AndreaBozzo/ceres-open-data-index huggingface dataset:
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 3 0935 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 2015-08-02T10:07:45.000 to 2015-08-02T17:27:32.500.

Tags: __
Organization: National Aeronautics and Space Administration
PVO VENUS MAG CALIBRATED P-SENSOR HIGH RES V2.0

This dataset contains full resolutionmagnetometer data from the Pioneer Venus Orbiter spacecraft beginning withorbit 3602 (Oct 16, 1988) and continuing until the orbiter was lost in theVenusian atmosphere (orbit 5055, Oct 7, 1992). The dataset differs from thehigh resolution magnetometer dataset from theprevious orbits due to ananomaly in the multiplexor that controlled the sampling of the magnetometersensors. During orbit 3602, and for the remainder of the mission, thespacecraft downlink contained magnetometer data from only the P sensor. TheP sensor is the sensor which is aligned with the spacecraft spin axis,nominally in the direction of the ecliptic normal.

Tags: __
Organization: National Aeronautics and Space Administration
Wind Linearly Interpolated 60 s Resolution Tri-axial Fluxgate Magnetometer in GSE Coordinates

Wind linearly interpolated to have the measurements on the minute at 60 s resolution tri-axial fluxgate magnetometer data in GSE coordinates. This data set consists of processed solar wind data that has been linearly interpolated to 1 min resolution at the position of the spacecraft using the interp1.m function in MATLAB. This data set was originally constructed by Dr. J.M. Weygand for Prof. R.L. McPherron, who was the principle investigator of two National Science Foundation studies: GEM Grant ATM 02-1798 and a Space Weather Grant ATM 02-08501. These data were primarily used in superposed epoch studies and cross correlation studies on solar wind. There are now two version of this data set. An off set has been found in the Wind MFI Bz component that is present after November 2004. Version 2 has this offset removed. Prof. R.L. McPherron determined the correction to be Bz = Bz - (-0.000000130406219.*odoy.*odoy + 0.000576303146.*odoy + 0.679940509 + 0.3215*cos(2*pi*(doy-171)/366)) where doy is the day of the year in units of days and odoy is the days sinces Jan 1, 1999 00:00:00 UT in units of days.

Tags: bow-shock, magnetic-fields, magneticfield-1-min, magnetometer, magnetopause, magnetotail, solar-wind, wind
Organization: National Aeronautics and Space Administration
MARS EXPRESS SUN MRS 1/2/3 EXTENDED MISSION 3 2787 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 Solar Conjunction measurement and covers the time 2011-03-03T15:45:40 to 2011-03-03T17:44:58.500.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSIWAC 4 PRL-MTP009 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 PRELANDING mission phase, covering the period from 2014-10-24T10:00:00.000 to 2014-11-21T23:24:59.000. 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
Wind 3DP EESA-LOW Electron Pitch-Angle Distributions

Wind 3DP electron pitch angle product providing electron fluxes in 8 directional bins relative to the local magnetic field direction at 15 different energy levels. Time resolution is mode- dependent, with 96s being used for the past several years and with higher resolution (e.g., 24s) used for some earlier intervals. For any given cadence, electron observations made over the full cadence interval and in all look directions in and out of the spacecraft spin plane, are folded together with the magnetic field vector as averaged over the cadence interval, to produce the pitch angle distributions. The data are calibrated science quality data.

Tags: thermalplasma
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 PRELANDING 0361 V1.0

This is a Rosetta Radio Science data set, collected during the PRELANDING phase 2014-01-21 to 2014-11-18. It is a Global Gravity measurement at the comet 67P and covers the time 2014-10-15T10:50:11.000 to 2014-10-15T15:09:51.500.

Tags: __
Organization: National Aeronautics and Space Administration
EPOXI 103P/HARTLEY2 ENCOUNTER - HRII CALIBRATED SPECTRA V3.0

This dataset contains calibrated, 1.05- to 4.8-micron spectral images of comet 103/P Hartley 2 acquired by the High Resolution Infrared Spectrometer (HRII) from 01 October through 26 November 2010 during the Hartley 2 encounter phase of the EPOXI mission. Version 3.0 includes the application of scaled master dark subtraction for DOY 307 and in scene dark subtraction for DOY 311-313, as well as the use of an average per scan optical bench temperature in the pipeline processing. Version 3 also includes the calibration enhancements implemented in Version 2 of this dataset: a new per-pixel linearity correction treatment and its propagation through the calibration steps (i.e., bad-pixel maps, flat-field file update, revised spectral calibration curve), new mode-dependent master darks, an optimized scaling factor for the master dark, and a refinement in the absolute spectral calibration curve.

Tags: __
Organization: National Aeronautics and Space Administration
Wind 3DP Solar Wind Plasma Corrected Electron Moments (EMFITS), 100 s Data

These Electron Parameters are Moments of Wind 3DP EESA-L and EESA-H Measurements, corrected for Spacecraft Potential and other Instrumental Effects. More Information can be found at: R. P. Lin et al., A Three-Dimensional Plasma and Energetic Particle Investigation for the Wind Spacecraft, Space Science Reviews, 71, 125-153, 1995. C. S. Salem et al., Precision Electron Measurements in the Solar Wind at 1 AU from NASA's Wind Spacecraft, J. Geophys. Res. Space Physics, 2017. M. Pulupa et al., Spin-Modulated Spacecraft Floating Potential: Observations and Effects on Electron Moments, J. Geophys. Res. Space Physics, 119, 647-657, doi:10.1002/2013JA019359, 2014.

Tags: thermalplasma
Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 4 3599 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 Global Gravity measurement and covers the time 2013-07-10T23:49:08.000 to 2013-07-11T02:41:19.500.

Tags: __
Organization: National Aeronautics and Space Administration
Wind Definitive Attitude, 10 min Data, Spin Axis Orientation Angles in GCI, GSE and GSM Coordinates

Wind Definitive Attitude Body Spin Rate and Spin Axis Orientation Right Ascension and Declination Angles in Geocentric Celestial Inertial, GCI, Geocentric Solar Ecliptic, GSE, and Geocentric Solar Magnetospheric, GSE, Coordinates

Tags: ephemeris
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 2 0751 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 2015-05-04T23:08:05.000 to 2015-05-05T07:21:42.000.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 PRELANDING 0303 V1.0

This is a Rosetta Radio Science data set, collected during the PRELANDING phase 2014-01-21 to 2014-11-18. It is a Global Gravity measurement at the comet 67P and covers the time 2014-09-19T06:02:02.000 to 2014-09-19T14:37:11.000.

Tags: __
Organization: National Aeronautics and Space Administration
Wind EPACT/LEMT 1-Hr He,C,O,Ne,Si,Fe Solar Energetic Particle Intensities Level 2 Data

Hourly-averaged fluxes of He, C, O Ne,Si, Fe nuclei in the general range 2-11 MeV/n. Poisson uncertainties are given for each flux.

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 1 0616 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 2015-03-02T13:36:00.000 to 2015-03-02T14:35:59.000.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P/CAL ALICE 4 PRL V1.0

This data set contains CODMAC level 4 data acquired by the Rosetta Orbiter ALICE UV Spectrometer during the comet 67P/Churyumov-Gerasimenko prelanding mission phase, which took place between 2014-01-21 and 2014-11-18.

Tags: __
Organization: National Aeronautics and Space Administration
Wind Energetic Particle Acceleration, Composition and Transport (EPACT) APE-B Telescope Proton Fluxes 18.90 to 21.90 MeV, Level 2, 1 hr Data

The Energetic Particles: Acceleration, Composition and Transport, EPACT, on Wind. The APE-B Telescope measures Proton Fluxes at Particle Energies of 18.90 MeV to 21.90 MeV.

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
VG1/VG2 JUPITER IRIS DERIVED GREAT RED SPOT PARAMETERS V1.0

The data set contains Jovian atmospheric parameters derived from spectra obtained with the Voyager infrared interferometer spectrometer (IRIS). The data set is ordered by time as measured by the Flight Data System Count (FDSC). This represents the data frame number modulo 60. Also included in the data set are information on pointing and associated geometry of the measurements and brightness temperatures obtained from measured radiances at selected wavenumbers.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER/ROSETTA-LANDER CAL CONSERT 4 PHC V1.0

This archive contains REFORMATTED data (CODMAC level 4) that refers to target CALIBRATION from the CONSERT instrument onboard ROSETTA Orbiter and Lander, acquired during the PHC phase. In addition to the scientific signal of interest, it contains all the values applied to the signal for calibration. It also contains documentation which describes the CONSERT experiment. The L4 dataset includes interpolated signals using a specific CONSERT method. It also provide fine propagation travel times of the signal between Philae and Rosetta. The data archived in this data set conform to the Planetary Data System (PDS) Standards, Version 3.6.

Tags: __
Organization: National Aeronautics and Space Administration
Wind Energetic Particle Acceleration Composition Transport (EPACT) SupraThermal Energetic Particle Telescope (STEP) Differential Ion Fluxes, 1 h Data

The EPACT Instrument on Wind STEP - SupraThermal Energetic Particle Telescope measures Ion Fluxes of Protons (H) in 0.12.5 MeV Energy Range and He-Fe Nuclei in the ~0.032 MeV/nucleon Energy Ranges in two identical Telescopes, each with a Geometrical Factor of 0.4 cm^2 sr and a Rectangular Field

Tags: energeticparticles, ephemeris, magneticfield, thermalplasma
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER X SREM 2 EARTH 1 V1.0

This data set contains count rates (1/s) as measured by the Standard Radiation Environment Monitor (SREM) instrument on the Rosetta spacecraft, along with their standard deviations. These are CODMAC Level 2 Experiment Data Record data, and provide a measure of the radiation in the spacecraft environment during the EARTH 1 mission phase.

Tags: __
Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 7 3988 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 2019-04-07T09:35:52.000 to 2019-04-07T09:58:01.549.

Tags: __
Organization: National Aeronautics and Space Administration
Wind Energetic Particle Acceleration Composition Transport (EPACT) SupraThermal Energetic Particle Telescope (STEP) Differential, Directional Carbon, Nitrogen, and Oxygen Fluxes, 10 min Data

The EPACT Instrument on Wind STEP - SupraThermal Energetic Particle Telescope measures Ion Fluxes of Protons (H) in 0.12.5 MeV Energy Range and He-Fe Nuclei in the ~0.032 MeV/nucleon Energy Ranges in two identical Telescopes, each with a Geometrical Factor of 0.4 cm^2 sr and a rectangular Field of View with an Angular Acceptance of 44° in Azimuth and 17° in Polar Angle.

Tags: energeticparticles, ephemeris, magneticfield, thermalplasma
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RPCMAG 3 ESC1 CALIBRATED V9.0

This dataset contains CALIBRATED (CODMAC LEVEL 3) DATA of theCOMET ESCORT 1 Phase (ESC1) from November 22, 2014 until March 10, 2015of the ROSETTA orbiter magnetometer RPCMAG. Observations are done inthe vicinity of comet 67P/CHURYUMOV-GERASIMENKO 1 (1969 R1).The current version of the dataset is V9.0.The difference to the datasets of earlier versions is mainly a significantlyimproved sensor temperature model, more detailed documentation about magneticdisturbance sources, more data handling information for the user andalso an improved quality flagging system.

Tags: __
Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 4 3497 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 Global Gravity measurement and covers the time 2013-01-14T08:20:45.000 to 2013-01-14T11:19:54.500.

Tags: __
Organization: National Aeronautics and Space Administration
Wind Definitive Orbit, 10 min Data, Spacecraft Position and Velocity in GCI, GSE, GSM, HEC, and HG Coordinates

Wind Definitive Orbit, Spacecraft Position and Velocity in Geocentric Celestial Inertial, GCI, Geocentric Solar Ecliptic, GSE, Geocentric Solar Magnetospheric, GSM, Heliospheric Ecliptic, HEC, and Heliographic, HG, Coordinates

Tags: ephemeris
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER COMET ESCORT 4 OSIWAC 2 EDR MTP023 V1.0

This data set contains images acquired by the OSIRIS Wide Angle Camera during the COMET ESCORT 4 phase of the Rosetta mission at the comet 67P, covering the period from 2015-11-17T23:25:00.000 to 2015-12-15T23:24:59.000.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSIWAC 2 ESC3-MTP019 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 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 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
Wind Energetic Particle Acceleration Composition Transport (EPACT) SupraThermal Energetic Particle Telescope (STEP) Differential, Directional Hydrogen Fluxes, 10 min Data

The EPACT Instrument on Wind STEP - SupraThermal Energetic Particle Telescope measures Ion Fluxes of Protons (H) in 0.12.5 MeV Energy Range and He-Fe Nuclei in the ~0.032 MeV/nucleon Energy Ranges in two identical Telescopes, each with a Geometrical Factor of 0.4 cm^2 sr and a rectangular Field of View with an Angular Acceptance of 44° in Azimuth and 17° in Polar Angle.

Tags: energeticparticles, ephemeris, magneticfield, thermalplasma
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RPCIES 3 ESC1 V2.0

This dataset contains CALIBRATED DATA of the Rosetta RPCIES instrument taken during the comet escort 1 phase (ESC1). The target of this phase was comet 67P/CHURYUMOV-GERASIMENKO 1 (1969 R1). Included are the data taken between 20 Nov 2014 and 10 Mar 2015. This version of the data has been reprocessed to remove an error introduced in the previous version.

Tags: __
Organization: National Aeronautics and Space Administration
Wind 3DP Weimer Propagated 60 s Resolution in GSM Coordinates

Wind 3DP propagated solar wind data and linearly interpolated to have the measurements on the minute at 60 s resolution data in GSM coordinates. This data set consists of propagated solar wind data that has first been propagated to a position just outside of the nominal bow shock (about 17, 0, 0 Re) and then linearly interpolated to 1 min resolution using the interp1.m function in MATLAB. The input data for this data set is a 1 min resolution processed solar wind data constructed by Dr. J.M. Weygand. The method of propagation is similar to the minimum variance technique and is outlined in Dan Weimer et al. [2003; 2004]. The basic method is to find the minimum variance direction of the magnetic field in the plane orthogonal to the mean magnetic field direction. This minimum variance direction is then dotted with the difference between final position vector minus the original position vector and the quantity is divided by the minimum variance dotted with the solar wind velocity vector, which gives the propagation time. This method does not work well for shocks and minimum variance directions with tilts greater than 70 degrees of the sun-earth line. This data set was originally constructed by Dr. J.M. Weygand for Prof. R.L. McPherron, who was the principle investigator of two National Science Foundation studies: GEM Grant ATM 02-1798 and a Space Weather Grant ATM 02-08501. These data were primarily used in superposed epoch studies References: Weimer, D. R. (2004), Correction to ‘‘Predicting interplanetary magnetic field (IMF) propagation delay times using the minimum variance technique,’’ J. Geophys. Res., 109, A12104, doi:10.1029/2004JA010691. Weimer, D.R., D.M. Ober, N.C. Maynard, M.R. Collier, D.J. McComas, N.F. Ness, C. W. Smith, and J. Watermann (2003), Predicting interplanetary magnetic field (IMF) propagation delay times using the minimum variance technique, J. Geophys. Res., 108, 1026, doi:10.1029/2002JA009405. There are now two version of this data set. An off set has been found in the Wind MFI Bz component that is present after November 2004. Version 2 has this offset removed. Prof. R.L. McPherron determined the correction to be Bz = Bz - (-0.000000130406219.*odoy.*odoy + 0.000576303146.*odoy + 0.679940509 + 0.3215*cos(2*pi*(doy-171)/366)) where doy is the day of the year in units of days and odoy is the days sinces Jan 1, 1999 00:00:00 UT in units of days.

Tags: 1-min, 3dp, bow-shock, magnetopause, magnetotail, plasma-data, propagated-solar-wind-data, solar-wind, thermalplasma-1-min, wind
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER EARTH RPCMAG 4 EAR1 RESAMPLED V9.0

This dataset contains RESAMPLED DATA (CODMAC LEVEL 4) of the FIRST EARTHSWINGBY (EAR1) of the ROSETTA orbiter magnetometer RPCMAG.The closest approach (CA) took place on March 4, 2005 at 22:09.Included are data of the swingby from March 1, 2005 until March 7, 2005 andthe Passive Checkout PC0 on March 29, 2005.The current version of the dataset is V9.0.The difference to the datasets of earlier versions is mainly a significantlyimproved sensor temperature model, more detailed documentation about magneticdisturbance sources, more data handling information for the user andalso an improved quality flagging system.

Tags: __
Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 3 3316 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 2012-12-16T06:55:05.000 to 2012-12-16T09:25:45.500.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-LANDER 67P ROMAP 2 FSS MAG V1.0

This archive contains edited data from the ROMAP-MAG instrument onboard ROSETTA Lander, acquired during the FSS (First Science Sequence) phase. The primary target is the comet 67P/Churyumov-Gerasimenko. It also contains documentation which describes the ROMAP experiment. The data archived in this data set conform to the Planetary Data System (PDS) Standards, Version 3.6.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER COMET ESCORT 1 OSINAC 3 RDR MTP012 V2.0

This data set contains images acquired by the OSIRIS Narrow Angle Camera during the COMET ESCORT 1 phase of the Rosetta mission at the comet 67P, covering the period from 2015-01-13T23:25:00.000 to 2015-02-10T23:24:59.000. This version V2.0 supersedes previous deliveries of the same dataset.

Tags: __
Organization: National Aeronautics and Space Administration
Wind Solar Wind Weimer Propagation Details at 1 min Resolution

Wind Weimer propagated solar wind data and linearly interpolated time delay, cosine angle, and goodness information of propagated data at 1 min Resolution. This data set consists of propagated solar wind data that has first been propagated to a position just outside of the nominal bow shock (about 17, 0, 0 Re) and then linearly interpolated to 1 min resolution using the interp1.m function in MATLAB. The input data for this data set is a 1 min resolution processed solar wind data constructed by Dr. J.M. Weygand. The method of propagation is similar to the minimum variance technique and is outlined in Dan Weimer et al. [2003; 2004]. The basic method is to find the minimum variance direction of the magnetic field in the plane orthogonal to the mean magnetic field direction. This minimum variance direction is then dotted with the difference between final position vector minus the original position vector and the quantity is divided by the minimum variance dotted with the solar wind velocity vector, which gives the propagation time. This method does not work well for shocks and minimum variance directions with tilts greater than 70 degrees of the sun-earth line. This data set was originally constructed by Dr. J.M. Weygand for Prof. R.L. McPherron, who was the principle investigator of two National Science Foundation studies: GEM Grant ATM 02-1798 and a Space Weather Grant ATM 02-08501. These data were primarily used in superposed epoch studies References: Weimer, D. R. (2004), Correction to ‘‘Predicting interplanetary magnetic field (IMF) propagation delay times using the minimum variance technique,’’ J. Geophys. Res., 109, A12104, doi:10.1029/2004JA010691. Weimer, D.R., D.M. Ober, N.C. Maynard, M.R. Collier, D.J. McComas, N.F. Ness, C. W. Smith, and J. Watermann (2003), Predicting interplanetary magnetic field (IMF) propagation delay times using the minimum variance technique, J. Geophys. Res., 108, 1026, doi:10.1029/2002JA009405.

Tags: 1-min, bow-shock, magneticfield-ace, magnetopause, magnetotail, processed-solar-wind-data, propagation-information, propagation-support-data, solar-wind
Organization: National Aeronautics and Space Administration