AndreaBozzo/ceres-open-data-index huggingface dataset:
Wind Linearly Interpolated 60 s Resolution Tri-axial Fluxgate Magnetometer in GSM Coordinates

Wind linearly interpolated to have the measurements on the minute at 60 s resolution tri-axial fluxgate magnetometer data in GSM 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 MARS MRS 1/2/3 EXTENDED MISSION 7 4006 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 2019-05-17T06:40:49.100 to 2019-05-17T07:02:57.449.

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Organization: National Aeronautics and Space Administration
Wind SWE Linearly Interpolated 60 s Resolution data in GSM Coordinates

Wind linearly interpolated to have the measurements on the minute at 60 s resolution SWE data in GSM 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.

Tags: bow-shock, magnetopause, magnetotail, plasma-data, solar-wind, thermalplasma-1-min, wind
Organization: National Aeronautics and Space Administration
Wind SWE Linearly Interpolated 60 s Resolution data in GSE Coordinates

Wind linearly interpolated to have the measurements on the minute at 60 s resolution SWE 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.

Tags: bow-shock, magnetopause, magnetotail, plasma-data, solar-wind, thermalplasma-1-min, wind
Organization: National Aeronautics and Space Administration
GO A PWS REFORMATTED IDA SPECTRUM ANALYZER FULL V1.0

This data set includes full resolution    electric and magnetic wave spectra obtained during a ~ 15-minute period    of contiguous observations near the closest approach to Ida and a number    of non-contiguous spectra taken prior to closest approach.  In addition    waveform survey data (uncalibrated) and all instrument housekeeping data    are included.  The parameters provided for both the electric and magnetic    field spectral data are uncalibrated data numbers.  Software and    calibration tables provided as part of this data set allow for fully    calibrated data for the electric field measurements in raw data numbers,    voltage at the antenna inputs (V), electric field (V/m), electric field    spectral density (V**2/m**2/Hz), or power flux (W/m**2/Hz).  The magnetic    field measurements can be provided in units of magnetic field spectral    density (nT**2/Hz).  The sources of these data are the High Frequency    Receiver, Sweep Frequency Receiver, and Spectrum Analyzer which make up    the Low Rate Science portion of the PWS. During the included time    interval, the instrument cycled between the electric and magnetic antennas    for the Sweep Frequency Receiver and the Spectrum Analyzer.  The High    Frequency Receiver is always connected to the electric antenna.  Hence,    for the Sweep Frequency Receiver and the Spectrum Analyzer, the temporal    resolution for electric measurements is basically one spectrum per 37.33    seconds.  For the High Frequency Receiver, the time between spectra is    18.67 seconds.  Note that the lowest 14 High Frequency Receiver channels    are sampled twice per 18.67 seconds while the remaining channels are    sampled only once.  The four Spectrum Analyzer channels are each sampled    7 times in an 18.67 sec interval.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 PRELANDING 0198 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 2014-08-11T14:00:35.000 to 2014-08-11T19:20:01.000.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 3 1112 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 2015-10-19T02:56:30.000 to 2015-10-19T03:49:31.000.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RPCMAG 2 ESC1 RAW V9.0

This dataset contains EDITED RAW DATA (CODMAC LEVEL 2) 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.This applies mainly to CALIBRATED and RESAMPLED datasets. The RAW dataset,however, has been updated as well in order provide all datasets at thesame stage, although RAW data proper did not change.

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Organization: National Aeronautics and Space Administration
MARS EXPRESS ASPERA-3 RAW-CAL NTRL PARTICLE IMAGER EXT1 V1.0

This data set contains Mars Express ASPERA-3 Neutral         Particle Imager (NPI) data from launch (June 2, 2003) to the         end of mission. These data are provided in units of count         rate (counts/second).

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Organization: National Aeronautics and Space Administration
Wind 3DP Linearly Interpolated 60 s Resolution data in GSM Coordinates

Wind linearly interpolated to have the measurements on the minute at 60 s resolution 3DP data in GSM 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.

Tags: bow-shock, magnetopause, magnetotail, plasma-data, solar-wind, thermalplasma-1-min, wind
Organization: National Aeronautics and Space Administration
ULY JUPITER ENCOUNTER EPHEMERIS                                        SYS3/ECL50 COORDS. VER. 1.0

This data set contains Ulysses                                      ephemeris data near Jupiter covering                                      the dates 1992-01-25 to 1992-02-18.                                      Two slightly different versions of                                      these data are included. The first                                      (TRJ25_48.TAB), provided by the                                      Ulysses MAG team (Imperial                                      College/JPL), includes position data                                      in Sys 3 spherical, ECL50 spherical,                                      and ECL50 Cartesian coordinates. The                                      Ulysses spin axis position is also                                      provided in ECL50 spherical                                      coordinates. The second version                                      (SPK25_48.TAB), generated at the                                      PDS/PPI node (UCLA), includes Sys 3                                      spherical trajectory, plus a                                      spacecraft local time. Note that the                                      position values for these two versions                                      differ slightly. This variation is due                                      to differences in the definitions of                                      the Jovian physical constants used to                                      generate them.

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Organization: National Aeronautics and Space Administration
ISEE-3 Linearly Interpolated 60 s Resolution Solar Wind Plasma data in GSM Coordinates

ISEE-3 linearly interpolated to have the measurements on the minute at 60 s resolution solar wind plasma data in GSM 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.

Tags: bow-shock, isee-3, magnetopause, magnetotail, plasma-data, propagated-solar-wind-data, solar-wind, thermalplasma-1-min
Organization: National Aeronautics and Space Administration
ISEE 1 Fast Plasma Experiment Solar Wind Weimer Propagated 60 s Resolution Data in GSM Coordinates

ISEE-1 Weimer propagated solar wind data and linearly interpolated to have the measurements on the minute at 60 s resolution FPE 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.

Tags: bow-shock, fast-plasma-experiment, isee-1, magnetopause, magnetotail, plasma-data, solar-wind, thermalplasma-1-min
Organization: National Aeronautics and Space Administration
IMP-8 Weimer Propagation Details at 1 min Resolution

IMP-8 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-imp-8, magnetopause, magnetotail, processed-solar-wind-data, propagation-information, propagation-support-data, solar-wind
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSINAC 4 EXT3-MTP033 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 2016-08-09T23:25:00.000 to 2016-09-02T06:39:59.000. 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.

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Organization: National Aeronautics and Space Administration
LOWELL 72-IN IMAGES AND PHOTOM. OF 9P/TEMPEL 1 V1.0

This data set contains broadband R images and derived photometry of comet 9P/Tempel 1, the target of the Deep Impact mission. Data were acquired by M. Buie at the Perkins 72-inch telescope of the Lowell Observatory during 11 nights of observing from 28 September 2000 through 14 January 2001, about 8.5 to 12.5 months after the comet passed through perihelion on 2 January 2000.

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Organization: National Aeronautics and Space Administration
ISEE-3 Linearly Interpolated 60 s Resolution Tri-axial Fluxgate Magnetometer in GSE Coordinates

ISEE-3 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.

Tags: bow-shock, isee-3, magnetic-fields, magneticfield-1-min, magnetometer, magnetopause, magnetotail, solar-wind
Organization: National Aeronautics and Space Administration
ISEE 2 Fast Plasma Experiment Linearly Interpolated 60 s Resolution data in GSM Coordinates

ISEE-2 Fast Plasma Experiment linearly interpolated to have the measurements on the minute at 60 s resolution data in GSM 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.

Tags: bow-shock, isee-2, magnetopause, magnetotail, plasma-data, solar-wind, thermalplasma-1-min
Organization: National Aeronautics and Space Administration
MARS EXPRESS SUN MRS 1/2/3                                     EXTENDED MISSION 8 4364 V1.0

This is a Mars Express                                     Radio Science data set, collected                                     during the extended mission phase                                     2023-01-01 to 2023-12-31.                                     It is a Solar Conjunction                                     measurement and covers the time                                     2023-11-06T05:32:47.100 to                                     2023-11-06T09:16:35.000.

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Organization: National Aeronautics and Space Administration
DAWN FC2 DERIVED VESTA GLOBAL MOSAICS V1.0

Abstract  :  This data set includes various Vesta global mosaics derived from images  acquired by the Framing Camera 2 (FC2) on the NASA Dawn spacecraft at  the high and low altitude mapping orbits (HAMO and LAMO). Data are  provided in cylindrical and polar stereographic projections. In addition to the mosaics, the flatfield and stray light used during the processing of the raw images are provided.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 1 0545 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 2015-01-22T17:08:15.000 to 2015-01-22T23:04:32.500.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER LUTETIA OSINAC 3 AST2 RDR V2.0

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 LUTETIA FLY-BY mission phase, covering the period  from 2010-05-17T00:00:00.000 to 2010-09-03T23:59:59.000. The prime target is asteroid 21 Lutetia. 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.

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Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 7 4171 V1.0

This is a Mars Express Radio Science data set, collected during the extended mission phase 2019-01-01 to 2020-12-31. It is a Occultation measurement and covers the time 2020-12-24T09:53:06.000 to 2020-12-24T10:15:14.449.

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Organization: National Aeronautics and Space Administration
ISEE 1 Linearly Interpolated 60 s Resolution Tri-axial Fluxgate Magnetometer in GSE Coordinates

ISEE-1 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.

Tags: bow-shock, isee-1, magnetic-field, magneticfield-1-min, magnetometer, magnetopause, magnetotail, solar-wind
Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 4 3597 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 2013-07-03T00:52:27.000 to 2013-07-03T03:08:20.500.

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Organization: National Aeronautics and Space Administration
MARS EXPRESS SUN MRS 1/2/3                                     EXTENDED MISSION 8 4373 V1.0

This is a Mars Express                                     Radio Science data set, collected                                     during the extended mission phase                                     2023-01-01 to 2023-12-31.                                     It is a Solar Conjunction                                     measurement and covers the time                                     2023-11-30T01:20:11.000 to                                     2023-11-30T05:59:43.000.

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Organization: National Aeronautics and Space Administration