AndreaBozzo/ceres-open-data-index huggingface dataset:
PSP FIELDS Digital Fields Board (DFB) AC-coupled Differential Voltage, V1-V2 Antennae, Dipole Mode, Bandpass filtered, High Gain, Sensor coordinates, Level 2 (L2), 0.873813 s Data

PSP FIELDS Digital Fields Board, DFB, dV12 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\nDFB AC bandpass data consist of peak and average values of the absolute value of bandpassed time series waveform data over a time interval equal to the reporting cadence. The AC bandpass data have the peak response frequency of each bin reported in the metadata. The frequency response curves for these bins are given in [3].\n\nThe Level 2 data products contained in this data file have been calibrated for:\n\n* 1) The ~6.3 dB loss associated with forming the bandpass signal, see reference [3]\n* 2) DFB in-band gain\n* 3) The search coil preamplifier response, when applicable\n\nCalibrations for the DFB digital filter gains and analog filter gains have not been implemented as it was determined that these could not be applied accurately to single numerical values representing a broadband signal response and because all bins except the highest frequency bin have a flat gain response equal to one due to these filters. Calibrations for the FIELDS preamplifiers have not been implemented as the preamplifier response is flat and equal to one through the DFB frequency range. Corrections for plasma sheath impedance gain and antenna effective length have not been applied to voltage sensor signals. 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 expressed 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 AC bandpass filtered data can vary by multiples of 2^N. During encounter when PSP is within 0.25 AU of the Sun, the DFB AC bandpass filtered data cadence is typically 1/8 of a NYsecond [2]. Timestamps correspond to the center time of each window.\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, waves-passive
Organization: National Aeronautics and Space Administration
Qeqertarsuaq (GDH) Ground-based Vector Magnetic Field (L2) 1.0 min Data

Qeqertarsuaq, Greenland, Ground-based Vector Magnetic Field Level 2 Data, 1.0 min Time Resolution, Station Code: (GDH), Station Location: (GEO Latitude 69.3, Longitude 306.5), DTU Network

Tags: magneticfield
Organization: National Aeronautics and Space Administration
SAKIGAKE INTERPLANETARY MAGNETIC FIELD DATA V 1.0

The original Data Set Name was MST5IMF. The data was delivered personally by Oyama. The component values indicate a crossing of the neutral sheet. The magnetic field is defined in terms of solar ecliptic coordinates with spacecraft at the center and the x direction positive towards the Sun, the y direction in the ecliptic plane, and the z direction given by a left handed coordinate system. A total force value is also given.

Tags: __
Organization: National Aeronautics and Space Administration
Ranua (RAN) Ground-based Vector Magnetic Field (L2) 10.0 s Data

Ranua, Finland, Ground-based Vector Magnetic Field Level 2 Data, 10.0 s Time Resolution, Station Code: (RAN), Station Location: (GEO Latitude 65.9, Longitude 26.4), IMAGE Network

Tags: magneticfield
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 1 0457 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 2014-11-25T13:35:10.000 to 2014-11-25T20:10:55.000.

Tags: __
Organization: National Aeronautics and Space Administration
PSP FIELDS Digital Fields Board (DFB) Searchcoil Magnetometer, SCM, Burst Waveform, Level 2 (L2), 0.873813 s Data

PSP FIELDS Digital Fields Board (DFB), Differential 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\nDFB burst waveform data consist of short bursts of time-series data from various FIELDS sensors. These data have been filtered by both analog and digital filters [3]. These data are pre-sorted by onboard competitive selection algorithms described in [3] before storage by FIELDS. A subset of this stored burst data is telemetered to Earth for scientist-selected regions of interest.\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/phase response\n* 3) DFB digital filter phase response\n* 4) The search coil preamplifier gain/phase response, when applicable\n\nCalibrations for the FIELDS voltage sensor preamplifiers have not been implemented as the preamplifier response is flat and equal to one through the DFB frequency range. Corrections for plasma sheath impedance gain and antenna effective length have not been applied to voltage sensor signals. 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 nT.\n\nThe Level 2 voltage data products when present in these data files are expressed in sensor coordinates: [dV12,dV34] for voltage measurements. Likewise, the Level 2 search coil magnetomete data products when present in these data files are expressed in sensor coordinates: [u,v,w] for magnetic field measurements.\n\nThe time resolution of the DFB burst waveform data can vary by multiples of 2^N. During encounter when PSP is within 0.25 AU of the Sun, the DFB burst waveform data cadence is typically 150,000 samples/s. This rate is the sample rate of the analog to digital converters, ADC, and data taken at this rate do not pass through a digital filter.\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 Phys. (2016), 121, 5088-5096. https://doi.org/10.1002/2016JA022344

Tags: instrumentstatus, magneticfield
Organization: National Aeronautics and Space Administration
Remus (RMUS) Ground-based Vector Magnetic Field (L2) 0.5 s Data

Remus, MI, Ground-based Vector Magnetic Field Level 2 Data, 0.5 s Time Resolution, Station Code: (RMUS), Station Location: (GEO Latitude 43.6, Longitude 274.8), THEMIS EPO/UCLA Network

Tags: magneticfield
Organization: National Aeronautics and Space Administration
VG2 JUP CRS DERIVEDPROTON/ION/ELECTRON FLUX BROWSE V1.0

The Cosmic Ray Subsystem (CRS) was      designed for cosmic ray studies. It consists      of two high Energy Telescopes (HET), four Low Energy      Telescopes (LET) and The Electron Telescope (TET). The      detectors have large geometric factors (~ 0.48 to 8 cm^2 ster)      and long electronic time constants (~ 24 [micro]sec) for low      power consumption and good stability. Normally, the data are      primarily derived from comprehensive ([Delta]E[1], [Delta]E[2]      and E) pulse-height information about individual events.      Because of the high particle fluxes encountered at Jupiter and      Saturn, greater reliance had to be placed on counting rates in      single detectors and various coincidence rates. In inter-      planetary space, guard counters are placed in anticoincidence      with the primary detectors to reduce the background from      high-energy particles penetrating through the sides of the      telescopes. These guard counters were turned off in the Jovian      magnetosphere when the accidental anticoincidence rate became      high enough to block a substantial fraction of the desired      counts. Fortunately, under these conditions the spectra were      sufficiently soft that the background, due to penetrating      particles, was small.

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

THEMIS Ground All Sky Imager at Prince George (53.82 deg GLat, 237.17 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
VG2 SAT MAG RESAMPLED KRONOGRAPHIC (L1)                                     COORDS 9.6SEC V1.1

This data set includes Voyager 2 Saturn      encounter magnetometer data from the Low Field Magnetometer (LFM)      resampled at a 9.6 second sample rate from the 60 msec instrument      sampling rate. Data coverage begins in the solar wind and continues      until at least the first magnetopause crossing. The data are given in      Kronographic (L1) coordinates. The data set is composed of the following      columns: 1) time - UT of the sample in the format      yyyy-mm-ddThh:mm:ss.sssZ, 2) spacecraft clock values      (m65536:mod60:fds_line), 3) mag_id - magnetometer id (1 = LFM, 2 = HFM),      4) Br - radial (Saturn to spacecraft) B-field component, 5) Btheta -      North/South (L1) B-field component (positive southward), 6) Bphi -      azimuthal (L1) B-field component (positive eastward), 7) Bmag -      magnitude of the averaged magnetic field components, 8) avg_Bmag -      average of the magnetic field magnitudes, 9) delta - magnetic      latitude = arcsin(Btheta/Bmag), 10) lambda - longitude =      180. - atan(Bphi/-Br), 11-13) rms_br, rms_bt, and rms_bn - rms vectors,      14) npts - number of points in average.  All magnetic field observations      are measured in nanoTesla. All of the magnetic field data are calibrated      (see the instrument calibration description for more details).  These      data are provided in a Saturn centered spherical system (L1), based on      the Saturn Longitude System (Voyager Measurements of the Rotation Period      of Saturn's Magnetic Field, Desch and Kaiser, JGR, 8, 253, 1981).

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

THEMIS Ground All Sky Imager at Prince George (53.82 deg GLat, 237.17 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
ROSETTA-ORBITER/ROSETTA-LANDER CAL CONSERT 2 CVP1 V1.0

This archive contains edited data from the CONSERT instrument onboard ROSETTA Orbiter and Lander, acquired during the Commissioning 1 phase. It also contains documentation which describes the CONSERT experiment. The data archived in this data set conform to the Planetary Data System (PDS) Standards, Version 3.6. This data set supersedes RO/RL-CAL-CONSERT-2-CVP-V1.0.

Tags: __
Organization: National Aeronautics and Space Administration
Romo (ROE) Ground-based Vector Magnetic Field (L2) 1.0 min Data

Romo, Denmark, Ground-based Vector Magnetic Field Level 2 Data, 1.0 min Time Resolution, Station Code: (ROE), Station Location: (GEO Latitude 55.2, Longitude 8.6), DTU Network

Tags: magneticfield
Organization: National Aeronautics and Space Administration
THEMIS GBO All Sky Imager at Rankin Inlet, NU, Canada. ASI Thumbnails Data.

THEMIS Ground All Sky Imager at Rankin Inlet (62.82 deg GLat, 267.89 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
DAWN FC2 CALIBRATED CRUISE  CHECKOUT/CALIB IMAGES V1.0

Abstract  :  Framing Camera 2 is one of two identical units flying on Dawn  spacecraft. This dataset includes the Reduced Data Record (RDR) version  of all available images acquired during the initial checkout and  pre-Vesta cruise phases (Checkout, Earth to Mars, and Mars to Vesta).  As in the original raw data sets, in addition to the imagery, ancillary  information is stored within the image headers, as well as a detailed  account of all the reference files used for the calibration. Calibration files needed for further processing are archived as a separate data set.

Tags: __
Organization: National Aeronautics and Space Administration
Savissivik (SVS) Ground-based Vector Magnetic Field (L2) 20.0 s Data

Savissivik, Greenland, Ground-based Vector Magnetic Field Level 2 Data, 20.0 s Time Resolution, Station Code: (SVS), Station Location: (GEO Latitude 76.0, Longitude 294.9), DTU Network

Tags: magneticfield
Organization: National Aeronautics and Space Administration
GO EARTH EPD RESAMPLED SUMMARY EARTH2 15.0 MIN V1.0

This data set contains fifteen minute averaged rate               data for all 64 EPD channels.  The browse set covers               the Earth 2 encounnter data from 1992 Day 311               through day 353.  All available motor positions               except zero are included in the averages.

Tags: __
Organization: National Aeronautics and Space Administration
Ulysses High Resolution Magnetic Field Data

This data set contains high resolution samples at about one-second intervals of the interplanetary magnetic field measured by the Ulysses Magnetic Field experiment. Field vector components are given in units of nanoteslas and in RTN coordinates, where R is the sun-s/c axis, T is the cross product of the solar rotation axis and R, and T is the cross product of R and T. The field magnitudes in nT are averages of scalar magnitudes at higher time resolution. Times are computed at the mid-point of each averaging interval and expressed in Spacecraft Event Time - UT (SCET-UT). Data gaps have not been flagged in any way - if there were no available data in a particular hour then there is no data record for that hour. No data from the Feb. 1992 encounter with Jupiter are included. Each file includes one day of data. Parameter key information given below is specific to the data version at nssdcftp and at the ESA Research and Scientific Support Department site identified below. Further details on the magnetic field measurements can be found in the following reference: Balogh, A., et al., Astron. Astrophys. Suppl. Ser., 92(2), 221, 1992.

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

THEMIS Ground All Sky Imager at Snap Lake (63.58 deg GLat, 249.13 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
VG2 JUP MAG RESAMPLED SYSTEM III (1965)COORDS 9.60SEC V1.1

This data set includes Voyager 2 Jupiter     encounter magnetometer data from the Low Field Magnetometer (LFM)     resampled at a 9.6 second sample rate from the 60 msec instrument     sampling rate. Data coverage begins in the solar wind and continues     until at least the first magnetopause crossing. The data are given in     Jovicentric System III(1965) right handed coordinates. The data set is     composed of the following columns: 1) time - UT of the sample in the     format yyyy-mm-ddThh:mm:ss.sssZ, 2) spacecraft clock values     (m65536:mod60:fds_line), 3) mag_id - magnetometer id (1 = LFM, 2 = HFM),     4) Br - radial (Jupiter to spacecraft) B-field component, 5) Btheta -     North/South (system III) B-field component (positive southward),     6) Bphi - azimuthal (system III) B-field component (positive eastward),     7) Bmag - magnitude of the averaged magnetic field components,     8) avg_Bmag - average of the magnetic field magnitudes, 9) delta -     magnetic latitude = arcsin(Btheta/Bmag), 10) lambda - longitude =     180. - atan(Bphi/-Br), 11-13) rms_br, rms_bt, and rms_bn - rms vectors,     14) npts - number of points in average.  All magnetic field     observations are measured in nanoTesla. All of the magnetic field     data are calibrated (see the instrument calibration description for     more details).

Tags: __
Organization: National Aeronautics and Space Administration
Tiksi (TIK) Ground-based Vector Magnetic Field (L2) 1.0 min Data

Tiksi, Russia, Ground-based Vector Magnetic Field Level 2 Data, 1.0 min Time Resolution, Station Code: (TIK), Station Location: (GEO Latitude 71.6, Longitude 128.9), AARI Network

Tags: magneticfield
Organization: National Aeronautics and Space Administration
CH3D ICE ABSORPTION COEFFICIENTS V1.0

This data set is the result of laboratory transmission spectroscopy experiments performed within a sealed cell in the ice laboratory at Northern Arizona University. We record spectra at wavelengths from 1 to 6 microns to study CH3D bands at 2.47, 2.87, and 4.56 microns (as indicated by '25', '29' and '45' in the data file names). We report temperature-dependent absorption coefficients of these bands when the CH3D is diluted in CH4 ice and also when it is dissolved in N2 ice. These absorption coefficient spectra can be combined with data from the literature to simulate arbitrary D/H ratio absorption coefficients for CH4 ice and for CH4 in N2 ice. The data were originally published in 2011 in Icarus, vol. 212, pp. 941-949, and that paper should be consulted for details about laboratory procedures and limitations of the data.

Tags: __
Organization: National Aeronautics and Space Administration
Trapper Creek (TRAP) Ground-based Vector Magnetic Field (L2) 0.5 s Data

Trapper Creek, AK, Ground-based Vector Magnetic Field Level 2 Data, 0.5 s Time Resolution, Station Code: (TRAP), Station Location: (GEO Latitude 62.3, Longitude 209.8), University of Alaska Network

Tags: magneticfield
Organization: National Aeronautics and Space Administration
CATS-ISS Level 1B Day Mode 7.2 Version 3-00

CATS-ISS_L1B_D-M7.2-V3-00 is the Cloud-Aerosol Transport System (CATS) International Space Station (ISS) Level 1B Day Mode 7.2 Version 3-00 data product. This collection spans from March 25, 2015 to October 29, 2017. CATS, which was launched on January 10, 2015, was a lidar remote sensing instrument that provided range-resolved profile measurements of atmospheric aerosols and clouds from the ISS. CATS was intended to operate on-orbit for up to three years. CATS provides vertical profiles at three wavelengths, orbiting between ~230 and ~270 miles above the Earth's surface at a 51-degree inclination with nearly a three-day repeat cycle. For the first time, scientists were able to study diurnal (day-to-night) changes in cloud and aerosol effects from space by observing the same spot on Earth at different times each day. CATS Level 2 Layer data products contain geophysical parameters and are derived from Level 1 data, at 60m vertical and 5km horizontal resolution.

Tags: earth-science-aerosols-atmosphere, earth-science-aerosols-atmosphere-aerosol-backscatter, earth-science-aerosols-atmosphere-aerosol-optical-depth-thickness, earth-science-clouds-atmosphere, earth-science-clouds-atmosphere-cloud-properties-cloud-height, earth-science-clouds-atmosphere-cloud-properties-cloud-vertical-distribution
Organization: National Aeronautics and Space Administration
EPOXI INFLIGHT CALIBRATIONS - HRII RAW SPECTRA V2.0

This dataset contains raw calibration spectra acquired by the High Resolution Infrared Spectrometer (HRII) from 04 October 2007 through 07 February 2011 during the EPOCh, 103P/Hartley 2 Encounter, and cruise phases of the EPOXI mission.

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

THEMIS Ground All Sky Imager at Taloyoak (69.54 deg GLat, 266.45 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