AndreaBozzo/ceres-open-data-index huggingface dataset:
MARS EXPRESS MARS MRS 1/2/3 EXTENDED MISSION 7 4126 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 2020-09-11T04:26:25.100 to 2020-09-11T04:48:33.500.

Tags: __
Organization: National Aeronautics and Space Administration
TIMED Global Ultraviolet Imager (GUVI) Airglow Flux 14-day Movies, at Wavelength 1304 Å in Mercator Projection

GUVI measures FUV Airglow in five Spectral Bands: the atomic HI Lyman-alpha Band, 121.6 nm, two atomic Oxygen OI Bands, 130.4 nm and 135.6 nm, and the molecular Nitrogen Lyman-Birge-Hopfield Short, LBHS, 141 to 152.8 nm, and Lyman-Birge-Hopfield Long, LBHL, 167.2 to 181.2 nm, Bands. The Cross-Track Scanning Spectrograph images a Ground Swath of 3000 km Width providing nearly Contiguous Global Coverage with 15 Orbits per Day. This L1CDisk, Level 1C Disk, Version 3, File provides the calibrated, geolocated, and rectified Intensities for the second OI, 1304 Å, Wavelength Band. This is a Movie with mapped Images of the Log Intensities by Orbit by using a Transverse Mercator Projection.

Tags: imageintensity
Organization: National Aeronautics and Space Administration
MARS EXPRESS SUN MRS 1/2/3 EXTENDED MISSION 8 4226 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 Solar Conjunction measurement and covers the time 2021-09-21T03:28:33.000 to 2021-09-21T06:49:25.500.

Tags: __
Organization: National Aeronautics and Space Administration
MARS EXPRESS ASPERA-3 RAW EDR ELECTRON SPECTROMTR EXT2 V1.0

This data set contains Mars Express ASPERA-3 Electron         Spectrometer (ELS) data for the second mission extension         (October 1, 2007 - May 31, 2009). These data are provided         in raw units of counts/accumulation.

Tags: __
Organization: National Aeronautics and Space Administration
TIMED Global Ultraviolet Imager (GUVI) Airglow Flux 14-day Movies, at Wavelength 1304 Å in South Polar Projection

GUVI measures FUV Airglow in five Spectral Bands: the atomic HI Lyman-alpha Band, 121.6 nm, two atomic Oxygen OI Bands, 130.4 nm and 135.6 nm, and the molecular Nitrogen Lyman-Birge-Hopfield Short, LBHS, 141 to 152.8 nm, and Lyman-Birge-Hopfield Long, LBHL, 167.2 to 181.2 nm, Bands. The Cross-Track Scanning Spectrograph images a Ground Swath of 3000 km Width providing nearly Contiguous Global Coverage with 15 Orbits per Day. This L1CDisk, Level 1C Disk, Version 3, File provides the calibrated, geolocated, and rectified Intensities for the second OI, 1304 Å, Wavelength Band. This is a Movie with mapped Images of the Log Intensities by Orbit by using a South Polar Projection.

Tags: imageintensity
Organization: National Aeronautics and Space Administration
MARS EXPRESS ASPERA-3 CAL RDR ELECTRON SPECTROMTR EXT5 V1.0

This data set contains calibrated Mars Express ASPERA-3         Electron Spectrometer (ELS) data for the fifth mission         extension (January 1, 2015 - Dec. 31, 2016).  These data         are provided in units of Differential Number Flux (DNF):         cnts/(cm**2-sr-sec-eV)

Tags: __
Organization: National Aeronautics and Space Administration
PSP FIELDS Digital Fields Board (DFB) DC-coupled Single Ended Voltage Waveform, Monopole Mode, Level 2 (L2), PT0.027306S Data

PSP FIELDS Digital Fields Board, DFB, Single Ended Voltage data:\n\nThe DFB is the low frequency, less than 75 kHz, component of the FIELDS experiment on the Parker Solar Probe spacecraft, see reference [1] below. For a full description of the FIELDS experiment, see reference [2]. For a description of the DFB, see reference [3].\n\nThe DFB continuous waveform data consist of time series data from various FIELDS sensors. These data have been filtered by both analog and digital filters [3].\n\nThe Level 2 data products contained in this data file have been calibrated for:\n\n* 1) DFB in-band gain\n* 2) DFB analog filter gain and phase response\n* 3) DFB digital filter phase response\n* 4) The search coil preamplifier gain and phase response, when applicable\n\nCalibrations for the DFB digital filter gain response have not been implemented, but the required convolution kernel is provided in this file. It was decided not to apply the digital filter gain response calibration to these Level 2 data because the application of the calibrations can introduce non-physical power at high frequencies when the non-corrected signal is dominated by noise. This effect should be examined carefully when determining spectral slopes and features at the highest frequencies. Calibrations for the FIELDS voltage sensor preamplifiers have not been implemented as the preamplifier response is flat and equal to one throughout the DFB frequency range. Corrections for plasma sheath impedance gain and antenna effective length have not been applied to the voltage sensor data. These corrections will be applied in the Level 3 DFB data products. Therefore, all voltage sensor quantities when present in these Level 2 data products are expressed by using units of Volts. Likewise, all magnetic field quantities when present in these Level 2 data products are expressed by using units of nanoTelsas.\n\nThe Level 2 data products contained in this data file are in spacecraft coordinates (e.g. x,y,z) or in sensor coordinates (e.g. dV12, dV34 for voltage measurements and [u,v,w] for the searchcoil magnetometer.\n\nThe time resolution of the DFB continuous waveform data can vary by multiples of 2^N. During encounter when PSP is within 0.25 AU of the Sun, the DFB continuous waveform data cadence is typically 256 samples/NYsecond [2].\n\nReferences:\n\n* 1) Fox, N.J., Velli, M.C., Bale, S.D. et al., Space Sci Rev (2016) 204:7. https://doi.org/10.1007/s1121401502116\n* 2) Bale, S.D., Goetz, K., Harvey, P.R. et al., Space Sci Rev (2016) 204:49. https://doi.org/10.1007/s1121401602445\n* 3) Malaspina, D.M., Ergun, R.E., Bolton, M. et al., JGR Space Physics (2016), 121, 5088-5096. https://doi.org/10.1002/2016JA022344

Tags: electricfield, instrumentstatus
Organization: National Aeronautics and Space Administration
TIMED Global Ultraviolet Imager (GUVI) Airglow Flux 14-day Movies, at Wavelength 1304 Å in North Polar Projection

GUVI measures FUV Airglow in five Spectral Bands: the atomic HI Lyman-alpha Band, 121.6 nm, two atomic Oxygen OI Bands, 130.4 nm and 135.6 nm, and the molecular Nitrogen Lyman-Birge-Hopfield Short, LBHS, 141 to 152.8 nm, and Lyman-Birge-Hopfield Long, LBHL, 167.2 to 181.2 nm, Bands. The Cross-Track Scanning Spectrograph images a Ground Swath of 3000 km Width providing nearly Contiguous Global Coverage with 15 Orbits per Day. This L1CDisk, Level 1C Disk, Version 3, File provides the calibrated, geolocated, and rectified Intensities for the second OI, 1304 Å, Wavelength Band. This is a Movie with mapped Images of the Log Intensities by Orbit by using a North Polar Projection.

Tags: imageintensity
Organization: National Aeronautics and Space Administration
TIMED Global Ultraviolet Imager (GUVI) Airglow Flux 14-day Movies, at Wavelength 1356 Å in Mercator Projection

GUVI measures FUV Airglow in five Spectral Bands: the atomic HI Lyman-alpha Band, 121.6 nm, two atomic Oxygen OI Bands, 130.4 nm and 135.6 nm, and the molecular Nitrogen Lyman-Birge-Hopfield Short, LBHS, 141 to 152.8 nm, and Lyman-Birge-Hopfield Long, LBHL, 167.2 to 181.2 nm, Bands. The Cross-Track Scanning Spectrograph images a Ground Swath of 3000 km Width providing nearly Contiguous Global Coverage with 15 Orbits per Day. This L1CDisk, Level 1C Disk, Version 3, File provides the calibrated, geolocated, and rectified Intensities for the third OI, 1356 Å, Wavelength Band. This is a Movie with mapped Images of the Log Intensities by Orbit by using a Transverse Mercator Projection.

Tags: imageintensity
Organization: National Aeronautics and Space Administration
TIMED Sounding of the Atmosphere using Broadband Emission Radiometry (SABER)IR Radiances in 10 channels (1.27 to 17ym) from 0 to 150 km, Version 1.07, Level 1B (L1B), 42 s Data

Contains the SABER Level 1B calibrated radiance profiles converted to radiance units with instrument effects removed, geolocated and gridded to uniform angle spacing.

Tags: lower-thermosphere, mesosphere, mlti, profile-timed, radiance, saber
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 1 0612 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 2015-02-28T22:34:15.000 to 2015-03-01T07:54:09.000.

Tags: __
Organization: National Aeronautics and Space Administration
PSP FIELDS Digital Fields Board (DFB) Searchcoil Magnetometer Waveform, Level 2 (L2), 3.413 ms Data

PSP FIELDS Digital Fields Board, DFB, Search Coil Magnetometer data:\n\nThe DFB is the low frequency, less than 75 kHz, component of the FIELDS experiment on the Parker Solar Probe spacecraft, see reference [1] below. For a full description of the FIELDS experiment, see reference [2]. For a description of the DFB, see reference [3].\n\nThe DFB continuous waveform data consist of time series data from various FIELDS sensors. These data have been filtered by both analog and digital filters [3].\n\nThe Level 2 data products contained in this data file have been calibrated for:\n\n* 1) DFB in-band gain\n* 2) DFB analog filter gain and phase response\n* 3) DFB digital filter phase response\n* 4) The search coil preamplifier gain and phase response, when applicable\n\nCalibrations for the DFB digital filter gain response have not been implemented, but the required convolution kernel is provided in this file. It was decided not to apply the digital filter gain response calibration to these Level 2 data because the application of the calibrations can introduce non-physical power at high frequencies when the non-corrected signal is dominated by noise. This effect should be examined carefully when determining spectral slopes and features at the highest frequencies. Calibrations for the FIELDS voltage sensor preamplifiers have not been implemented as the preamplifier response is flat and equal to one throughout the DFB frequency range. Corrections for plasma sheath impedance gain and antenna effective length have not been applied to the voltage sensor data. These corrections will be applied in the Level 3 DFB data products. Therefore, all voltage sensor quantities when present in these Level 2 data products are expressed by using units of Volts. Likewise, all magnetic field quantities when present in these Level 2 data products are expressed by using units of nanoTelsas.\n\nThe Level 2 data products contained in this data file are in spacecraft coordinates (e.g. x,y,z) or in sensor coordinates (e.g. dV12, dV34 for voltage measurements and [u,v,w] for the searchcoil magnetometer.\n\nThe time resolution of the DFB continuous waveform data can vary by multiples of 2^N. During encounter when PSP is within 0.25 AU of the Sun, the DFB continuous waveform data cadence is typically 256 samples/NYsecond [2].\n\nReferences:\n\n* 1) Fox, N.J., Velli, M.C., Bale, S.D. et al., Space Sci Rev (2016) 204:7. https://doi.org/10.1007/s1121401502116\n* 2) Bale, S.D., Goetz, K., Harvey, P.R. et al., Space Sci Rev (2016) 204:49. https://doi.org/10.1007/s1121401602445\n* 3) Malaspina, D.M., Ergun, R.E., Bolton, M. et al., JGR Space Physics (2016), 121, 5088-5096. https://doi.org/10.1002/2016JA022344

Tags: instrumentstatus, magneticfield
Organization: National Aeronautics and Space Administration
TIMED Global Ultraviolet Imager (GUVI) Airglow Flux 14-day Movies, at Wavelength LBH1 in Mercator Projection

GUVI measures FUV Airglow in five Spectral Bands: the atomic HI Lyman-alpha Band, 121.6 nm, two atomic Oxygen OI Bands, 130.4 nm and 135.6 nm, and the molecular Nitrogen Lyman-Birge-Hopfield Short, LBHS, 141 to 152.8 nm, and Lyman-Birge-Hopfield Long, LBHL, 167.2 to 181.2 nm, Bands. The Cross-Track Scanning Spectrograph images a Ground Swath of 3000 km Width providing nearly Contiguous Global Coverage with 15 Orbits per Day. This L1CDisk, Level 1C Disk, Version 3, File provides the calibrated, geolocated, and rectified Intensities for the fourth LBH1, 1400-1500 Å, Wavelength Band. This is a Movie with mapped Images of the Log Intensities by Orbit by using a Transverse Mercator Projection.

Tags: imageintensity
Organization: National Aeronautics and Space Administration
CASSINI SS/S RPWS CALIBRATED LP CONTINUOUS CURRENT V1.0

The Cassini Radio and Plasma Wave Science (RPWS) Langmuir Probe      continuous current data set comprises calibrated probe current      measurements acquired up to 20 Hz rate at fixed bias voltage during the      entire Cassini mission.  These currents can be used to infer high      temporal  resolution density fluctuations between standard Langmuir      Probe sweeps.  If related to densities determined during a sweep prior      to or following the 20 Hz data, or using other electron density      estimates, the relative currents can be  assigned absolute densities.      Data are presented in text tables and are organized so as to have      fixed-length records for ease in data handling.

Tags: __
Organization: National Aeronautics and Space Administration
TIMED Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) O₃, CO₂, and H₂O Mixing Ratios, O, O₂, OH, and NO Volume Emission Rates, and also National Meteorological Center, NMC, Neutral Temperature Density, and Pressure, Version 2.0, Level 2A (L2A), 42 s Data

Contains SABER Level 1 spectra that have been processed into vertical profiles of geophysical quantities on a uniform altitude grid. These vertical profiles are at the highest available horizontal and temporal resolution. Routine products include profiles of temperature (kelvin), pressure (milibars), CO2, O3, H2O, and the volume emission rates (ergs/cm^3/sec).

Tags: lower-thermosphere, mesosphere, mlti, profile-timed, saber
Organization: National Aeronautics and Space Administration
MARS EXPRESS ASPERA-3 RAW-CAL NTRL PARTICLE IMAGER EXT3 V1.0

This data set contains Mars Express ASPERA-3 Neutral         Particle Imager (NPI) data for the third mission extension         (January 1, 2010 - Dec. 31, 2012).  These data are provided         in units of count rate (counts/second).

Tags: __
Organization: National Aeronautics and Space Administration
TIMED SEE Level2 EGS Solar Irradiance Data

The EUV Grating Spectrograph (EGS) aboard SEE performs measurements of the Sun for about 3 minutes every orbit (97 minutes) which usually gives 14-15 measurements per day. The Level 2 data is time averaged over the entire day, after being 1-AU corrected and removing flares. The 1-AU correction is provided.

Tags: egs, irradiance-timed, see, sun
Organization: National Aeronautics and Space Administration
TIMED Global Ultraviolet Imager (GUVI) Airglow Flux 14-day Movies, at Wavelength LBH2 in Mercator Projection

GUVI measures FUV Airglow in five Spectral Bands: the atomic HI Lyman-alpha Band, 121.6 nm, two atomic Oxygen OI Bands, 130.4 nm and 135.6 nm, and the molecular Nitrogen Lyman-Birge-Hopfield Short, LBHS, 141 to 152.8 nm, and Lyman-Birge-Hopfield Long, LBHL, 167.2 to 181.2 nm, Bands. The Cross-Track Scanning Spectrograph images a Ground Swath of 3000 km Width providing nearly Contiguous Global Coverage with 15 Orbits per Day. This L1CDisk, Level 1C Disk, Version 3, File provides the calibrated, geolocated, and rectified Intensities for the fifth LBH2, 1650-1800 Å, Wavelength Band. This is a Movie with mapped Images of the Log Intensities by Orbit by using a Transverse Mercator Projection.

Tags: imageintensity
Organization: National Aeronautics and Space Administration
TIMED SEE Level2 XPS Solar Irradiance Data

The 12 X-Ray Photometers (XP) aboard SEE perform full-disk irradiance measurements of the Sun for about 3 minutes every orbit (97 minutes) which usually gives 14-15 measurements per day. 8 of the XPs produce XUV signals (more info on XP coatings) and one other XP provides a hydrogen Lyman-alpha measurement (121.5 nm). The XPS Level 2 data is time averaged over the entire day, after being 1-AU corrected and removing flares. The 1-AU correction is provided.

Tags: irradiance-timed, see, sun, xps
Organization: National Aeronautics and Space Administration
TIMED SEE Level2A XPS Solar Irradiance Data

The 12 X-Ray Photometers (XP) aboard SEE perform full-disk irradiance measurements of the Sun for about 3 minutes every orbit (97 minutes) which usually gives 14-15 measurements per day. 8 of the XPs produce XUV signals (more info on XP coatings) and one other XP provides a hydrogen Lyman-alpha measurement (121.5 nm). The XPS Level 2A data is time averaged over each measurement, after being 1-AU corrected and removing flares. The 1-AU correction is provided.

Tags: irradiance-timed, see, sun, xps
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 ROSETTA EXTENSION 1 1360 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 2016-01-21T07:54:35.000 to 2016-01-21T13:47:37.500.

Tags: __
Organization: National Aeronautics and Space Administration
Chlorophyll time series, Department of Fisheries and Oceans (DFO), Canada

This time series of chl data was obtained from the BioChem archive run by the Department of Fisheries and Oceans, Canada. Water sampling and chlorophyll analysis methods are described in the Mitchell et al. (2002) protocol document accompanying the data.DFO (2014). BioChem: database of biological and chemical oceanographic data. Department of Fisheries and Oceans, Canada.http://isdm.gc.ca/biochem/biochem-eng.htm

Tags: earth-science-ocean-chemistry-oceans, earth-science-ocean-optics-oceans, earth-science-ocean-temperature-oceans, earth-science-salinity-density-oceans
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSINAC 4 ESC3-MTP019 RDR V2.0

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 on the Rosetta spacecraft during the COMET ESCORT 3 mission phase, covering the period from 2015-07-28T23:25:00.000 to 2015-08-25T23:24:59.000. The prime target is comet 67P/Churyumov-Gerasimenko 1 (1969 R1). This version V2.0 supersedes previous deliveries of the same dataset with the following changes since the last version: Lien corrected dataset after October 2018 PSA/PDS external peer review. 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.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER STEINS OSINAC 4 AST1 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 on the Rosetta spacecraft  during the STEINS FLY-BY mission phase, covering the period  from 2008-08-04T00:00:00.000 to 2008-10-05T23:59:59.000. The prime target is asteroid 2867 Steins. This version V1.0 is the first version of this dataset.

Tags: __
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 2 0687 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 2015-04-01T13:59:55.000 to 2015-04-01T15:38:20.500.

Tags: __
Organization: National Aeronautics and Space Administration
ULYSSES JUPITER HISCALE LEMS 30 ION COUNTS

This data set consists of HISCALE                                      Low-Energy Magnetic Spectrometer                                      (LEFS) ion counts at 30 degrees from                                      the spacecraft spin axis. These                                      measurements were taken during the                                      Ulysses Jupiter encounter 1991-12-31                                      to 1992-02-16, and include 1 hour                                      averaged inbound cruise data                                      (1991-12-31 to 1992-02-01), and 15                                      minute averaged encounter data                                      (1992-02-02 to 1992-02-16).

Tags: __
Organization: National Aeronautics and Space Administration
TWINS 1 Neutral-atom L1 Images and Movies

TWINS 1 neutral-atom spectrometer level-1 magnetospheric images and image movies at full (9 energy steps and 15 minute) resolution. Images have been smoothed using a technique that provides approximately uniform statistics across the image. Each image has 4x4 degree angular resolution and includes 15 minutes of data. These images are derived on the ground from direct events measurements of the time of flight and detection location on the anode for individual ENAs. Each image has 4x4 degree angular resolution and includes 15 minutes of data. The first dimension of the image represents the scan angle in instrument coordinates. In this system the azimuthal attitude vector points to +90 degree scan angle. The second is the imaged angle, where 90 degrees is the central viewing angle of the instrument and the direction of the polar attitude vector.

Tags: neutralatomimages
Organization: National Aeronautics and Space Administration
TWINS-1 Ephemeris, Definitive Spacecraft Attitude, PT0.512S Data

Two Wide-angle Imaging Neutral-atom Spectrometers 1, TWINS 1, Spacecraft Attitude data, Earth Centered Inertial, ECI, coordinates. This TWINS data set contains spacecraft attitude data as polar and azimuthal instrument pointing vectors. The polar vector points along the TWINS rotation axis. The azimuthal vector lies in the plane normal to the polar vector and points toward the central scanning position, which is defined as the zero-point location. Such pointing is derived from both the spacecraft attitude history, SAH, file and the sensor mounting orientation. The computation employed is designed to achieve a pointing accuracy of 0.5°. Any deviation from this accuracy level is indicated in the header record metadata.

Tags: ephemeris
Organization: National Aeronautics and Space Administration