time resolution magnetic field vectors      acquired by the Galileo magnetometer (MAG). It includes both      satellite flyby and non-flyby data. These data were acquired in      order to characterize various portions of the Jovian magnetosphere      at high time resolution. The Galileo Magnetospheres Working Group      (MWG) collectively acquired high time resolution data for short      intervals in order to try and regain some of the magnetospheric      science lost due to the low data rates of the phase 2 mission (no      high gain antenna) mission. These observations are scattered in      Jovian distance, local time, System III longitude, etc. in order      to provide some insight into processes that may be active in      different regions of the magnetosphere.

Tags: __
Organization: National Aeronautics and Space Administration
LANL 1991 Geosynchronous Orbit Particle Analyzer (SOPA) at 60 sec Resolution in Spacecraft Coordinates

The LANL 1991-080 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
ROSETTA-ORBITER 67P OSINAC 3 ESC2-MTP015 RDR V3.0

This CODMAC level 3 data set contains radiometric calibrated image data in W/m^2/sr/nm, acquired by the OSIRIS Narrow Angle Camera on the Rosetta spacecraft during the COMET ESCORT 2 mission phase, covering the period from 2015-04-08T11:25:00.000 to 2015-05-05T23:24:59.000. 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
DAWN GRAND CALIBRATED (RDR) CERES COUNTS V1.0

The GRaND Reduced Data Records (RDR) contain a timeseries of calibrated spectra, counting data, and ephemeris, pointing,and geometry (EPG) data. The EPG data are contained in a single file,with an entry for every science data record acquired by GRaND within thedataset start-stop times. Each record has a unique identifier,spacecraft clock ticks, which is used as a serial number to identify datafrom the same record in other files containing spectra and counting data.The RDR data set includes a time series of corrected gamma ray spectraacquired by GRaND's bismuth-germanate (BGO) scintillator.

Tags: __
Organization: National Aeronautics and Space Administration
ISIS 2 CRC Electron Density Profiles

This data set, provided by the Communications Research Centre (CRC) in Ottawa, Canada, consists of electron density profiles for the ionosphere above the F2 maximum (topside ionosphere). The data are computed from digital values of frequency and virtual height, scaled from ionograms that are measured by the ISIS 2 (International Satellites for Ionospheric Studies) Swept-Frequency Sounder. The data are ordered chronologically. Telemetry stations are not identified, but satellite location, Greenwich mean time of observation, solar zenith angle at the satellite, dip latitude at the satellite, total electron content down to the lowest height of topside signal reflection (normally near 300 km), and other relevant information is noted with each profile. The format gives sequences of numbers for each point scaled from the ionogram. These sequences include electron density at the successive points, and the coefficients a2, b3, b4, b5, etc. from which geometric heights can be calculated, using formulas 40 and 41 in J. E. Jackson, "The reduction of topside ionograms to electron-density profiles," Proceedings of the IEEE., p. 960, June 1969. These formulas can also be used to calculate interpolated density-height values. A CRC interpolation program (available at NSSDC) can be used with this data set.  (

Tags: profile
Organization: National Aeronautics and Space Administration
CASSINI ORBITER MAG CALIBRATED SUMMARY 1 MINUTE AVERAGE V2.0

This data set contains calibrated 1 minute averaged Cassini      magnetometer data, for the entire Cassini mission. These data are      provided in Kronographic (KRTP, KSO, KSM) coordinates at Saturn,      Geographic coordinates (GSE, GSM) for the Earth flyby, Jovigraphic      coordinates for the Jupiter flyby, and RTN coordinates for the entire      mission. These data were calibrated, converted to physical coordinates      and averaged to 1 minute by the Cassini MAG team at Imperial College.

Tags: __
Organization: National Aeronautics and Space Administration