AndreaBozzo/ceres-open-data-index huggingface dataset:
Ekati THEMIS Ground-based All Sky Imager; Full Resolution Images.

THEMIS Ground All Sky Imager at Ekati (64.72 deg GLat, 250.67 deg GLong): 256 x 256 pixel full resolution images of auroral oval.  The ASI stations monitor a 170 degree field of view imaging the auroral oval at kilometer resolution.  The ASI is comprised of a fisheye lens and CCD in a stainless steel enclosure topped with a transparent acrylic dome.  The CCD has a resolution of 256 x 256 pixels.  Exposure control ranges from 5 s to 1 ms although the typical data rate is one image every 3 seconds.  Silicone heaters keep the instrument within the nominal temperature range.  During daylight hours a sun shades deploy to protect the CCD.\n

Tags: imageintensity
Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 7 4128 V1.0

This is a Mars Express Radio Science data set, collected during the extended mission phase 2019-01-01 to 2020-12-31. It is a Occultation measurement and covers the time 2020-09-13T05:21:46.000 to 2020-09-13T05:43:54.500.

Tags: __
Organization: National Aeronautics and Space Administration
THEMIS GBO All Sky Imager at Ekati, NT, Canada. ASI Thumbnails Data.

THEMIS Ground All Sky Imager at Ekati (64.72 deg GLat, 250.67 deg GLong): 32 x 32 pixel thumbnails for full ASI images.  The ASI stations monitor a 170 degree field of view imaging the auroral oval at kilometer resolution.  The ASI is comprised of a fisheye lens and CCD in a stainless steel enclosure topped with a transparent acrylic dome.  The CCD has a resolution of 256 x 256 pixels.  Exposure control ranges from 5 s to 1 ms although the typical data rate is one image every 3 seconds.  Silicone heaters keep the instrument within the nominal temperature range.  During daylight hours sun shades deploy to protect the CCD.\n

Tags: imageintensity
Organization: National Aeronautics and Space Administration
Fresno (FRN) Ground-based Vector Magnetic Field (L2) 1.0 s Data

Fresno, CA, Ground-based Vector Magnetic Field Level 2 Data, 1.0 s Time Resolution, Station Code: (FRN), Station Location: (GEO Latitude 37.1, Longitude 240.3), USGS Network

Tags: magneticfield
Organization: National Aeronautics and Space Administration
Fort Simpson THEMIS Ground-based All Sky Imager; Full Resolution Images.

THEMIS Ground All Sky Imager at Fort Simpson (61.76 deg GLat, 238.77 deg GLong): 256 x 256 pixel full resolution images of auroral oval.  The ASI stations monitor a 170 degree field of view imaging the auroral oval at kilometer resolution.  The ASI is comprised of a fisheye lens and CCD in a stainless steel enclosure topped with a transparent acrylic dome.  The CCD has a resolution of 256 x 256 pixels.  Exposure control ranges from 5 s to 1 ms although the typical data rate is one image every 3 seconds.  Silicone heaters keep the instrument within the nominal temperature range.  During daylight hours a sun shades deploy to protect the CCD.\n

Tags: imageintensity
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RPCMIP 3 ESC1 V2.0

This archive contains calibrated data from the RPC-MIP instrument onboard ROSETTA Orbiter, acquired during the comet escort part 1 mission phase. The primary target was comet 67P/C-G. It also contains documentation which describes the MIP experiment. This is V2.0 updated after Science Review.

Tags: __
Organization: National Aeronautics and Space Administration
THEMIS GBO All Sky Imager at Fort Simpson, NT, Canada. ASI Thumbnails Data.

THEMIS Ground All Sky Imager at Fort Simpson (61.76 deg GLat, 238.77 deg GLong): 32 x 32 pixel thumbnails for full ASI images.  The ASI stations monitor a 170 degree field of view imaging the auroral oval at kilometer resolution.  The ASI is comprised of a fisheye lens and CCD in a stainless steel enclosure topped with a transparent acrylic dome.  The CCD has a resolution of 256 x 256 pixels.  Exposure control ranges from 5 s to 1 ms although the typical data rate is one image every 3 seconds.  Silicone heaters keep the instrument within the nominal temperature range.  During daylight hours sun shades deploy to protect the CCD.\n

Tags: imageintensity
Organization: National Aeronautics and Space Administration
Gjoa Haven (GJOA/GJO) Ground-based Vector Magnetic Field (L2) 0.5 s Data

Gjoa Haven, NU, Ground-based Vector Magnetic Field Level 2 Data, 0.5 s Time Resolution, Station Code: (GJOA/GJO), Station Location: (GEO Latitude 68.6, Longitude 264.1), MACCS Network

Tags: magneticfield
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P VIRTIS 2 ESCORT 2 MTP015 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 2 MTP015 phase, which occurred from 2015-04-08 to 2015-05-06. 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

Tags: __
Organization: National Aeronautics and Space Administration
Fort Yukon THEMIS Ground-based All Sky Imager; Full Resolution Images.

THEMIS Ground All Sky Imager at Fort Yukon (66.56 deg GLat, 214.79 deg GLong): 256 x 256 pixel full resolution images of auroral oval.  The ASI stations monitor a 170 degree field of view imaging the auroral oval at kilometer resolution.  The ASI is comprised of a fisheye lens and CCD in a stainless steel enclosure topped with a transparent acrylic dome.  The CCD has a resolution of 256 x 256 pixels.  Exposure control ranges from 5 s to 1 ms although the typical data rate is one image every 3 seconds.  Silicone heaters keep the instrument within the nominal temperature range.  During daylight hours a sun shades deploy to protect the CCD.\n

Tags: imageintensity
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 3 1111 V1.0

This is a Rosetta Radio Science data set, collected during the COMET ESCORT 3 phase 2015-07-01 to 2015-10-21. It is a Global Gravity measurement at the comet 67P and covers the time 2015-10-18T20:28:00.000 to 2015-10-18T23:45:09.000.

Tags: __
Organization: National Aeronautics and Space Administration
Climate Normals for Last Glacial Maximum and Modern (1975-2005), Alaska

This dataset provides two 30-year climate normal data products for conditions during the last glacial maximum (LGM; ~18,000 years ago) and a modern time period (1975-2005) for the entire state of Alaska. The first set of products are monthly climate variable averages at 60 m resolution, including: minimum, maximum, and average temperatures, total precipitation, total surface radiation, rain, snow, potential evapotranspiration (PET), actual evapotranspiration (AET), and water deficit. The second set of products are annual summary climate variable averages for the same variables (excepting average temperature and rain) at 60m, 120m, 240m, 800m, 1km, 2km, 3km, 4km, 5km, 10km and 12km resolutions. The 30-year climate normal monthly averages were derived by topographically downscaling climate variables from existing coarse-resolution general circulation model outputs combined with local weather station data and digital surface models for Alaska for both the LGM and modern time periods at 60 m resolution. From this baseline, monthly averages for total surface radiation, rain, snow, potential evapotranspiration, actual evapotranspiration, and water deficit were also modeled. The annual averages are coarser resolution upsampled versions of the 60 m resolution monthly average data.

Tags: earth-science-atmospheric-radiation-atmosphere-solar-radiation, earth-science-atmospheric-temperature-atmosphere-surface-temperature, earth-science-atmospheric-water-vapor-atmosphere-water-vapor-processes-evaporation, earth-science-paleoclimate-indicators-climate-indicators-paleoclimate-reconstructions, earth-science-precipitation-atmosphere-precipitation-amount, earth-science-precipitation-atmosphere-solid-precipitation-snow
Organization: National Aeronautics and Space Administration
Gakona THEMIS Ground-based All Sky Imager; Full Resolution Images.

THEMIS Ground All Sky Imager at Gakona (62.39 deg GLat, 214.87 deg GLong): 256 x 256 pixel full resolution images of auroral oval.  The ASI stations monitor a 170 degree field of view imaging the auroral oval at kilometer resolution.  The ASI is comprised of a fisheye lens and CCD in a stainless steel enclosure topped with a transparent acrylic dome.  The CCD has a resolution of 256 x 256 pixels.  Exposure control ranges from 5 s to 1 ms although the typical data rate is one image every 3 seconds.  Silicone heaters keep the instrument within the nominal temperature range.  During daylight hours a sun shades deploy to protect the CCD.\n

Tags: imageintensity
Organization: National Aeronautics and Space Administration
Homer (HOMR) Ground-based Vector Magnetic Field (L2) 0.5 s Data

Homer, AK, Ground-based Vector Magnetic Field Level 2 Data, 0.5 s Time Resolution, Station Code: (HOMR), Station Location: (GEO Latitude 59.7, Longitude 209.5), University of Alaska Network

Tags: magneticfield
Organization: National Aeronautics and Space Administration
MARS EXPRESS MARSIS RDR ACTIVE IONOSPHERE SOUNDING EXT2 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.

Tags: __
Organization: National Aeronautics and Space Administration
Goose Bay THEMIS Ground-based All Sky Imager; Full Resolution Images.

THEMIS Ground All Sky Imager at Goose Bay (53.32 deg GLat, 299.54 deg GLong): 256 x 256 pixel full resolution images of auroral oval.  The ASI stations monitor a 170 degree field of view imaging the auroral oval at kilometer resolution.  The ASI is comprised of a fisheye lens and CCD in a stainless steel enclosure topped with a transparent acrylic dome.  The CCD has a resolution of 256 x 256 pixels.  Exposure control ranges from 5 s to 1 ms although the typical data rate is one image every 3 seconds.  Silicone heaters keep the instrument within the nominal temperature range.  During daylight hours a sun shades deploy to protect the CCD.\n

Tags: imageintensity
Organization: National Aeronautics and Space Administration
Hot Springs (HOTS) Ground-based Vector Magnetic Field (L2) 0.5 s Data

Hot Springs, MT, Ground-based Vector Magnetic Field Level 2 Data, 0.5 s Time Resolution, Station Code: (HOTS), Station Location: (GEO Latitude 47.6, Longitude 245.3), THEMIS EPO/UCLA Network

Tags: magneticfield
Organization: National Aeronautics and Space Administration
IHW COMET HALLEY - U-V VISIBILITY DATA

NASA's International Halley Watch (IHW) has created a Comet Halley Archive. The collection of data spans the full wavelength range as submitted by scientists to the IHW. The observations belong to one of the following Disciplines: Amateur, Astrometry, Infrared Studies, Large-Scale Phenomena, Meteor Studies, Near-Nucleus Studies, Photometry and Polarimetry, Radio Studies, and Spectroscopy and Spectrophotometry. The data collected by these nine disciplines were augmented by Spacecraft measurements. The data were submitted to IHW, but the evaluation and selection for the Archive has been the primary responsibility of the Discipline Specialist Teams for each network in cooperation with the Lead Center. The Radio Studies Network provided u-v visibility data containing 7 continuum and 29 spectral line observations, 17 of the latter being OH. The dates spanned were from 1985 November 13 through 1986 January 31.

Tags: __
Organization: National Aeronautics and Space Administration
MARS EXPRESS ASPERA-3 FLUX DDR ION MASS ANALYZER EXT8 V1.0

This data set contains Mars Express ASPERA-3 Ion Mass         Analyzer (IMA) data for the eighth mission extension         (January 1, 2021 - December 31, 2022).         The data are provided in units of Differential Number Flux,         m-2 s-1 sr-1 eV-1

Tags: __
Organization: National Aeronautics and Space Administration
THEMIS GBO All Sky Imager at Gillam, MB, Canada. ASI Thumbnails Data.

THEMIS Ground All Sky Imager at Gillam (56.35 deg GLat, 265.34 deg GLong) 32 x 32 pixel thumbnails for full ASI images.  The ASI stations monitor a 170 degree field of view imaging the auroral oval at kilometer resolution.  The ASI is comprised of a fisheye lens and CCD in a stainless steel enclosure topped with a transparent acrylic dome.  The CCD has a resolution of 256 x 256 pixels.  Exposure control ranges from 5 s to 1 ms although the typical data rate is one image every 3 seconds.  Silicone heaters keep the instrument within the nominal temperature range.  During daylight hours sun shades deploy to protect the CCD.\n

Tags: imageintensity
Organization: National Aeronautics and Space Administration
MGN V RADAR SYSTEM DERIVED MIDR COMPRESSED THRICE V1.0

This data set contains the Magellan Compressed Thrice Mosaicked Image Data Records (C3-MIDRs) which consists of mosaics generated by computing 3x3 pixel arithmetic moving averages from the C2-MIDRs. Each C3-MIDR is in a sinusoidal equal area projection and has an origin at 0 degrees latitude, with the central meridian defined as the longitude bisecting the mosaic. Each C1-MIDR has 7168 lines (aligned with latitudes) and 8192 samples, arranged as 56 1024 x 1024 files on CD-ROM. C3-MIDRs, with their 2.025 km pixel widths, are designed to cover the planet at reasonably high resolution and high signal to noise ratio. The 1024 x 1024 files have a VICAR2 format, with embedded VICAR2 labels. The data have been placed on CD-ROMs with documentation, detached Planetary Data System labels, and summary tabular information.

Tags: __
Organization: National Aeronautics and Space Administration
CLM Simulated Solar-Induced Fluorescence, Niwot Ridge, Colorado, USA, 1998-2018

This dataset provides results for simulations of solar-induced chlorophyll fluorescence (SIF) implemented within the terrestrial biosphere Community Land Model (CLM 4.5) for Niwot Ridge, Colorado, USA, from 1998-2018. The data include outputs from three model simulations designed to test the importance of non-photochemical quenching (NPQ), that is, the absorbed light energy dissipated as heat, in determining seasonal SIF.

Tags: earth-science-ecological-dynamics-biosphere-ecosystem-functions-photosynthesis, earth-science-vegetation-biosphere-chlorophyll, earth-science-vegetation-biosphere-leaf-characteristics
Organization: National Aeronautics and Space Administration
LP ELECTRON REFLECTOMETER OMNI DIR.        ELECTRON FLUX 80SEC V1.1

Time ordered low resolution datafrom the Lunar Prospector Electron Reflectometer, averaged over 16spacecraft spins, in units of particles/cm**2/sec/steradian/eV,for dates 1998-01-16 to 1999-07-29.

Tags: __
Organization: National Aeronautics and Space Administration
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 3 3267 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 2012-04-25T09:54:12.000 to 2012-04-25T14:50:44.500.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 3 0930 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 2015-07-30T21:26:00.000 to 2015-07-31T05:23:46.500.

Tags: __
Organization: National Aeronautics and Space Administration
ACE SWEPAM/SWICS Level 3 Merged Solar Wind Proton Data

These data files contain 12-min resolution solar wind\nproton flow velocity (GSE, RTN and GSM components), scalar speed, density, \nand (radial component of) temperature, plus the alpha particle to proton \ndensity ratio.  The data are typically from the SWEPAM instrument.  But \nbecause SWEPAM has reduced sensitivity at the lowest energies, and at \ntimes underestimates the proton density, especially for very slow wind, \nproton density is sometimes culled from low-speed (.LT. ~350 km/s) \nintervals in the SWEPAM Level 2 data, and proton temperature may also \nbe culled. More rarely, the solar wind velocity may also be culled, \nespecially during periods of both high solar energetic particle \nbackground and high wind speeds.  In these cases, SWICS-determined \nproton density and temperature, and possibly also flow speed (not \nvelocity vectors), are included in the data records, with a flag to\nindicate whether, and which, SWICS parameters are in the records.\nAs of July, 2012, data were available to the end of 2009.

Tags: thermalplasma
Organization: National Aeronautics and Space Administration
STEREO-B/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
GO EAR PLS SUMM EARTH-1 ET V1.0

This file is a listing of particle energy spectra from the      Galileo Plasma Instrument (PLS) during the first Earth      Encounter. Detector reponses from ion detetors 2P, 4P, and      6P, and from electron detector 4E are available through the      PDS as separate files.

Tags: __
Organization: National Aeronautics and Space Administration
STEREO-B 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
AE-E MSIS Neutral Density Data

This set of neutral density data was deduced from the mass spectrometer measurements on the Atmosphere Explorer E's Bennett Ion-Mass Spectrometer and Open-Source Neutral Mass Spectrometer.  The density numbers (in cm-3) for hydrogen, nitrogen and molecular oxygen were provided by A. Hedin (GSFC, Code 914, now retired). They are related to A. Hedin's atmospheric modelling work (Mass Spectrometer and Incoherent Scatter atmospheric model - MSIS). In addition to density, the record includes also orbital parameters.

Tags: neutralgas, radiance, thermalplasma
Organization: National Aeronautics and Space Administration
STEREO-B 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
Circumpolar Flaw Lead System Study

Measurements taken within the Cape Bathurst flaw lead on board the icebreaker C.C.G.S. Amundsen to examine how physical changes affect biological processes in the flaw lead through an entire annual cycle (October 2007 - August 2008). The circumpolar flaw lead occurs each year when the central pack ice moves away from the coastal fast ice creating an area of open water called a flaw lead.

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
ACE SWICS 2.0 Solar Wind 2-Hour Data

The SWICS 2.0 dataset consists of time series measurements by ACE/SWICS of the elemental abundance, charge state composition, and kinetic distribution of heavy ions in the solar wind. This data set begins after August 23, 2011, when a radiation and age-induced hardware anomaly altered the instrument's operational state. It should not be confused with SWICS 1.1, the recalibrated data set extending from launch up to the anomaly. SWICS 2.0 continues to make heavy ion measurements which are not available from any other instrument, and new data analysis methods have been developed to address the statistical and calibration issues of the current instrument state.

Tags: ioncomposition, thermalplasma
Organization: National Aeronautics and Space Administration
STEREO-B/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