AndreaBozzo/ceres-open-data-index huggingface dataset:
ROSETTA-ORBITER CAL RPCMIP 3 CR5 V1.0

This archive contains data from the RPC-MIP instrument onboard ROSETTA Orbiter acquired during the CRUISE 5 mission phase. It also contains documentation which describes the RPC-MIP experiment. The data archived in this data set conform to the Planetary Data System Standards, Version 3.6.

Tags: __
Organization: National Aeronautics and Space Administration
STEREO-A In-Situ Measurements of Particles and CME Transients (IMPACT) Fluxgate Magnetometer (MAG) Magnetic Field Vectors, in Radial-Tangential-Normal (RTN) Coordinates, Level Beacon (LB), PT0.125S Data

STEREO Ahead reprocessed IMPACT/MAG Beacon magnetic field vector component and vector magnitude data expressed in Heliographic, HG, Radial-Tangential-Normal, RTN, Cartesian coordinates around the 2015 solar conjunction. * Version 1: Used internally at UCB and UCLA ONLY, No corrections applied to raw MAG data * Version 2: Offset correction applied to MAG data * Version 3: Initial algorithm for correcting glitches for the X sensor on STEREO Ahead applied * Version 4: Improvement in glitch correction algorithm applied * Version 5: Further refinement of the glitch correction for the X sensor on STEREO Ahead, Also, two timing issues resolved: - a) applying a 6 ms time shift to account for time lag between IMPACT IDPU and MAG - b) fixing an occasional 1 s 'glitch' * Version 6: Added FILTER_VALUE variable

Tags: magneticfield
Organization: National Aeronautics and Space Administration
ACE Electron Proton Alpha Monitor (EPAM) LEMS120 MFSA, Spacecraft Frame, Sectored Proton Fluxes, Daily Averages

Daily-averaged sectored proton fluxes from the MF Spectrum Analyzer of the ACE/EPAM LEMS120 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the spacecraft rest frame.

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
ACE Electron Proton Alpha Monitor (EPAM) LEMS120 MFSA, Spacecraft Frame, Sectored Z>1 Ion Fluxes, 17 min Averages

17-min-averaged sectored Z>1 ion fluxes from the MF Spectrum Analyzer of the ACE/EPAM LEMS120 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the spacecraft rest frame.

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
STEREO-A Plasma and Supra-Thermal Ion Composition (PLASTIC) He+ Hourly Phase Space Densities

STEREO-A Plasma and Supra-Thermal Ion Composition, PLASTIC, He+ Phase Space Density, PSD, binned by V/Vsw, Level 3, Hourly Resolution Data

Tags: energeticparticles, thermalplasma
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P NAVCAM 2 PRELANDING MTP004 V1.1

This dataset contains ROSETTA NAVCAM RAW DATA of the Prelanding Phase from 4th June 2014 to 2nd July 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.

Tags: __
Organization: National Aeronautics and Space Administration
ACE Electron Proton Alpha Monitor (EPAM) LEMS120 MFSA, Spacecraft Frame, Sectored Proton Fluxes, Hourly Averages

Hourly-averaged sectored proton fluxes from the MF Spectrum Analyzer of the ACE/EPAM LEMS120 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the spacecraft rest frame.

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
STEREO-A Plasma and Supra-Thermal Ion Composition (PLASTIC) He+ Daily Phase Space Densities

STEREO-A Plasma and Supra-Thermal Ion Composition, PLASTIC, He+ Phase Space Density, PSD, binned by V/Vsw, Level 3, Daily Resolution Data

Tags: energeticparticles, thermalplasma
Organization: National Aeronautics and Space Administration
ACE Electron Proton Alpha Monitor (EPAM) LEMS30 MFSA, Solar Wind Frame, Sectored Z>1 Ion Fluxes, Hourly Averages

Hourly-averaged sectored Z>1 ion fluxes from the MF Spectrum Analyzer of the ACE/EPAM LEMS30 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the solar wind rest frame.

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
ACE Electron Proton Alpha Monitor (EPAM) LEMS30 MFSA, Solar Wind Frame, Sectored Proton Fluxes, Daily Averages

Daily-averaged sectored proton fluxes from the MF Spectrum Analyzer of the ACE/EPAM LEMS30 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the solar wind rest frame.

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
ACE Electron Proton Alpha Monitor (EPAM) CA60-W Channels, Spacecraft Frame, Sectored Ion Count Rates, Hourly Averages

Hourly-averaged sectored count rates from CA60 - Channels W1, W2, W3, W4, W5, W6, W7, and W8.

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
STEREO-A Plasma and Suprathermal Ion Composition (PLASTIC) 1-min Proton Plasma Parameters

This data product contains 1-minute values of solar wind proton flow speed, density, and temperature and corresponding thermal speed. The records also hold flow velocity vector components and direction angles in HERTN and RTN coordinates. Chi-squared and statistical uncertainties are included, as are various flags. STEREO position information is given in radial distance and HEE, HEEQ and HCI direction angles.

Tags: thermalplasma
Organization: National Aeronautics and Space Administration
SDO/AIA 171 Angstrom FITS Data

The SDO/AIA 171 Å Level 1 FITS Data .The 171 Å channel observes the Fe ix line from quiet corona and upper transition region (0.63 MK).\n\nThe Atmospheric Imaging Assembly (AIA) onboard Solar Dynamics Observatory (SDO) focuses on the evolution of the magnetic environment in the Sun’s atmosphere, and its interaction with embedded and surrounding plasma. The AIA investigation covers a broad range of science objectives that focus on five core research themes that both advance solar and heliospheric physics in general and provide advanced warning of coronal and inner-heliospheric disturbances of interest to the Living With a Star (LWS) program, i.e., global change, space weather, human exploration of space, and technological infrastructure in space and on Earth.\n\nAIA provides the following essential capabilities: i) A view of the entire Sun in 4k x 4k resolution (pixel size of 0.6 arcseconds), with full thermal coverage of the corona; ii) A high signal-to-noise ratio for two- to three-second exposures that reaches 100 in quiescent conditions for the low-temperature coronal-imaging channels and during flaring in the higher-temperature channels, with a dynamic range of up to 10,000; iii) Essentially uninterrupted viewing for months at a temporal cadence of 12 seconds in seven extreme UV (EUV) band passes (94, 131, 171, 193, 211, 304 and 335 Å), and 24 seconds for two UV channels (1600 and 1700 Å) band passes; iv) In special observing modes, AIA can capture images of the Sun at higher cadence while keeping within the instrument allocated telemetry by using a subset of bandpass channels, and/or using a crop table.

Tags: imageintensity
Organization: National Aeronautics and Space Administration
VO1/VO2 MARS IRTM BINNED DATA AND DERIVED CLOUDS V1.0

This data set, derived from the Viking Orbiter Infrared Thermal Mapper (IRTM) data set, has been binned in both space and time. It consists of two complementary portions, water ice cloud observations and surface observations. For details on the IRTM instrument and data set, refer to [KIEFFER_ETAL_1977].

Tags: __
Organization: National Aeronautics and Space Administration
ACE Electron Proton Alpha Monitor (EPAM) LEMS30 MFSA, Solar Wind Frame, Sectored Proton Fluxes, Hourly Averages

Hourly-averaged sectored proton fluxes from the MF Spectrum Analyzer of the ACE/EPAM LEMS30 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the solar wind rest frame.

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER EARTH/CAL NAVCAM 2 EARTH SWING-BY 2 V1.1

This dataset contains ROSETTA NAVCAM RAW DATA of the Cruise Phase EAR2 from 16th Sep 2007 to 22nd Jan 2008 during the 2nd Earth Fly By on its journey to comet 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.

Tags: __
Organization: National Aeronautics and Space Administration
SOHO UVCS Data

The primary scientific goals of the UVCS (UltraViolet Coronagraph Spectrometer) are to: (1) locate and characterize the coronal source regions of the solar wind; (2) identify and understand the dominant physical processes that accelerate the solar wind; (3) understand how the coronal plasma is heated in solar wind acceleration regions; and, (4) increase our knowledge of the coronal phenomena that control the physical properties of the solar wind as determined by in situ measurements. The UVCS is intended to determine the primary plasma parameters of the solar corona from its base to as high as 10 Re. It is expected to measure signatures of both thermal and nonthermal processes: electron temperatures, effective temperatures of protons and several minor ions; electron and ion densities of O+5, Mg+9, Si+11, and Fe+11; and flow velocities of the electron/proton plasma and of O+5, Mg+9, and Si+11. The instrument consists of an occulted telescope and a high resolution spectrometer assembly. Three off-axis telescope mirrors focus co-registered images of the extended corona onto the three entrance slits of the spectrometer assembly. The spectrometer assembly consists of three sections. One is optimized for line profile measurements of H I Lyman alpha, with a range of 114.8--128.3 nm, extendable to 113.0 nm and 130.0 nm with grating motions. A second section is optimized for line intensity measurements of O VII (103.2 nm) and is also used to observe Si XII in second order (499 and 521 nm; first order range is 93.2--106.8 nm). The third section is used to measure polarized radiance of the visible corona. A filter with a bandpass of 450.0--600.0 nm is mounted in front of a photomultiplier tube. The EUV spectrometer sections use toroidal concave diffraction gratings in Rowland circle mounts that produce stigmatic imaging at the subject wavelengths. There are entrance slit changing mechanisms on each spectrometer. The detectors for the EUV are multi-anode microchannel arrays, each with 360 x 1024 pixels on 0.025 mm centers. The instantaneous field of view (FOV) of the instrument is the portion of the solar image that passes through the spectrometer entrance slits. Internal mirror motions are used to step the instantaneous FOV across the 141' x 40' FOV defined by the entrance aperture. Offset pointing adjustments can be used to extend the FOV for EUV measurements down to the solar limb, and also onto the solar disk for measurements of absolute spectral line intensities and positions. The UVCS can rotate its FOV about the sun-center to observe any segment of the corona within 10 solar radii. Twelve rotations of 30 degrees would build up a spectroscopic description of the full corona out to 5 solar radii, with additional data out to 10 solar radii. This information was taken from the article ``UVCS - the Ultraviolet Coronagraph Spectrometer for SOHO,'' by J. L. Kohl and G. Noci (Proceedings of the First SOHO Workshop, ESA SP-348, pp. 23-26, November 1992).

Tags: imageintensity
Organization: National Aeronautics and Space Administration
ACE Electron Proton Alpha Monitor (EPAM) LEMS30 MFSA, Solar Wind Frame, Sectored Z>1 Ion Fluxes, Daily Averages

Daily-averaged sectored Z>1 ion fluxes from the MF Spectrum Analyzer of the ACE/EPAM LEMS30 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the solar wind rest frame.

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 PRELANDING 0306 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 2014-09-20T16:50:05.000 to 2014-09-21T00:27:41.000.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 3 0952 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 2015-08-09T10:11:20.000 to 2015-08-09T17:26:15.000.

Tags: __
Organization: National Aeronautics and Space Administration
STEREO SECCHI Cor2 telescopes P0 FITS files

Percent Polarized data from STEREO SECCHI, Sun Earth Connection Coronal and Heliospheric Investigation, Cor2 telescopes at 1 hr cadence (except for special observing campaigns) and full resolution (2048²). The data are generally available within about three days.

Tags: imageintensity
Organization: National Aeronautics and Space Administration
ACE Electron Proton Alpha Monitor (EPAM) LEMS30 MFSA, Spacecraft Frame, Sectored Z>1 Ion Fluxes, Hourly Averages

Hourly-averaged sectored Z>1 ion fluxes from the MF Spectrum Analyzer of the ACE/EPAM LEMS30 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the spacecraft rest frame.

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
MARS EXPRESS ASPERA-3 RAW EDR ELECTRON SPECTROMTR EXT6 V1.0

This data set contains Mars Express ASPERA-3 Electron         Spectrometer (ELS) data for the sixth mission extension         (January 1, 2017 - Dec. 31, 2018). These data are provided         in raw units of counts/accumulation.

Tags: __
Organization: National Aeronautics and Space Administration
STEREO-A/SECCHI/Cor1 FITS data

The COR1 telescope is the inner coronagraph of the Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI) instrument suite aboard the twin Solar Terrestrial Relations Observatory (STEREO) spacecraft. Like all coronagraphs, COR1 is designed to measure the weak light from the solar corona in the presence of scattered light from the much brighter solar photosphere. It designed to observe the white light corona from 1.4 to 4 solar radii.

Tags: imageintensity
Organization: National Aeronautics and Space Administration
ACE Electron Proton Alpha Monitor (EPAM) LEFS/LEMS MFSA, Spacecraft Frame, Spin-Averaged Z>1 Ion Fluxes, Hourly Averages

Hourly-averaged ion fluxes from the MF Spectrum Analyzer of the ACE/EPAM instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the spacecraft rest frame.

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
STEREO-A In-Situ Measurements of Particles and CME Transients (IMPACT) Fluxgate Magnetometer (MAG) Burst Mode, Magnetic Field Vector, Spacecraft (SC) Coordinates, Level 1 (L1), 31 ms Data

This data product contains Level 1 0.03125-s or 32 Hz burst-mode values of solar wind magnetic field data measured by the IMPACT Magnetometer on STEREO-A in Spacecraft, SC, coordinates.

Tags: instrumentstatus, magneticfield
Organization: National Aeronautics and Space Administration
CAMEX-4 LIDAR ATMOSPHERIC SENSING EXPERIMENT (LASE) V1

The CAMEX-4 LIDAR Atmospheric Sensing Experiment (LASE) dataset was collected by the LASE instrument, which is an airborne DIAL (Differential Absorption Lidar) system used to measure water vapor, aerosols, and clouds throughout the troposphere. LASE operates by locking to a strong water vapor line and electronically tuning to any spectral position on the absorption line to choose the suitable absorption cross-section for optimum measurements over a range of water vapor concentrations in the atmosphere. During CAMEX-4, LASE operated from the NASA DC-8 using strong and weak water vapor lines in both the nadir and zenith modes, thereby simultaneously acquiring data below and above the aircraft.

Tags: earth-science-aerosols-atmosphere-aerosol-backscatter, earth-science-atmospheric-water-vapor-atmosphere-water-vapor-indicators-water-vapor, earth-science-atmospheric-water-vapor-atmosphere-water-vapor-profiles
Organization: National Aeronautics and Space Administration
CALIPSO Lidar Level 1B profile data, V4-51

CAL_LID_L1-Standard-V4-51 is the Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observation (CALIPSO) Lidar Level 1B profile data, Version 4-51 data product. This data product was collected using the Cloud-Aerosol Lidar with Orthogonal Polarization (CALIOP) instrument. The CALIOP Level 1B data product contains a half orbit (day or night) of calibrated and geolocated single-shot (highest resolution) lidar profiles, including 532 nm and 1064 nm attenuated backscatter and depolarization ratio at 532 nm. The product released contains data from nominal science mode measurements.

Tags: earth-science-lidar-spectral-engineering, earth-science-lidar-spectral-engineering-lidar-backscatter, earth-science-lidar-spectral-engineering-lidar-depolarization-ratio
Organization: National Aeronautics and Space Administration
NEW HORIZONS  LORRI POST-LAUNCH CHECKOUT  RAW V3.0

This data set contains Raw data taken by the New Horizons  Long Range Reconnaissance Imager  instrument during the  post-launch checkout  mission phase. This is VERSION 3.0 of this data set.   During the Launch Phase, LORRI conducted a variety of instrument  commissioning activities in preparation for science operations. An  extensive series of bias images was collected during the spring  and summer of 2006, before the LORRI aperture door was opened.  Images were also collected of LORRI's internal lamps. The LORRI  aperture door was opened on 2006 August 29, and an extensive  series of calibration observations of stars in the open cluster M7  was performed during the next several days. Commissioning test  observations were also performed on the planetary targets Jupiter,  Uranus, Neptune, and Pluto. The Jovian observations were conducted  specifically to test LORRI's ability to perform imaging using  exposure times that were short compared to the frame transfer time  (i.e., shorter than 13 ms). Some histogram-only solar scattered  light observations were performed during a Ralph commissioning  test.   LORRI V3.0 provides a few updates from LORRI V2.0. The lossy images  were recalibrated, including expanding the 'bad' pixel designation  of 8x8 boxes affected by the first 34 pixels of header information  in the calibrated quality map. Also, updates were made to the  documentation and catalog files, primarily to resolve liens from the  V2.0 peer review. No new observations were added with Version 3.0.

Tags: __
Organization: National Aeronautics and Space Administration
CALIPSO Imaging Infrared Radiometer (IIR) Level 1B Radiance, Standard V2-01

CAL_IIR_L1-Standard-V2-01 is the Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observations (CALIPSO) Imaging Infrared Radiometer (IIR) Level 1B Radiance, Standard Version 2-01 data product. Data for this product was collected using the CALIPSO IIR instrument. Data collection for this product is ongoing. The IIR Level 1B data product contains a half orbit of geolocated, calibrated radiances. Image data are registered to a 1 km grid centered on the lidar track. The Level 1B data product is written in HDF. The version of this product was changed from 2-00 to 2-01 to account for a change in the operating system of the CALIPSO production cluster. CALIPSO was launched on April 28, 2006 to study the impact of clouds and aerosols on the Earth's radiation budget and climate. It flies in the international A-Train constellation for coincident Earth observations. The CALIPSO satellite comprises three instruments, Cloud-Aerosol LIdar with Orthogonal Polarization (CALIOP), IIR, and Wide Field Camera (WFC). CALIPSO is a joint satellite mission between NASA and the French Agency, CNES.

Tags: earth-science-infrared-wavelengths-spectral-engineering-infrared-radiance
Organization: National Aeronautics and Space Administration
ACE Electron Proton Alpha Monitor (EPAM) LEFS/LEMS MFSA, Solar Wind Frame, Spin-Averaged Z>1 Ion Fluxes, 17 min Averages

17-min-averaged ion fluxes from the MF Spectrum Analyzer of the ACE/EPAM instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the solar wind rest frame.

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RPCLAP 3ESC4 CALIB2 V1.0

This data set containsCALIBRATED data from Rosetta RPC-LAP, acquired during the COMET ESCORT 4mission phase where the primary target was the comet67P/CHURYUMOV-GERASIMENKO 1 (1969 R1). It contains instrument outputs involts and amperes, calibrated and corrected for instrument offsets.

Tags: __
Organization: National Aeronautics and Space Administration