AndreaBozzo/ceres-open-data-index huggingface dataset:
ANTARES Baja California Station

The ANTARES regional network is composed of coastal time-series stations located around Latin America (www.antares.ws). The main goal is to study long-term changes due to both climate and anthropogenic effects, as well as for ocean color purposes of satellite match-ups and algorithm development.

Tags: earth-science-ocean-chemistry-oceans, earth-science-ocean-optics-oceans, earth-science-ocean-temperature-oceans, earth-science-salinity-density-oceans
Organization: National Aeronautics and Space Administration
DAWN VIR CAL (RDR) CRUISE CHECKOUT/CALIB VIS SPECTRA V1.0

This data set contains the spectral radiance (W/(m**2*sr*micron)) data from the Dawn VIR instrument VIS channel for all cruise mission phases. The data are from the cruise phase from launch to Vesta (Sep 2009-May 2011), and Vesta to Ceres (Sep 2012-Dec 2014).

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Organization: National Aeronautics and Space Administration
Wind Solar Wind Experiment (SWE) Electron Pitch-Angle Distributions (12-15s rate) (New Mode)

Wind SWE electron pitch angle product providing electron fluxes at 30 directional bins relative to the instantaneous magnetic field direction at 13 different energy levels from a later mode (post-VEIS-era) of the electron instrument. The electron pitch-angle distributions included in this data set are derived from sorting, by pitch (wrt B) and energy, the solar wind electron distributions measured by the Wind/SWE electron instrument (see Ogilvie et al., "SWE, a comprehensive plasma instrument for the Wind spacecraft", Space Sci. Rev., 71, 55, 1995). Pitch-angle distrubutions, organized by energy, are computed from 9s measurements which are usually separated by one or more 3s spin-periods. These quantities are reliable and citable with caution, meaning that the PI advises that the user should discuss their interpretations with a member of the SWE science team before publishing. The following comments are intended to aid in the use and interpretation of the electron pitch-angle distributions reported in this data set. For each 'energy spectrum', observations are made at 13 energy channels: E = 19.34, 38.68, 58.03, 77.37, 96.71, 116.1, 193.4, 290.1, 425.5, 580.3, 773.7, 1006., and 1238. eV. The observations made at each energy are sorted into pitch-angle bins, six degrees in width, from 0 degrees (flux nearly parallel to B) to 180 degrees (flux nearly anti-parallel with B). A "spin-averaged" set of observations (aggregated from all pitch-angle bins, each energy) is also reported, one value for each energy channel. The value reported for any bin (including the spin-averaged "energy bins") is given as a phase-space density, f [#/{cc*(cm/s)^3}], averaged over contributing detectors. The data set reported here contains: f_pitch_E00, f_pitch_E01, f_pitch_E02, f_pitch_E03, f_pitch_E04, f_pitch_E05, f_pitch_E06, f_pitch_E07, f_pitch_E08, f_pitch_E09, f_pitch_E10, f_pitch_E11, f_pitch_E12 (the pitch-angle distributions for each energy channel, with 30 pitch-angle bins for each), and f_pitch_SPA (with 13 spin-averaged energy bins). For reference, the electron speeds ( V , in cm/s) corresponding to the energy channels used, are reported in this data set.

Tags: thermalplasma
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSIWAC 4 ESC2-MTP016 RDR-REFLECT V1.0

This CODMAC level 4 data set contains radiometric calibrated and geometric distortion corrected (resampled) image data in reflectance units (normalized and thus without unit), acquired by the OSIRIS Wide Angle Camera on the Rosetta spacecraft during the COMET ESCORT 2 mission phase, covering the period from 2015-05-05T23:25:00.000 to 2015-06-02T23:24:59.000. The prime target is comet 67P/Churyumov-Gerasimenko 1 (1969 R1). This version V1.0 is the first version of this dataset: Lien corrected dataset after October 2018 PSA/PDS external peer review.

Tags: __
Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 3 3305 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 2012-06-09T07:30:56.000 to 2012-06-09T10:59:49.500.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P NAVCAM 2 PRELANDING MTP007 V1.1

This dataset contains ROSETTA NAVCAM RAW DATA of the Prelanding Phase from 2nd Sep 2014 to 23rd Sep 2014 before reaching target 67P/CG. This data set V1.1 supersedes the V1.0. It includes updates of the Browse images, adding of the FITS version, clarification of calibration target, document updates and resolve other minor outstanding errata.

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Organization: National Aeronautics and Space Administration
PHOENIX MARS MECA NON-IMAGING RDR V1.0

Phoenix MECA non-imaging reduced data records include (1) calibrated MECA TECP thermocouple, electrical conductivity, relative humidity, and relative permittivity data, (2) calibrated MECA AFM scan height and error data, and (3) reduced WCL ion-selective electrode, conductivity, chronopotentiometry, cyclic voltammetry, and pressure and temperature data.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 1 0571 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 2015-02-09T22:50:30.000 to 2015-02-10T05:11:37.000.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P NAVCAM 2 COMET ESCORT 1 MTP010 V1.1

This dataset contains ROSETTA NAVCAM RAW DATA of the Escort Phase from 21st Nov 2014 to 19th Dec 2014 when at the vicinity of target 67P/CG. This data set V1.1 supersedes the V1.0. It includes updates of the Browse images, adding of the FITS version, clarification of calibration target, document updates and resolve other minor outstanding errata.

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Organization: National Aeronautics and Space Administration
Wind SMS Suite SupraThermal Ion Composition Spectrometer (SMS/STICS) Ion Velocity Distribution Functions (VDFs), Level 2 (L2), 3-minute Data in Solar Wind

The data include Wind STICS 3-minute 3D velocity distribution functions (VDFs) in three units (phase space density, differential number flux and counts), together with their statistical errors, for selected ion species using triple coincidence (H+, He+, He2+, C5+, O+, O6+, and Fe10+) and double coincidence (H+, He+, He2+, O+, O6+) measurements in the solar wind. For details, see https://spdf.gsfc.nasa.gov/pub/data/wind/documents/wind_stics_lv2_release_notes_revD.pdf.\nThe Suprathermal Ion Composition Spectrometer (STICS) is a time of flight (TOF) plasma mass spectrometer, capable of identifying mass and mass per charge for incident ions up to 200 keV/e. It uses an electrostatic analyzer to admit ions of a particular energy per charge (E/Q) into the TOF chamber. The E/Q voltage is stepped through 32 values, sitting at each value for approximately 24 sec., to measure ions over the full E/Q range of 6 - 200 keV/e. Ions then pass through a carbon foil and TOF chamber, before finally impacting on a solid-state detector (SSD) for energy measurement. STICS combines these three measurements of E/Q, TOF and residual energy, producing PHA words. This triple-coincidence technique greatly improves the signal to noise ratio in the data. Measurements of E/Q and TOF without residual energy also produce PHA words. These double-coincidence measurements are characterized by better statistics since ions whose energy does not allow them to be registered by the SSD can still be counted in double-coincidence measurements. However, ion identification in double-coincidence measurements are limited to a select number of ions that are well separated in E/Q - TOF space.  The STICS instrument provides full 3D velocity distribution functions, through a combination of multiple telescopes and spacecraft spin. The instrument includes 3 separate TOF telescopes that view 3 separate latitude sectors, as shown in Figure 1 (https://spdf.gsfc.nasa.gov/pub/data/wind/documents/wind_stics_lv2_release_notes_revD.pdf). In addition, the WIND spacecraft spins, allowing the 3 telescopes to trace out a nearly 4π steradian viewing area. The longitudinal sectors are shown in Figure 2. The solar direction is in sectors 8-10 while the earthward direction is in sectors 0-2.

Tags: ioncomposition
Organization: National Aeronautics and Space Administration
Antares Cartagena station, Colombia

Antares Cartagena station is located 10 km offshore, across from the Cartagena Bay/Caribbean Sea at 75&deg; 36'W, 10&deg; 22'N in Cartagena, Colombia. Activities in the station are coordinated by the General Maritime Directorate for the Caribbean Oceanographic and Hydrographic Research Center (CIOH).Activities at Antares Cartagena Station started in 2008 when the CIOH joined the ANTARES monitoring network (see http://www.antares.ws/?p=station.php&st=7). The CIOH has measured in situ CTD temprature, pressure, salinity, oxygen and fluorescence. Additionally, water samples are taken at discrete depths with Niskin bottles and temperature, salinity, oxygen and pH are measured through multiparameter probe.Assays for determining chlorophyll, planktonic community analysis, determination of nutrients (nitrate, nitrite, ammonium, orthophosphates and silicates) and SST, are performed in CIOH's laboratory which is accredited under NTC ISO / IEC 17025:2001 for physic-chemical analysis of marine and estuarine waters.

Tags: earth-science-ocean-chemistry-oceans, earth-science-ocean-optics-oceans, earth-science-ocean-temperature-oceans, earth-science-salinity-density-oceans
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSIWAC 4 PRL-MTP006 RDR-REFLECT V1.0

This CODMAC level 4 data set contains radiometric calibrated and geometric distortion corrected (resampled) image data in reflectance units (normalized and thus without unit), acquired by the OSIRIS Wide Angle Camera on the Rosetta spacecraft during the PRELANDING mission phase, covering the period from 2014-08-01T10:00:00.000 to 2014-09-02T09:59:59.000. The prime target is comet 67P/Churyumov-Gerasimenko 1 (1969 R1). This version V1.0 is the first version of this dataset: Lien corrected dataset after October 2018 PSA/PDS external peer review.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 ROSETTA EXTENSION 1 1365 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 2016-01-24T01:38:35.000 to 2016-01-24T09:13:36.500.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RPCIES 2 EXT1 V1.0

This dataset contains EDITED DATA of the Rosetta RPCIES instrument taken during the Rosetta Extension 1 phase (EXT1). The target of this phase was comet 67P/CHURYUMOV-GERASIMENKO 1 (1969 R1). Included are the data taken between 01 Jan 2016 and 05 Apr 2016.

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Organization: National Aeronautics and Space Administration
LP MOON SPACECRAFT ATTITUDE V1.0

The Lunar Prospector attitude data set consists of values for the spacecraft spin rate and spin axis orientation (attitude) as a function of time. These values are determined from spacecraft attitude data (sun and limb crossing sensors) and ephemeris data. Spacecraft orientations are given as right ascension and declination of the spacecraft spin axis in the Mean-of-J2000 Ecliptic reference frame. The attitude data set consists of a single, cumulative file for the entire mission. Records are added to this file following each significant change in either the spin rate or spin axis orientation. The spacecraft spin rates and attitudes in this data set are orbit averages. The instantaneous spin rate can be determined from the sun pulse data set. The instantaneous spin rate varies as the spacecraft passes into and out of the Moon's shadow and after each spacecraft maneuver. Generally, an attitude record is included for times immediately before and after each maneuver.

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Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 3 3367 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 2012-08-16T04:22:45.000 to 2012-08-16T06:58:40.500.

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Organization: National Aeronautics and Space Administration
NEW HORIZONS  MVIC PLUTO CRUISE  RAW V1.0

This data set contains Raw data taken by the New Horizons  Multispectral Visible Imaging Camera  instrument during the  pluto cruise  mission phase. This is VERSION 1.0 of this data set.   The spacecraft was in hibernation for much of the Pluto Cruise  mission phase, and the focus for RALPH (MVIC and LEISA) during  Annual CheckOuts one through four (ACO1-4) was preparation for the  Pluto Encounter in 2015, including functional tests, and calibrations.  Science observations performed during this phase included Uranus and  Neptune at phase angles (44 degrees and 34 degrees, respectively) not  available from Earth (MVIC), calibrations with Neptune as a navigation  test target (MVIC), Sun in the Solar Illumination Assembly (SIA) (MVIC  and LEISA), the M6 and M7 clusters (MVIC), and other  calibrations (stray light, dark, interference with other instruments).

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Organization: National Aeronautics and Space Administration
ANTARES monitoring station in Ubatuba, Southeast Brazilian Bight

The ANTARES regional network is composed of coastal time-series stations located around Latin America. The main goal is to study long-term changes due to both climate and anthropogenic effects, as well as for ocean color purposes of satellite match-ups and algorithm development. The Ubatuba-ANTARES station is located in the Southeast Brazilian Bight, 12 nautical miles from the coastline, at approximately 40 m depth. Ubatuba inner shelf is influenced by mesoscale cyclonic meandering of the Brazil Current system at a region with a crosscurrent transfer of slope waters into the shelf. This ecosystem is mainly oligo-mesotrophic, but also strongly influenced by the South Atlantic Central Water upwelled locally or remotely forced from northeastern upwelling cores mainly during austral summer. In the winter, colder, less saline and relatively richer waters from southern latitudes advect northwards along the shelf.

Tags: earth-science-ocean-chemistry-oceans, earth-science-ocean-optics-oceans, earth-science-ocean-temperature-oceans, earth-science-salinity-density-oceans
Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 7 4097 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 2019-12-07T10:10:00.000 to 2019-12-07T12:05:00.000.

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Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 3 3334 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 2012-07-02T08:18:11.000 to 2012-07-02T09:56:20.500.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER CHECKOUT OSIWAC 2 CR2 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 CRUISE 2 mission phase, covering the period  from 2005-04-05T00:00:00.000 to 2006-07-28T23:59:59.000. The prime objective was commissioning / calibration. Several targets of opportunity were observed, but none of them is identifiable as prime target. 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
MGS SAMPLER MARS ORBITER CAMERA IMAGES

Mars Orbiter Camera (MOC) data  products on this volume are nine Narrow Angle Camera images  selected from orbits between 13 and 100; i.e., some images are  from outside the Assessment Orbits range of 19-36. The images  are in GIF format with detached PDS labels, and they have had  some cosmetic corrections applied (see VOLINFO for description).  As the images are large, reduced-size versions have also been  included for browsing. To assist in locating the images on the  planet, 'finder frames' have been provided; these are Viking  Orbiter MDIMs showing the outlines of the MOC images in the  context of the larger area. The locations of the MOC images  are also shown on the Mercator and South Polar Stereographic  orbit ground track maps below. (Note: MOC image files are named  according to the form NAnnnnxx, where nnnn is the orbit number  and xx is the image number within the orbit.)

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Organization: National Aeronautics and Space Administration
Wind Solar Wind Experiment (SWE) Averaged Electron Pitch Angle Distribution (12-15s rate)

Averaged Wind SWE electron pitch angle data (12-15 seconds rate) from a later mode (post-VEIS-era) of the electron instrument. The electron pitch-angle distribution averages included in this data set are derived from integrating the electron pitch-angle distributions measured by the Wind/SWE electron instrument (see Ogilvie et al., "SWE, a comprehensive plasma instrument for the Wind spacecraft", Space Sci. Rev., 71, 55, 1995). Averages of phase-space density (f) over key regions of the unit sphere (the set of all possible electron velocity directions) are computed from 9s measurements which are usually separated by one or more 3s spin-periods. These quantities are reliable and citable with caution, meaning that the PI advises that the user should discuss their interpretations with a member of the SWE science team before publishing. The following comments are intended to aid in the use and interpretation of the averages reported in this data set. We begin this analysis with a measure of f for each pitch-angle bin, six degrees in width, from 0 degrees (flux nearly parallel to B) to 180 degrees (flux nearly anti-parallel with B). The f values for pitch-angles from 0-90 degrees (parallel streaming) are integrated (with angluar weighting and assumptions of gyrotropy) over this half-sphere, then averaged by dividing out the 2-pi solid angle of the half-sphere; the result being referred to as the 'f_para' average. Similarly, the 'f_perp' (flux nearly perpendicular to B) average is the result of integrating f for pitch-angles from 60-120 degrees (a region also 2-pi in solid angle). Next, the 'f_anti' (flux nearly anti-parallel to B) average covers the half-sphere of "backward" streaming electrons; having pitch-angles from 90-180 degrees. Finally, the 'f_omni' (omni-directional) average provides the integral of f over the full sphere, divided by the full 4-pi solid angle; providing a measure of total electron flux into the region of observation. The above analysis is carried out for each of 13 energy channels: E = 19.34, 38.68, 58.03, 77.37, 96.71, 116.1, 193.4, 290.1, 425.5, 580.3, 773.7, 1006., and 1238. eV. For reference, the electron speeds ( V , in cm/s) corresponding to these energies are reported in this data set. Hence the data set reported here contains: f_para, f_perp, f_anti, f_omni (for each of 13 values of E), and the 13 values of V (constant, included for reference).

Tags: thermalplasma
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER EARTH RPCMAG 4 EAR2 RESAMPLED V9.0

This dataset contains RESAMPLED DATA (CODMAC LEVEL 4) of the SECOND EARTHSWINGBY (EAR2) of the ROSETTA orbiter magnetometer RPCMAG.The closest approach (CA) took place on November 13, 2007 at 20:57.Included are data of the Active Checkout 6 in September 2007 and the PassiveCheckout PC7 in January 2008.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.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSINAC 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 Narrow 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 0852 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 2015-06-21T21:02:00.000 to 2015-06-21T22:40:07.500.

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Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3                                     EXTENDED MISSION 9 4414 V1.0

This is a Mars Express                                     Radio Science data set, collected                                     during the extended mission phase                                     2023-01-01 to 2026-12-31.                                     It is a Occultation                                     measurement and covers the time                                     2024-02-24T22:36:29.300 to                                     2024-02-24T22:58:37.300.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER/ROSETTA-LANDER CAL CONSERT 2 EAR3 V2.0

This archive contains edited data that refers to target earth (CODMAC level 2) from the CONSERT instrument onboard ROSETTA Orbiter and Lander, acquired during the EAR3 mission phase (Earth swing-by 3). It also contains documentation which describes the CONSERT experiment. The data archived in this data set conform to the Planetary Data System (PDS) Standards, Version 3.6. This data set supersedes RO/RL-E-CONSERT-2-EAR3-V1.0.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P NAVCAM 2 COMET ESCORT 4 MTP024 V1.0

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.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSINAC 4 ESC2-MTP016 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 COMET ESCORT 2 mission phase, covering the period from 2015-05-05T23:25:00.000 to 2015-06-02T23:24:59.000. The prime target is comet 67P/Churyumov-Gerasimenko 1 (1969 R1). This version V1.0 is the first version of this dataset: Lien corrected dataset after October 2018 PSA/PDS external peer review.

Tags: __
Organization: National Aeronautics and Space Administration