AndreaBozzo/ceres-open-data-index huggingface dataset:
ROSETTA-ORBITER 67P RSI 1/2/3 ROSETTA EXTENSION 1 1322 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 2016-01-08T08:58:40.000 to 2016-01-08T14:37:56.500.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER COMET ESCORT 1 OSIWAC 2 EDR MTP012 V2.0

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

Tags: __
Organization: National Aeronautics and Space Administration
STEREO-A PLASTIC Suprathermal Event List

This data product contains a list of automatically identified suprathermal proton events measured on the Wide Angle Partition without a Solid State Detector (WAP non-SSD) portion of the STEREO/PLASTIC instrument. This list in conjunction with the IMPACT magnetic field information and PLASTIC solar wind data can aid a user in identifying energetic proton events related to Stream Interaction Regions (SIRs), shocks, upstream events, magnetospheric events, etc.

Tags: thermalplasma
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER MARS RPCLAP3 MARS CALIB2 V1.0

This data set containsCALIBRATED data from Rosetta RPC-LAP, acquired during the MARS SWING-BYmission phase where the primary target was the planet MARS. It containsinstrument outputs in volts and amperes, calibrated and corrected forinstrument offsets.

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Organization: National Aeronautics and Space Administration
Cluster-Samba Electron Drift Instrument (EDI) Data at the ESA Cluster Science Archive

The Electron Drift Instrument (EDI) data products from the Cluster spacecraft in three main categories: (1) Electron enegergies measured between 0.5 and 1.0 keV for the Windshield Wiper mode: time series of the three components of the electron drift velocity and of the three components of the electric field in Cartesian GSE coordinate system (corrected for spacecraft motion) with different qualities and time resolution at 1-4 sec (PP, PPP, MPD); (2) Ambient electron measurements at fixed enegeris of 0.5 or 1.0 keV: time series of electron counts normally at 16 ms for the three pitch angles 0 deg, 90 deg, 180 deg, the detector look direction in the spacecraft frame and in GSE and the status for AE mode; and (3) Overview plot of the main parameters for both modes for every 3 h for one reference spacecraft (usually Cluster III).  Besides the main products, there also are raw data and auxiliary data. Raw data consist of merged science files (MSF) that are obtained by merging the housekeeping and science (burst (BM) and normal (NM) mode) telemetry files. They are in binary format.  Auxiliary are either data used internally by the main data production software or data dedicated to intercalibration or time-interval lists of the EDI operation modes. For more details, see "The Cluster Active Archive: Studying the Earth's Space Plasma Environment", edited by Dr. Harri Laakso, Matthew G. T. T. Taylor, C. Philippe Escoubet, from which this information was obtained.

Tags: electricfield
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 2 0845 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 2015-06-16T03:48:45.000 to 2015-06-16T05:15:07.500.

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Organization: National Aeronautics and Space Administration
STEREO-A PLasma and Supra-Thermal Ion Composition (PLASTIC) He++ Phase Space Densities and Counts in 6 normailzed Velocity Ranges and Proton Plasma Moments, Level 3 (L3), 1 h Data

This data set presents STEREO-A PLASTIC PickUp Ion, PUI, He⁺² phase space densities, PSD, in the spacecraft frame of reference. The data set provides 1 hr averages of He⁺², phase space density as a function of V/Vsw in 51 velocity ranges, where V and Vsw are the PUI particle speed and bulk speed of solar wind protons, respectively. These data are delivered to the public domain on a regular basis. Efforts are made to include the latest known calibration and background determinations, however, these are expected to undergo revision. We therefore suggest that users regularly return to this page, and make sure to get the most recent revision. If the STEREO PLASTIC data are used in presentations or publications, we strongly suggest that that the authors contact A.B. Galvin, STEREO PLASTIC PI, at toni.galvin@unh.edu and Dr. B. Klecker at berndt.klecker@mpe.mpg.de to ensure that the latest release of the data is utilized. Also, please acknowledge the STEREO PLASTIC Investigation, A.B. Galvin and NASA Grants NNX15AU01G and 80NSSC17K0556. For reporting purposes, we request bibliography information for any publication, etc., using these data. Please send information on the use of these data to A.B. Galvin. If you have questions regarding the data formats, please contact the STEREO PLASTIC Data System Manager: Lorna Ellis at lorna.ellis@unh.edu.

Tags: energeticparticles, instrumentstatus, thermalplasma
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P VIRTIS 2 ESCORT 4 MTP023 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 ESCORT 4 MTP023 phase, which occurred from 2015-11-18 to 2015-12-16. 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
AVIRIS-NG L1B Calibrated Radiance, Facility Instrument Collection, V1

This dataset contains Level 1B (L1B) orthocorrected, scaled radiance image files as well as files of observational geometry and illumination parameters and supporting sensor band information from the Airborne Visible / Infrared Imaging Spectrometer-Next Generation (AVIRIS-NG) instrument. This is the NASA Earth Observing System Data and Information System (EOSDIS) facility instrument archive of these data. The NASA AVIRIS-NG is a pushbroom spectral mapping system with high signal-to-noise ratio (SNR), designed and toleranced for high performance spectroscopy. AVIRIS-NG measures reflected radiance at 5-nm intervals in the Visible to Shortwave Infrared (VSWIR) spectral range from 380-2510 nm. The AVIRIS-NG sensor has a 1 milliradian instantaneous field of view, providing altitude dependent ground sampling distances from 20 m to sub-meter range. In this dataset, for each flight line, six file types are included: orthocorrected calibrated radiance image (img) files, geometric lookup table (glt) and orthocorrected observation geometry and illumination (obs_ort) files. Also included are unprojected files of input geometry (igm), parameters relating to the geometry of observation and illumination (obs), and orthocorrected locations of each pixel (loc). In addition, ancillary files for the flight line are provided, including quick look images and polygon outlines of imagery footprints. The AVIRIS-NG L1B data are provided in ENVI binary format, which includes a flat binary file accompanied by a header (.hdr) file holding metadata in text format. The ancillary files include JPEG images and maps in Keyhole Markup Language (KML). The AVIRIS-NG is flown on a variety of aircraft platforms including the Twin Otter, the King Air B-200, and NASA's high altitude ER-2. This archive currently includes data from 2014 - 2022. Additional AVIRIS-NG facility instrument L1B data will be added as they become available. AVIRIS-NG supports NASA Science and applications in many areas including plant composition and function, geology and soils, greenhouse gas mapping, and calibration of orbital platforms.

Tags: earth-science-infrared-wavelengths-spectral-engineering-infrared-radiance, earth-science-visible-wavelengths-spectral-engineering-visible-radiance
Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 8 4252 V1.0

This is a Mars Express Radio Science data set, collected during the extended mission phase 2021-01-01 to 2022-12-31. It is a Occultation measurement and covers the time 2022-05-11T08:07:56.000 to 2022-05-11T10:40:03.000.

Tags: __
Organization: National Aeronautics and Space Administration
Cluster-Tango Electron Drift Instrument (EDI) Data at the ESA Cluster Science Archive

The Electron Drift Instrument (EDI) data products from the Cluster spacecraft in three main categories: (1) Electron enegergies measured between 0.5 and 1.0 keV for the Windshield Wiper mode: time series of the three components of the electron drift velocity and of the three components of the electric field in Cartesian GSE coordinate system (corrected for spacecraft motion) with different qualities and time resolution at 1-4 sec (PP, PPP, MPD); (2) Ambient electron measurements at fixed enegeris of 0.5 or 1.0 keV: time series of electron counts normally at 16 ms for the three pitch angles 0 deg, 90 deg, 180 deg, the detector look direction in the spacecraft frame and in GSE and the status for AE mode; and (3) Overview plot of the main parameters for both modes for every 3 h for one reference spacecraft (usually Cluster III).  Besides the main products, there also are raw data and auxiliary data. Raw data consist of merged science files (MSF) that are obtained by merging the housekeeping and science (burst (BM) and normal (NM) mode) telemetry files. They are in binary format.  Auxiliary are either data used internally by the main data production software or data dedicated to intercalibration or time-interval lists of the EDI operation modes. For more details, see "The Cluster Active Archive: Studying the Earth's Space Plasma Environment", edited by Dr. Harri Laakso, Matthew G. T. T. Taylor, C. Philippe Escoubet, from which this information was obtained.

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

Total B and %B 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
ROSETTA-ORBITER 67P OSINAC 2 PRL-MTP003 EDR V3.0

This CODMAC level 2 data set contains uncalibrated image data in DN unit, acquired by the OSIRIS Narrow Angle Camera on the Rosetta spacecraft during the PRELANDING mission phase, covering the period from 2014-05-07T12:48:00.000 to 2014-06-04T10:49:59.000. The prime target is comet 67P/Churyumov-Gerasimenko 1 (1969 R1). This version V3.0 supersedes previous deliveries of the same dataset with the following changes since the last version: Lien corrected dataset after the July and October 2018 PSA/PDS external peer reviews. Updated documentation and ancillary files, added document on bandpass filter. Updated SCIENCE_USER_GUIDE_V03.PDF to include one section about FAQ and one section about image data quality. Added shutter backtravel and readout issues to image quality map. Updated DATA_QUALITY_ID keyword in image header. Improved handling of images with missing packets. Included FITs files. Browse products changed to the same size as the original image.

Tags: __
Organization: National Aeronautics and Space Administration
Cluster Summary Parameter Electron Drift Instrument (EDI) Data

This instrument (EDI: Electron Drift Instrument) measures the drift of a weak beam of test electrons that, when emitted in certain directions, return to the spacecraft after one gyration. This drift is related to the electric field and the gradient in the magnetic field, and these quantities can, by the use of different electron energies, be determined separately. The fundamental time step to determine the new parameters and direct the beams and the detectors is 2 ms. Inter-experiment links include: magnetic field information from FGM and STAFF, a blanking pulse received from WHISPER to warn of possible interference from that active experiment, and a similar blanking pulse sent to PEACE when the EDI electron beam could interfere with the PEACE electron measurement. For more details of the Cluster mission, the spacecraft, and its instruments, see the report Cluster: mission, payload and supporting activities, March 1993, ESA SP-1159, and the included article The Electron Drift Instrument for Cluster, by G. Paschmann et al., from which this information was obtained.

Tags: auroral-region, bow-shock, cluster, cusp, electricfield-60-second, lobe, magnetosheath, magnetosphere, magnetotail, polar-cap, solar-wind
Organization: National Aeronautics and Space Administration
STEREO-A Carrington Maps for the SECCHI Cor1 Telescope

Synoptic (or Carrington) Maps comprise an efficient method to summarize both short term and long term coronal evolution. This resource contains East and West limb maps from the Cor1 and Cor2 coronagraphs, East(West) limb maps for HI1/2-A (HI1/2-B) imagers, and central meridian maps from the EUVI telescope. Maps are available for each Carrington Rotation since the beginning of the STEREO mission. The maps demonstrate the evolution of the corona from a relatively simple, two-sectored structure to an increasingly complex multi-sectored structure. Distortions and discontinuities in the streamer belt visible in the limb maps are associated with active regions on the sun, the shape of the current sheet, and coronal mass ejections. Meridian maps for EUVI illustrate the corresponding structures and long-term changes in the lower atmosphere.

Tags: imageintensity
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSIWAC 4 EXT2-MTP029 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 Wide Angle Camera during the ROSETTA EXTENSION 2 phase of the Rosetta mission, covering the period from 2016-05-03T23:25:00.000 to 2016-05-31T23:24:59.000.

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Organization: National Aeronautics and Space Administration
MARS EXPRESS SUN MRS 1/2/3 EXTENDED MISSION 7 4065 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 Solar Conjunction measurement and covers the time 2019-09-20T00:15:00.000 to 2019-09-20T02:45:00.000.

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Organization: National Aeronautics and Space Administration
STEREO-A/SECCHI/HI-1 FITS data

The Heliospheric Imager-1 (HI-1) telescope is part of the Sun Earth Connection Coronal and Heliospheric Investigations (SECCHI) instrument suite on the NASA STEREO mission. The SECCHI on the two STEREO spacecraft are identical suites of remote sensing instruments designed to observe coronal mass ejections (CMEs) at the Sun and in transit outwards to 1 AU. The HI-1 telescope observes the inner heliosphere from 12 to 84 solar radii with the band-pass wavelength of 450-750 nm.

Tags: imageintensity
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 PRELANDING 0247 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 2014-08-27T06:36:40.000 to 2014-08-27T12:05:39.000.

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Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 3 3285 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 2012-05-12T09:07:16.000 to 2012-05-12T10:17:05.500.

Tags: __
Organization: National Aeronautics and Space Administration
STEREO-A Carrington Maps for the SECCHI Cor2 Telescope

Synoptic (or Carrington) Maps comprise an efficient method to summarize both short term and long term coronal evolution. This resource contains East and West limb maps from the Cor1 and Cor2 coronagraphs, East(West) limb maps for HI1/2-A (HI1/2-B) imagers, and central meridian maps from the EUVI telescope. Maps are available for each Carrington Rotation since the beginning of the STEREO mission. The maps demonstrate the evolution of the corona from a relatively simple, two-sectored structure to an increasingly complex multi-sectored structure. Distortions and discontinuities in the streamer belt visible in the limb maps are associated with active regions on the sun, the shape of the current sheet, and coronal mass ejections. Meridian maps for EUVI illustrate the corresponding structures and long-term changes in the lower atmosphere.

Tags: imageintensity
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER COMET PRELANDING OSIWAC 3 RDR DATA MTP 004

This data set contains calibrated images acquired by the OSIRIS Wide AngleCamera during the prelanding phase of the Rosetta mission at the comet 67P,covering the period from 2014-06-04 to 2014-06-18.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 PRELANDING 0351 V1.0

This is a Rosetta Radio Science data set, collected during the PRELANDING phase 2014-01-21 to 2014-11-18. It is a Global Gravity measurement at the comet 67P and covers the time 2014-10-12T03:13:11.000 to 2014-10-12T08:18:56.000.

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Organization: National Aeronautics and Space Administration
STEREO SECCHI EUVI Wsvelet-processed images

The EUVI images (all four wavelengths) are processed via a wavelet-based multi-scale algorithm to remove the zeroth order component (primarily stray light). The algorithm is tuned to enhance the off-limb emission in the images. The resulting images are stored as both FITS (using the original header) and PNGs and can be ingested by the SECCHI Solarsoft IDL routines for analysis

Tags: imageintensity
Organization: National Aeronautics and Space Administration
STEREO-A/SECCHI/Cor2 FITS data

Cor2 is one of the coronagraphs aboard the STEREO-A spacecraft. It is part of the SECCHI instrument suite. It observes the off-limb corona between 2.5-15 solar radii in visible light. It acquires both total and polarized brightness images.

Tags: imageintensity
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 1 0575 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 2015-02-11T11:03:35.000 to 2015-02-11T13:07:10.500.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSINAC 4 EXT3-MTP033 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 ROSETTA EXTENSION 3 phase of the Rosetta mission, covering the period from 2016-08-09T23:25:00.000 to 2016-09-02T06:39:59.000.

Tags: __
Organization: National Aeronautics and Space Administration
STEREO-A/WAVES Low Frequency Receiver, Data

Radio measurements of power spectral density,radio flux density, Stokes Q, U, V parameters and angular half width of source measured by the STEREO-A/WAVES instrument. There a 48 linearly spaced frequency channels from 2.61 to 153 kHz. Time resolution varies with instrument mode ranging from 15 seconds to 1 minute.

Tags: electricfield, waves
Organization: National Aeronautics and Space Administration
MARS EXPRESS MARSIS RDR ACTIVE IONOSPHERE SOUNDING EXT1 V1.0

The Mars Express MARSIS Active Ionospheric Sounder (AIS) full      resolution data set includes all spectral information      calibrated in units of spectral density for the entire Mars      Express nominal mission.  The data set consists of a transmit      frequency followed by a time series of spectral density      measurements of the received power.  Browse products contain      a spectrogram overview plot and individual ionograms for each      sounding  activity.

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 1 0509 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 2014-12-27T01:43:05.000 to 2014-12-27T12:08:04.500.

Tags: __
Organization: National Aeronautics and Space Administration
STEREO-A SWAVES new one minute averages of the low (lfr) frequency receiver data.

The two STEREO radio receivers measure wave intensity, source direction and angular size in the frequency \n   range 40 kHz to 16 MHz, corresponding to heliocentric source distances of about 1 Rs to 1 AU. One 10-40 kHz \n   receiver measures radio and plasma waves near the 1 AU electron plasma frequency. One receiver makes high \n   time resolution measurements at 50 MHz. Time Domain Samplers make simultaneous wideband waveform measurements \n   on three electric components. Antenna systems include three mutually orthogonal 6-meter monopoles. \n

Tags: stereo-a, swaves, waves-low-frequency-receiver
Organization: National Aeronautics and Space Administration
CASSINI SS/S RPWS CALIBRATED LP POTENTIAL CURRENT V1.0

The Cassini Radio and Plasma Wave Science (RPWS) Langmuir Probe      Sweep voltage-current data set comprises calibrated      Voltage-Current (U-I) characteristics acquired almost      continuously from most mission phases during the entire Cassini      mission.  The full data set of Voltage-Current characteristics      is intended to become the most comprehensive and complete data      set from which thermal plasma parameters can be derived in the      Cassini RPWS archive.  Data are presented in text tables and are      organised so as to have fixed-length records for ease in data      handling.  These can be used to derive higher level data      products like thermal plasma parameters, e.g., electron density      and temperature.

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Organization: National Aeronautics and Space Administration
CNOFS CINDI IVM 500 ms Ion Drift Data

This data set contains plasma parameters of the equatorial F-region in the ionosphere measured by the Ion Velocity Meter (IVM) of the Coupled Ion-Neutral Dynamics Investigation (CINDI) payload on board the CNOFS spacecraft. Data are available in HDF format, with an IDL program to read and plot them. Each file contains data from one day of spacecraft operation and the file contains eight primary geophysical parameters: the ion temperature (Ti) in degrees Kelvin, the ion flow in m/s in the ram (i.e.--spacecraft velocity) direction (+Vx in the direction of spacecraft velocity), the ion flows in m/s in the horizontal and vertical directions (Vy and Vz) at right angles to the ram direction (+Vz is downward, +Vy is roughly southward), the total ion density (Ni) (the sum of O+ and H+ and He+ concentrations) in ions/cc, and the individual H+, He+, and O+ concentrations in ions/cc. In addition, ion velocities also are given in the coordinate system of the local magnetic field (parallel, perpendicular, and meridional) in the plots and as ASCII data on the UT Dallas website. Based on the IGRF model, the data are transformed into magnetic coordinates only if all three ion velocities in the spacecraft coordinates are available and good.

Tags: thermalplasma
Organization: National Aeronautics and Space Administration