AndreaBozzo/ceres-open-data-index huggingface dataset:
ATom: Nucleation Mode Aerosol Size Spectrometer Calibration and Performance Data

This dataset provides extensive calibration and in-flight performance data for two nucleation mode aerosol size spectrometer (NMASS) instruments utilized in the NASA Atmospheric Tomography Mission (ATom). Each NMASS has five condensation particle counters (CPCs) that detect particles above a different minimum size, determined by the maximum vapor supersaturation encountered by the particles. Operated in parallel, the CPCs provide continuous concentrations of particles in different cumulative size classes between 3 and 60 nm. Knowing the response function of each CPC, numerical inversion techniques were applied to recover size distributions from the continuous concentrations. Data provided include: NMASS counting efficiencies and diameters of calibration aerosols, inverted particle size distributions; comparisons of NMASS and Scanning Mobility Particle Sizer (SMPS) results; and performance at flows, temperatures, and pressures measured by both NMASSs and comparison with Ultra-High Sensitivity Aerosol Spectrometer (UHSAS) concentrations collected on board the NASA DC-8 aircraft during an ATom flight in February 2017.

Tags: earth-science-aerosols-atmosphere-aerosol-particle-properties, earth-science-aerosols-atmosphere-organic-particles, earth-science-aerosols-atmosphere-sulfate-particles, earth-science-air-quality-atmosphere-emissions, earth-science-air-quality-atmosphere-particulates, earth-science-atmospheric-chemistry-atmosphere-carbon-and-hydrocarbon-compounds
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P NAVCAM 2 COMET ESCORT 4 MTP024 V1.1

This dataset contains ROSETTA NAVCAM RAW DATA of the Escort Phase 4 from 15th Dec 2015 to 12th Jan 2016 when at the vicinity of target 67P/CG. This data set V1.1 supersedes the V1.0. It includes updates of the Browse images, clarification of calibration target, document updates and resolve other minor outstanding errata.

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Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 6 3927 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 2018-03-21T08:06:08.000 to 2018-03-21T08:36:06.949.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 1 0565 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 2015-02-05T22:57:10.000 to 2015-02-06T08:54:06.500.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P VIRTIS 2 PRELANDING MTP009 V2.0

This release contains the digital numbers (DN) contained in the telemetry (TM) packages of the VIRTIS instrument on board of the spacecraft Rosetta. This volume contains data at the vicinity of comet 67P, from the PRELANDING MTP009 phase, which occurred from 2014-10-24 to 2014-11-22. This version of the dataset (2.0) is produced by a fixed EGSE software. The old version of the software produced incomplete products, reduced by one line

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSIWAC 4 ESC4-MTP023 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 4 mission phase, covering the period from 2015-11-17T23:25:00.000 to 2015-12-15T23:24:59.000. The prime target is comet 67P/Churyumov-Gerasimenko 1 (1969 R1). This version V1.0 is the first version of this dataset: Lien corrected dataset after October 2018 PSA/PDS external peer review.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 2 0677 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 2015-03-28T01:59:30.000 to 2015-03-28T06:39:10.000.

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Organization: National Aeronautics and Space Administration
ATom: Global Modeled and CAFS Measured Cloudy and Clear Sky Photolysis Rates, 2016

This dataset provides the results from nine global chemistry-climate or chemistry-transport models that estimated gridded values of atmospheric photolytic rates (J values) for ozone (O3), designated J-O1D, and nitrogen dioxide (NO2), designated J-NO2, under cloudy and clear sky scenarios. Each model produced global 4-D fields (latitude by longitude by pressure for 24 hours) for one day in mid-August 2016 (nominally) of results from two simulations: first using their standard treatment of clouds (all sky or cloudy) and a second with clouds and aerosols removed (clear sky). Model resolution ranges from 0.5 to 2.5 degrees. Observed J-O1D and J-NO2 values from the first ATom deployment (29 July - 23 August 2016) were collected with the Charged-coupled device Actinic Flux Spectroradiometer (CAFS) instrument. The ATom CAFS measurements are 3-second averages along the flight path for selected remote areas over the tropical and northern Pacific Ocean. Both all-sky (cloudy) and synthesized clear-sky J values are provided. (3) Additional data are included for clouds and ozone column plus other cloudy and clear sky parameters for the same remote areas of the tropical and northern Pacific Ocean. These auxiliary data are provided for use with included MATLAB scripts to reproduce the plots and analyses performed in the related publication by Hall et al. (2018). Note that while the analyses in the related publication were limited to the Pacific basin, the global model data are archived with this dataset.

Tags: earth-science-atmospheric-chemistry-atmosphere-nitrogen-compounds-nitrogen-dioxide, earth-science-atmospheric-chemistry-atmosphere-oxygen-compounds-atmospheric-ozone, earth-science-atmospheric-chemistry-atmosphere-photochemistry-photolysis-rates, earth-science-atmospheric-chemistry-atmosphere-trace-gases-trace-species, earth-science-clouds-atmosphere-cloud-dynamics
Organization: National Aeronautics and Space Administration
DEEP IMPACT 9P/TEMPEL ENCOUNTER - REDUCED ITS IMAGES V3.0

This dataset contains calibrated images of comet 9P/Tempel 1 acquired by the Impactor Targeting Sensor Visible CCD (ITS) after the impactor was released from the flyby spacecraft on 03 July 2005 during the Deep Impact mission. Version 3.0 was calibrated by the EPOXI mission pipeline and includes corrected observation times with a maximum difference of about 40 milliseconds, a change to decompress the camera's zero-DN lookup table entry to the top of its range and flag the affected pixels as saturated, and the replacement of the I-over-F data products by multiplicative constants for converting radiance products to I-over-F.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 1 0576 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 2015-02-12T08:54:45.000 to 2015-02-12T10:45:07.500.

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

ACE linearly interpolated to have the measurements on the minute at 60 s resolution SWEPAM 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: ace, advanced-composition-explorer, plasma-data, solar-wind, swepam, thermalplasma-1-min
Organization: National Aeronautics and Space Administration
ICE RADIO WAVE ELECTRON MAPPING DATA V1.0

The data are presented as the values of the density and temperature of the electrons measured (radio mapping) during the tail crossing of comet Giacobini-Zinner by ISEE-3/ICE as derived from spectroscopy of the thermal noise spectrum. The data was provided to the National Space Science Data Center (NASA/GSFC) by the Principal Investigator of the Radio Mapping Experiment on ISEE-3/ICE, Dr. Jean-Louis Steinberg of the Observatoire de Paris, Meudon, France cover the time interval 10:00 - 12:00 UT on September 11, 1985. The time resolution is 54 seconds.

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Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 3 3288 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 2012-05-15T13:09:18.000 to 2012-05-15T15:33:18.500.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSIWAC 4 PRL-MTP001 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 PRELANDING mission phase, covering the period from 2014-01-20T10:00:00.000 to 2014-05-07T12:47:59.000. 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
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 4 3584 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 2013-06-04T05:33:54.000 to 2013-06-04T07:20:00.500.

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Organization: National Aeronautics and Space Administration
EPOXI INFLIGHT CALIBRATIONS - MRI RAW IMAGES V2.0

This dataset contains raw calibration images acquired by the Medium Resolution Visible CCD (MRI) from 04 October 2007 through 28 November 2010 during the EPOCh, 103P/Hartley 2 Encounter, and cruise phases of the EPOXI mission.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 PRELANDING 0424 V1.0

This is a Rosetta Radio Science data set, collected during the PRELANDING phase 2014-01-21 to 2014-11-19. It is a Global Gravity measurement at the comet 67P and covers the time 2014-11-12T07:00:45.000 to 2014-11-12T11:04:59.000.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 3 0926 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 2015-07-28T21:24:50.000 to 2015-07-29T00:24:27.000.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 4 1144 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 2015-10-31T04:58:35.000 to 2015-10-31T08:21:19.000.

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Organization: National Aeronautics and Space Administration
NEW HORIZONS REX JUPITER ENCOUNTER CALIBRATED V1.0

This data set contains Calibrated data taken by the New Horizons Radio Science Experiment instrument during the Jupiter encounter mission phase. This is VERSION 1.0 of this data set. The REX datasets over the mission include calibrations using known radio sources, Jupiter, and cold sky measurements; operational readiness tests (ORTs); internal test pattern calibration; and prime science radiometry and occultation observations during the Pluto Encounter.

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Organization: National Aeronautics and Space Administration
ACE Weimer Propagated 60 s Resolution Tri-axial Fluxgate Magnetometer in GSE Coordinates

ACE Weimer propagated solar wind data and 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 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: ace, advanced-composition-explorer, magnetic-field, magneticfield-1-min, magnetometer, propagated-solar-wind-data, solar-wind
Organization: National Aeronautics and Space Administration
CASSINI V/E/J/S/SS RPWS EDITED WIDEBAND FULL RES V1.0

The Cassini Radio and Plasma Wave Science (RPWS) edited full      resolution data set includes all wideband waveform data for the      entire Cassini mission.  This data set includes uncalibrated      values for each wideband channel for each sensor for all times      during the mission including the second Venus flyby, the Earth      flyby, the Jupiter flyby, interplanetary cruise, and the entire      Saturn tour.  Data for this data set are acquired from the RPWS      Wideband Receiver (WBR).  Data are presented in a set of time      series organized so as to have fixed-length records for ease in      data handling.  Data from the different WBR modes (i.e. 10-kHz,      80-kHz, and frequency-translated 80-kHz data)  are segregated into      separate files.  This data set includes all wideband data acquired      by the RPWS.  A browse data set is included with these data which      provides for a graphical search of the data using a series of      thumbnail and full-sized spectrograms which lead the user to the      particular data file(s) of interest. The wideband data provide the      highest resolution data from the RPWS instrument in the form of a      set of waveform series.  These data can be used in their original      time domain in order to look for solitary features such as dust      impacts or electrostatic solitary waves.  Or, they can be      transformed into the frequency domain in order to examine the      detailed time and spectral evolution of plasma waves or radio      emissions.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 PRELANDING 0265 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 2014-09-01T18:04:30.000 to 2014-09-02T00:29:34.000.

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Organization: National Aeronautics and Space Administration
STARDUST DFMI WILD 2 ENCOUNTER EDR DATA

This data set contains raw data collected by the Dust Flux Monitor Instrument (DFMI) flown on board the STARDUST spacecraft during the Wild 2 comet encounter on January 2, 2004. The data in this archive are organized into one table in standard PDS format. This table records dust events which resulted from the encounter with the particles surrounding comet Wild 2. The data in the table spans a 33 minute period surrounding the encounter with Wild 2.

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Organization: National Aeronautics and Space Administration
Geotail Linearly Interpolated 60 s Resolution Coordinates Comprehensive Plasma Instrumentation (CPI) data in GSE

Geotail linearly interpolated to have the measurements on the minute at 60 s resolution CPI 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, cpi, geotail, magnetopause, magnetotail, plasma-data, solar-wind, thermalplasma-1-min
Organization: National Aeronautics and Space Administration
ACE Weimer Propagated 60 s Resolution Tri-axial Fluxgate Magnetometer in GSM Coordinates

ACE Weimer propagated solar wind data and 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 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: ace, advanced-composition-explorer, magnetic-field, magneticfield-1-min, magnetometer, propagated-solar-wind-data, solar-wind
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 PRELANDING 0437 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 2014-11-16T14:32:20.000 to 2014-11-17T02:48:31.000.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSINAC 5 ESC3-MTP019 DDR-GEO V1.0

This CODMAC level 5 data set contains derived data products that include pixel-precise georeferencing information, acquired by the OSIRIS Narrow Angle Camera on the Rosetta spacecraft during the COMET ESCORT 3 mission phase, covering the period from 2015-07-28T23:25:00.000 to 2015-08-25T23:24:59.000. The prime target is comet 67P/Churyumov-Gerasimenko 1 (1969 R1). This version V1.0 is the first version of this dataset: Lien corrected dataset after October 2018 PSA/PDS external peer review.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 PRELANDING 0215 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 2014-08-17T10:00:45.000 to 2014-08-17T11:44:18.000.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P VIRTIS 3 PRELANDING MTP009 V2.0

This release contains the calibrated data of the VIRTIS instrument on board of the spacecraft Rosetta. This volume contains data from the PRELANDING MTP009 phase, which occurred from 2014-10-24 to 2014-11-22 when at the vicinity of comet 67P. This data set V2.0 supersedes V1.0. It includes major updates on the data and documentation.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 ROSETTA EXTENSION 1 1383 V1.0

This is a Rosetta Radio Science data set, collected during the ROSETTA EXTENSION 1 phase 2016-01-01 to 2016-04-05. It is a Global Gravity measurement at the comet 67P and covers the time 2016-01-30T09:18:20.000 to 2016-01-30T13:08:18.000.

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Organization: National Aeronautics and Space Administration
DAWN VIR RAW (EDR) VESTA INFRARED SPECTRA V2.0

This data set contains the raw  infrared channel digital numbers (DN) contained in the telemetry  packages taken by the Dawn VIR spectrometer for all Vesta encounter  mission phaes. The data in this version of the data set include  minor updates to the data files and labels. The data cover the time  period between 2011-05-03 and 2012-07-18.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 ROSETTA EXTENSION 1 1431 V1.0

This is a Rosetta Radio Science data set, collected during the ROSETTA EXTENSION 1 phase 2016-01-01 to 2016-04-05. It is a Global Gravity measurement at the comet 67P and covers the time 2016-02-19T02:26:15.000 to 2016-02-19T11:29:34.000.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSINAC 4 PRL-MTP005 RDR V1.0

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 Narrow Angle Camera during the PRELANDING phase of the Rosetta mission, covering the period from 2014-07-02T08:35:00.000 to 2014-08-01T09:59:59.000.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 4 1133 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 2015-10-27T10:24:15.000 to 2015-10-27T14:11:30.000.

Tags: __
Organization: National Aeronautics and Space Administration