AndreaBozzo/ceres-open-data-index huggingface dataset:
CERES ERBE-like Gridded Instantaneous TOA Fluxes Aqua Crosstrack Edition4

CER_ES9_Aqua-Xtrk_Edition4 is the Clouds and the Earth's Radiant Energy System (CERES) Earth Radiation Budget Experiment (ERBE)-like Gridded Instantaneous Top-of-the-Atmosphere (TOA) Fluxes Aqua Cross-track Edition 4 data product, which was collected using the CERES-Flight Model (FM3) and FM4 instruments on the Aqua platform. Data collection for this product is ongoing. The ERBE-like Monthly Regional Averages (ES-9) products contain a month of space and time-averaged CERES data for a single satellite using measurements from the primary cross-track instrument. All instantaneous shortwave and longwave fluxes at the TOA from the CERES ES-8 product for a month are sorted by 2.5-degree spatial regions, by day number, and by the local hour of observation. The mean of the instantaneous fluxes for a given region-day-hour bin is determined and recorded on the ES-9, along with other flux statistics and scene information. For each region, the daily average flux is estimated from an algorithm that uses the available hourly data, scene identification data, and diurnal models. This algorithm is "like" the algorithm used for ERBE. ES-9 also contains hourly average fluxes for the month and an overall monthly average for each region. These average fluxes are given for both clear-sky and total-sky scenes. CERES is a key Earth Observing System (EOS) program component. The CERES instruments provide radiometric measurements of the Earth's atmosphere from three broadband channels. The CERES missions are a follow-on to the successful ERBE mission. The first CERES instrument, the protoflight model (PFM), was launched on November 27, 1997, as part of the Tropical Rainfall Measuring Mission (TRMM). Two CERES instruments (FM1 and FM2) were launched into polar orbit on board the Earth Observing System (EOS) flagship Terra on December 18, 1999. Two additional CERES instruments (FM3 and FM4) were launched on board Earth Observing System (EOS) Aqua on May 4, 2002. The CERES FM5 instrument was launched on board the Suomi National Polar-orbiting Partnership (NPP) satellite on October 28, 2011. The newest CERES instrument (FM6) was launched on board the Joint Polar-Orbiting Satellite System 1 (JPSS-1) satellite, now called NOAA-20, on November 18, 2017.

Tags: earth-science-atmospheric-radiation-atmosphere-albedo, earth-science-atmospheric-radiation-atmosphere-longwave-radiation, earth-science-atmospheric-radiation-atmosphere-net-radiation, earth-science-atmospheric-radiation-atmosphere-outgoing-longwave-radiation, earth-science-atmospheric-radiation-atmosphere-radiative-flux, earth-science-atmospheric-radiation-atmosphere-shortwave-radiation
Organization: National Aeronautics and Space Administration
CO2 and CH4 Fluxes from Waterbodies, Yukon-Kuskokwim Delta, Alaska, 2016-2019

This dataset provides estimates of carbon dioxide (CO2) and methane (CH4) diffusive fluxes from waterbodies, and watershed landcover data for the central-interior of the Yukon-Kuskokwim Delta (YK delta), Alaska. Dissolved concentrations of methane and carbon dioxide were predicted using an integrated terrestrial-aquatic approach to scale observations based on landscape and waterbody remote sensing drivers. The observations include ~300 samples of surface water dissolved gases collected in July 2016-2019 from the central region of the YK Delta, Alaska. A machine learning model was used to generate estimated fluxes. Model inputs include Sentinel-2 MSI with derived normalized difference vegetation index (NDVI) and normalized difference water index (NDWI), an Arctic digital elevation model (DEM) with derived slope and flow accumulation, Sentinel-1 C-band July and December VV and VH composites, and a landcover map. Waterbody size, shape, and reflectance were determined using object-based image analysis in Google Earth Engine. Landscape-level input data were averaged in non-nested sub-basins calculated using the System for Automated Geoscientific Analyses (SAGA) "channel network" algorithm at three threshold sizes. Cross validation was used to tune and select variables for gradient boosting models. The trained gradient boosting models were then used to predict dissolved methane and carbon dioxide in all waterbodies (~17,000) in the region. These aquatic concentrations were converted to fluxes using an average gas transfer velocity from observations (0.33 m/d). The data are provided in GeoTIFF and shapefile formats.

Tags: earth-science-atmospheric-chemistry-atmosphere-carbon-and-hydrocarbon-compounds-atmospheric-car, earth-science-ecosystems-biosphere-terrestrial-ecosystems-alpine-tundra, earth-science-land-use-land-cover-land-surface-land-use-land-cover-classification, earth-science-surface-water-terrestrial-hydrosphere-surface-water-chemistry, earth-science-surface-water-terrestrial-hydrosphere-surface-water-features, earth-science-surface-water-terrestrial-hydrosphere-surface-water-features-lakes-reservoirs, earth-science-surface-water-terrestrial-hydrosphere-surface-water-features-rivers-streams, earth-science-surface-water-terrestrial-hydrosphere-watershed-characteristics, earth-science-terrestrial-hydrosphere-indicators-climate-indicators-permafrost-melt, earth-science-topography-land-surface-topographic-effects, earth-science-vegetation-biosphere-vegetation-index-normalized-difference-vegetation-index-ndvi, earth-science-water-quality-water-chemistry-terrestrial-hydrosphere-gases-dissolved-carbon-diox, earth-science-water-quality-water-chemistry-terrestrial-hydrosphere-gases-dissolved-gases
Organization: National Aeronautics and Space Administration
VG2 JUP PWS EDITED SPECTRUM ANALYZER                                      4.0SEC V1.0

This data set consists of 4-second      edited, wave electric field intensities from the Voyager 2 Plasma Wave      Receiver spectrum analyzer obtained in the vicinity of the Jovian      magnetosphere. For each 4-second interval, a field strength is      determined for each of the 16 spectrum analyzer channels whose center      frequencies range from 10 Hertz to 56.2 kiloHertz and which are      logarithmically spaced in frequency, four channels per decade. The time      associated with each set of intensities (16 channels) is the time of      the beginning of the scan. During data gaps where complete 4-second      spectra are missing, no entries exist in the file, that is, the gaps are      not zero-filled or tagged in any other way. When one or more channels      are missing within a scan, the missing measurements are zero-filled.      Data are edited but not calibrated. The data numbers in this data set      can be plotted in raw form for event searches and simple trend analysis      since they are roughly proportional to the log of the electric field      strength.

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Organization: National Aeronautics and Space Administration
CERES ERBE-like Gridded Instantaneous TOA Fluxes (ES9) NPP CERES FM-5 Edition2

The ERBE-like Monthly Regional Averages (ES-9) product contains a month of space and time-averaged Clouds and the Earth's Radiant Energy System (CERES) data for a single satellite using measurements from the primary cross-track instrument. All instantaneous shortwave and longwave fluxes at the Top-of-the-Atmosphere (TOA) from the CERES ES-8 product for a month are sorted by 2.5-degree spatial regions, by day number, and by the local hour of observation. The mean of the instantaneous fluxes for a given region-day-hour bin is determined and recorded on the ES-9, along with other flux statistics and scene information. For each region, the daily average flux is estimated from an algorithm that uses the available hourly data, scene identification data, and diurnal models. This algorithm is "like" the algorithm used for the Earth Radiation Budget Experiment (ERBE). The ES-9 also contains hourly average fluxes for the month and an overall monthly average for each region. These average fluxes are given for both clear-sky and total-sky scenes. CERES is a key Earth Observing System (EOS) program component. The CERES instruments provide radiometric measurements of the Earth's atmosphere from three broadband channels. The CERES missions follow the successful Earth Radiation Budget Experiment (ERBE) mission. The first CERES instrument (PFM) was launched on November 27, 1997, as part of the Tropical Rainfall Measuring Mission (TRMM). Two CERES instruments (FM1 and FM2) were launched into polar orbit on board the EOS flagship Terra on December 18, 1999. Two additional CERES instruments (FM3 and FM4) were launched on board EOS Aqua on May 4, 2002. The CERES instrument (FM5) was launched on board the Suomi National Polar-orbiting Partnership (NPP) satellite on October 28, 2011. The last CERES instrument (FM6) was launched on board the Joint Polar Satellite System 1 (JPSS-1) satellite on November 18, 2017.

Tags: earth-science-atmospheric-radiation-atmosphere-albedo, earth-science-atmospheric-radiation-atmosphere-longwave-radiation, earth-science-atmospheric-radiation-atmosphere-net-radiation, earth-science-atmospheric-radiation-atmosphere-outgoing-longwave-radiation, earth-science-atmospheric-radiation-atmosphere-radiative-flux, earth-science-atmospheric-radiation-atmosphere-shortwave-radiation
Organization: National Aeronautics and Space Administration
CASSINI HIGH RATE DETECTOR V16.0

The High Rate Detector (HRD) from the University of Chicago is an independent part of the CDA instrument on the Cassini Orbiter that measures the dust flux and particle mass distribution of dust particles hitting the HRD detectors. This data set includes all data from the HRD through December 31, 2015. Please refer to Srama et al. (2004) for a detailed HRD description.

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

Geotail linearly interpolated to have the measurements on the minute at 60 s resolution CPI data in GSM coordinates. This data set consists of processed solar wind data that has been linearly interpolated to 1 min resolution at the position of the spacecraft using the interp1.m function in MATLAB. This data set was originally constructed by Dr. J.M. Weygand for Prof. R.L. McPherron, who was the principle investigator of two National Science Foundation studies: GEM Grant ATM 02-1798 and a Space Weather Grant ATM 02-08501. These data were primarily used in superposed epoch studies and cross correlation studies on solar wind.

Tags: bow-shock, cpi, geotail, magnetopause, magnetotail, plasma-data, solar-wind, thermalplasma-1-min
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 PRELANDING 0262 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 2014-08-31T12:31:00.000 to 2014-08-31T17:51:40.500.

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Organization: National Aeronautics and Space Administration
CERES ERBE-like Footprint TOA Fluxes (ES8) NPP-FM5 Edition2

The ERBE-like Footprint TOA Fluxes (ES-8) product contains 24 hours of instantaneous Clouds and the Earth's Radiant Energy System (CERES) data for a single scanner instrument, Flight Model 5 (FM5) on the Suomi NPP spacecraft. The ES-8 contains filtered radiances recorded every 0.01-second for the total (TOT), shortwave (SW), and window (WN) channels and the unfiltered SW, longwave (LW), and WN radiances. The SW and LW radiances at spacecraft altitude are converted to Top-of-the-Atmosphere (TOA) fluxes with a scene identification algorithm and Angular Distribution Models (ADMs), which are "like" those used for the Earth Radiation Budget Experiment (ERBE). The TOA fluxes, scene identification, and angular geometry are included in the ES-8. CERES is a key Earth Observing System (EOS) program component. The CERES instruments provide radiometric measurements of the Earth's atmosphere from three broadband channels. The CERES missions follow the successful Earth Radiation Budget Experiment (ERBE) mission. The first CERES instrument (PFM) was launched on November 27, 1997, as part of the Tropical Rainfall Measuring Mission (TRMM). Two CERES instruments (FM1 and FM2) were launched into polar orbit on board the EOS flagship Terra on December 18, 1999. Two additional CERES instruments (FM3 and FM4) were launched on board EOS Aqua on May 4, 2002. The CERES instrument (FM5) was launched on board the Suomi National Polar-orbiting Partnership (NPP) satellite on October 28, 2011. The last CERES instrument (FM6) was launched on board the Joint Polar Satellite System 1 (JPSS-1) satellite on November 18, 2017.

Tags: earth-science-atmospheric-radiation-atmosphere-longwave-radiation, earth-science-atmospheric-radiation-atmosphere-outgoing-longwave-radiation, earth-science-atmospheric-radiation-atmosphere-radiative-flux, earth-science-atmospheric-radiation-atmosphere-shortwave-radiation
Organization: National Aeronautics and Space Administration
MARS EXPRESS ASPERA-3 CAL RDR ELECTRON SPECTROMTR EXT2 V1.0

This data set contains calibrated Mars Express ASPERA-3         Electron Spectrometer (ELS) data for the second mission         extension (October 1, 2007 - May 31, 2009).  These data         are provided in units of Differential Number Flux (DNF):         cnts/(cm**2-sr-sec-eV)

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Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSIWAC 4 PRL-MTP005 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 2014-07-02T08:35:00.000 to 2014-08-01T09:59:59.000. 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
NEW HORIZONS MVIC KEM1 RAW V6.0

This data set contains Raw data taken by the New Horizons Multispectral Visible Imaging Camera instrument during the KEM1 ENCOUNTER mission phase. This is VERSION 6.0 of this data set. This version includes data acquired by the spacecraft between 08/14/2018 and 04/30/2022. It only includes data downlinked before 05/01/2022. Future datasets may include more data acquired by the spacecraft after 08/13/2018 but downlinked after 04/30/2022. The data includes functional tests and images during the approach and departure of Arrokoth. A look back at Pluto was also performed after the Arrokoth flyby. A Color Scan of Neptune and Uranus was done along with a Solar Star Calibration and Radiometric Calibration.

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Organization: National Aeronautics and Space Administration
Voyager 2 Uranus Plasma Wave Spectrometer (PWS) Resampled Spectrum Analyzer, Version 1.0, 48 s Summary Data

* Data Set Overview\n* =================\n\nThis Data Set consists of 48 s calibrated, averaged Wave Electric Field Intensities from the Voyager 2 Plasma Wave Receiver Spectrum Analyzer obtained in the Vicinity of the Uranian Magnetosphere. For each 48 s Interval, a geometric average Field Strength is determined for each of the 16 Spectrum Analyzer Channels whose Center Frequencies range from 10 Hz to 56.2 kHz and which are logarithmically spaced in Frequency, four Channels per Decade. The Time associated with each Set of Averages is the Beginning of the Averaging Interval. Averages are stored in Units of V/m. During Data Gaps where complete 48 s Intervals are missing, no Entries exist in the File, that is, the Gaps are not Zero-filled or Tagged in any other way. Additional Information about this Data Set and the Instrument which produced it can be found elsewhere in this Catalog. An Overview of the Data in this Data Set can be found in (Gurnett et al., 1986) and a complete Instrument Description can be found in (Scarf and Gurnett, 1977).\n\n+-------------------------------------------------------+\n| Parameter Characteristics      | Value                |\n---------------------------------------------------------\n| Sampling Parameter Name        | TIME                 |\n| Data Set Parameter Name        | PLASMA WAVE SPECTRUM |\n| Sampling Parameter Resolution  | 48.000000            |\n| Sampling Parameter Interval    | 48.000000            |\n| Minimum Sampling Parameter     | 197708201553.000000  |\n| Minimum Available Sampling Int | 4.000000             |\n| Data Set Parameter Unit        | VOLT/METER           |\n| Noise Level                    | 0.000005             |\n| Sampling Parameter Unit        | SECOND               |\n+-------------------------------------------------------+

Tags: waves-passive
Organization: National Aeronautics and Space Administration
ODYSSEY MARS MARIE CALIBRATED DATA V1.0

The MARIE (Martian Radiation Environment Experiment) aboard the 2001       Mars Odyssey spacecraft, was launched on April 7, 2001 and arrived at       Mars on October 24, 2001.  Data were collected intermittently during       the cruise phase, starting in late April and ending in late July.  A       problem with MARIE&apos;s onboard computer occurred in early August and       the instrument was turned off until early March 2002, after       Odyssey&apos;s mapping orbit had been established.  Data have been       collected from that time to the present without major interruption.       Routine minor interruptions of up to 36 hours have occurred during the       orbital phase, in which the instrument&apos;s data is erased from the       local storage (after having been downloaded).  MARIE is oriented to       point in the direction opposite Odyssey&apos;s velocity vector.  Space       radiation is for most part isotropic, so the orientation of Odyssey is       usually not critical and references to external coordinate systems are       not a part of the data returned by MARIE.  There is one exception to       the statement that space radiation is isotropic.  During the early       stages of solar particle events, there can be directionality in the       particle flux.

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

ACE linearly interpolated to have the measurements on the minute at 60 s resolution tri-axial fluxgate magnetometer data in GSE coordinates. This data set consists of processed solar wind data that has been linearly interpolated to 1 min resolution at the position of the spacecraft using the interp1.m function in MATLAB. This data set was originally constructed by Dr. J.M. Weygand for Prof. R.L. McPherron, who was the principle investigator of two National Science Foundation studies: GEM Grant ATM 02-1798 and a Space Weather Grant ATM 02-08501. These data were primarily used in superposed epoch studies and cross correlation studies on solar wind.

Tags: ace, advanced-composition-explorer, magnetic-field, magneticfield-1-min, magnetometer, solar-wind
Organization: National Aeronautics and Space Administration
VOYAGER 2 SATURN PLASMA DERIVED ELECTRON                                      BROWSE 96 SEC

THIS DATA SET CONTAINS THE THERMAL          ELECTRON DENSITY AND TEMPERATURE IN THE PLS ENERGY RANGE          (10-5950 EV) FROM VOYAGER 2 AT SATURN DERIVED BY FITTING THE LOW          ENERGY ELECTRON COMPONENT WITH A  MAXWELLIAN DISTRIBUTION, AND THE          MOMENT DENSITY AND TEMPERATURE OF THE HOT ELECTRONS CALCULATED AFTER          THE SIGNAL FROM THE THERMAL COMPONENT IS SUBTRACTED FROM THE          ELECTRON SPECTRA.  IT IS A SUBSET OF THE DATA SET          VG2-S-PLS-5-ELE-FIT-96.0SEC WHICH SHOULD BE OBTAINED BEFORE THIS          DATA IS USED.  SPACECRAFT CHARGING MAY RESULT IN FACTOR OF 2-3          ERRORS IN THE THERMAL ELECTRON DENSITY.

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Organization: National Aeronautics and Space Administration
CERES Clouds and Radiative Swath Terra FM1 MODIS Edition4A

CER_CRS_Terra-FM1-MODIS_Edition4A is the Clouds and the Earth's Radiant Energy System (CERES) Clouds and Radiative Swath (CRS) Terra Flight Model 1 (FM1) Moderate-Resolution Imaging Spectroradiometer (MODIS) Edition4A data product, which was collected using the CERES-FM1 instrument on the Terra platform. Please note that only a few variables from the SSF have been included, and this product should be used in conjunction with the CER_SSF_Terra-FM1-MODIS_Edition4A product. The Clouds and Radiative Swath (CRS) product contains one hour of instantaneous CERES data for a single scanner instrument. The CRS contains geolocation, geometry, packet identification, minimal cloud properties, and TOA fluxes from the CERES SSF product. For each CERES footprint on the Single Scanner Footprint (SSF), the CRS product also contains vertical flux profiles evaluated at six levels in the atmosphere: the surface, 850-, 500-, 200-, 70-, and 0.01-hPa for both clear-sky and total-sky. CERES is a key Earth Observing System (EOS) program component. The CERES instruments provide radiometric measurements of the Earth's atmosphere from three broadband channels. The CERES missions follow the successful Earth Radiation Budget Experiment (ERBE) mission. The first CERES instrument, the protoflight model (PFM), was launched on November 27, 1997, as part of the Tropical Rainfall Measuring Mission (TRMM). Two CERES instruments (FM1 and FM2) were launched into polar orbit on board the Earth Observing System (EOS) flagship Terra on December 18, 1999. Two additional CERES instruments (FM3 and FM4) were launched on board Earth Observing System (EOS) Aqua on May 4, 2002. The CERES FM5 instrument was launched on board the Suomi National Polar-orbiting Partnership (NPP) satellite on October 28, 2011. The newest CERES instrument (FM6) was launched on board the Joint Polar-Orbiting Satellite System 1 (JPSS-1) satellite, now called NOAA-20, on November 18, 2017.

Tags: earth-science-aerosols-atmosphere-aerosol-optical-depth-thickness, earth-science-atmospheric-radiation-atmosphere-albedo, earth-science-atmospheric-radiation-atmosphere-emissivity, earth-science-atmospheric-radiation-atmosphere-incoming-solar-radiation, earth-science-atmospheric-radiation-atmosphere-longwave-radiation, earth-science-atmospheric-radiation-atmosphere-net-radiation, earth-science-atmospheric-radiation-atmosphere-outgoing-longwave-radiation, earth-science-atmospheric-radiation-atmosphere-radiative-flux, earth-science-atmospheric-radiation-atmosphere-shortwave-radiation, earth-science-atmospheric-radiation-atmosphere-solar-irradiance, earth-science-atmospheric-temperature-atmosphere-surface-temperature-skin-temperature, earth-science-atmospheric-water-vapor-atmosphere-water-vapor-indicators-total-precipitable-wate, earth-science-clouds-atmosphere-cloud-microphysics-cloud-optical-depth-thickness, earth-science-clouds-atmosphere-cloud-properties-cloud-base-temperature, earth-science-clouds-atmosphere-cloud-properties-cloud-fraction, earth-science-surface-radiative-properties-land-surface
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER COMET PRELANDING OSIWAC 2 EDR MTP 007 V1.0

This data set contains raw EDR images acquired by the OSIRIS Wide AngleCamera during the prelanding phase of the Rosetta mission at the comet 67P,covering the period from 2014-09-02 to 2014-09-16.

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Organization: National Aeronautics and Space Administration