AndreaBozzo/ceres-open-data-index huggingface dataset:
CAMEX-4 MIPS 915 MHZ DOPPLER WIND PROFILER V1

The CAMEX-4 MIPS 915 MHZ Doppler Wind Profiler dataset was collected by the University of Alabama in Huntsville (UAH) Mobile Integrated Profiling System (MIPS), which is a mobile atmospheric profiling system. It includes a 915 MHz Doppler profiler, lidar ceilometer, 12 channel microwave profiling radiometer, Doppler Sodar, Radio Acoustic Sounding System (RASS), Field Mills, and surface observing station. This dataset contains 15 minute averaged 3-D wind profiles. Additionally, radial velocity and backscatter intensity data are contained in the dataset.

Tags: earth-science-atmospheric-winds-atmosphere-wind-profiles
Organization: National Aeronautics and Space Administration
CAMEX-4 MIPS SURFACE STATION 2 V1

The University of Alabama in Huntsville (UAH) Mobile Integrated Profiling System (MIPS) is a mobile atmospheric profiling system. It includes a 915 MHz Doppler profiler, lidar ceilometer, 12 channel microwave profiling radiometer, Doppler Sodar, Radio Acoustic Sounding System (RASS), Field Mills, and surface observing station. This dataset consists of data from Surface Station Two which contained multiple instruments including an anemometer, rain gauge, thermometer, pyranometer and barometer. Information, collected at 0.5 Hz, includes windspeed and direction as well as precipitation, temperature/humidity, solar radiation, and atmospheric pressure.

Tags: earth-science-atmospheric-pressure-atmosphere-surface-pressure, earth-science-atmospheric-radiation-atmosphere-solar-radiation, earth-science-atmospheric-temperature-atmosphere-surface-temperature-air-temperature, earth-science-atmospheric-water-vapor-atmosphere-water-vapor-indicators-humidity, earth-science-atmospheric-winds-atmosphere-surface-winds, earth-science-precipitation-atmosphere-liquid-precipitation-rain, earth-science-precipitation-atmosphere-precipitation-amount, earth-science-precipitation-atmosphere-precipitation-rate
Organization: National Aeronautics and Space Administration
Polar Plasma Wave Instrument (PWI), High Frequency Waveform Receiver, 25kHz bandwidth, 6-channel fields

PWI>Plasma Wave Instrument Reference: Gurnett, D.A. et al, The Polar Plasma Wave Instrument, Space Science Reviews, Vol. 71, pp. 597-622, 1995. donald-gurnett@uiowa.edu An FFT on 1024 values was used in calibrating the data; i.e., perform FFT, calibrate in frequency domain, perform inverse FFT to get calibrated time series. Coordinate system used: local magnetic field-aligned, a spacecraft centered coordinate system where Z is parallel to the local B-field determined from Polar MFE, X points outward and lies in the plane defined by the Z-axis and the radial vector from the earth to the spacecraft, and Y completes a right-handed system and points eastward. The X- and Z-axes are contained in the north-south plane. Effective bandwidth is 1.5*delta_f, where delta_f depends on the size of the FFT used to convert to the frequency domain, and delta_t. These data come in snapshots of 31816 points per channel, every 9.2 seconds, where the duration of each snapshot is 0.045 seconds. The time for individual samples is the epoch time of the snapshot incremented by delta_t in milliseconds for each successive sample. That is: sample_time = epoch_time + sample_offset * delta_t The data in this file will be in sets of 31744 (31*1024) points per channel because the FFT size does not come out even within the number of points per snapshot. To obtain the time for each point in the snapshot, increment each Epoch time after the first with Delta_T (in ms). The unattenuated frequency range for this file type is 20Hz to 25000Hz. The cadence value given here is computed from the inverse of the sampling rate (71.43 kHz). For a description of the PWI receivers and the different operational modes see: http://www-pw.physics.uiowa.edu/plasma-wave/istp/polar/modes.html

Tags: auroral-hiss, bernstein-waves, cdf-global-attribute-adid_ref-nssd2001, cdf-global-attribute-data_type-h7hfwr-6-channel-14-usec, cdf-global-attribute-data_version-2, cdf-global-attribute-discipline-space-physicsmagnetospheric-science, cdf-global-attribute-mission_group-polar-cdf-global-attribute-mission_group-magnetospheric-data, cdf-global-attribute-mods-created-feb-2012, cdf-global-attribute-project-istpinternational-solar-terrestrial-physics, chorus, continuum-radiation, electostatic-solitary-waves, equatorial-noise, esw, ion-acoustic-waves, langmuir-waves, lower-hybrid-waves, plasmaspheric-hiss, upper-hybrid-waves, waves-passive-cdf-global-attribute-title-polar-pwi-hfwr, whistlers
Organization: National Aeronautics and Space Administration
NEW HORIZONS  SWAP PLUTO ENCOUNTER  CALIBRATED V3.0

This data set contains Calibrated data taken by the New Horizons  Solar Wind Around Pluto  instrument during the  Pluto encounter  mission phase. This is VERSION 3.0 of this data set.   This data set contains SWAP observations taken during the  the Approach (Jan-Jul, 2015), Encounter, Departure, and  Transition mission sub-phases, including flyby observations  taken on 14 July, 2015, and departure and calibration data  through late October, 2016. This data set completes the  Pluto mission phase deliveries for SWAP.     This is version 3.0 of this dataset. Changes since version 2.0 include  the addition of data downlinked between the end of January, 2016 and  the end of October, 2016, completing the delivery of all data covering  the Pluto Encounter and subsequent Calibration Campaign.   Also, updates were made to the calibration files, documentation, and  catalog files. Finally, downlink data several days beyond the end of  the nominal end of mission phase were included in this data set in an  attempt to fill out the products at the nominal end of mission phase;  refer to the CONFIDENCE_LEVEL_NOTE in this data set catalog for more  details.

Tags: __
Organization: National Aeronautics and Space Administration
Helios 2 Hourly Trajectory Data

This directory includes hourly heliocentric coordinate data for the \nHelios 1 spacecraft as extracted into the ASCII files HE1TRJyy.asc (yy \nis the two-digit year) from the merged solar wind magnetic and plasma \ndata set in HELIOS_1/MGD_FREEMAN. All trajectory parameters except solar \necliptic and heliographic inertial coordinates were taken from the \noriginal merged dataset. The other parameters were computed and added \nusing the code HELTRJCON in the MGD_FREEMAN directory. Source routines \nfor coordinate conversions in this code were provided by R. Parthasarathy\nof the Satellite Situation Center at NSSDC. The code READHEL in \nMGD_FREEMAN was used to read the archived datasets into an intermediate \nformat for input to HELTRJCON. Code HELTRJCN1 was used to correct the \nsolar ecliptic angles as of 6/14/94 (see Note 2 above). HELTRJCON was \nalso corrected as of this date.\n\nData Parameter Description:\n\nNY       - YEAR OF THE DATA INTERVAL (LAST TWO DIGITS ONLY). \nND       - DAY OF THE DATA INTERVAL FROM THE FIRST DAY OF THE ABOVE YEAR,  \n              JAN. 1= DAY 1.  \nNH       - HOUR OF THE DAY OF THE DATA INTERVAL.                      \nNCARROT  - CARRINGTON ROTATION NUMBER AS SEEN BY AN EARTH BASED OBSERVER    \n              AT THE START OF THE DATA INTERVAL.                           \nSPAU     - SPACECRAFT HELIOCENTRIC DISTANCE IN ASTRONOMICAL UNITS.  \nSECLAT   - SOLAR ECLIPTIC LATITUDE IN DEGREES\nSECLON   - SOLAR ECLIPTIC LONGITUDE IN DEGREES\nHELLAT   - SOLAR HELIOGRAPHIC LATITUDE IN DEGREES\nHELLON   - SOLAR HELIOGRAPHIC (CARRINGTON) LONGITUDE IN DEGREES\nHILLON   - SOLAR HELIOGRAPHIC INERTIAL LONGITUDE IN DEGREES WITH RESPECT TO\n              ASCENDING NODE OF SOLAR EQUATOR ON THE ECLIPTIC\nESSCSANG - EARTH-SUN-SPACECRAFT SEPARATION ANGLE (IN DEGREES, 0-360). \nICODE    -  DATA CODE: 1 MEANS PLASMA DATA ONLY ARE PRESENT FOR THAT HOURLY \n              INTERVAL; 2 MEANS MAGNETOMETER DATA ONLY; 3 MEANS BOTH PLASMA \n              AND MAGNETOMETER DATA PRESENT. \n\nNote 1: The solar ecliptic coordinates are given with respect to true\nequinox and ecliptic of date. The solar ascending node was located at\necliptic longitude +74.367 degrees as of 1 Jan. 1900 at 1200 UT; this\nlongitude increases by 1.4 degrees/century.\n\nNote 2: The solar ecliptic cordinates in this directory before 6/14/94 were\ncalculated incorrectly and have been corrected as of this date. The\nheliographic angles are from the original source dataset and had no problems.\n\n

Tags: ephemeris
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER COMET ESCORT 2 OSIWAC 2 EDR MTP014 V2.0

This data set contains images acquired by the OSIRIS Wide Angle Camera during the COMET ESCORT 2 phase of the Rosetta mission at the comet 67P, covering the period from 2015-03-10T23:25:00.000 to 2015-04-08T11:24:59.000. This version V2.0 supersedes previous deliveries of the same dataset.

Tags: __
Organization: National Aeronautics and Space Administration
CAMEX-4 MIPS FIELD MILL V1

The University of Alabama in Huntsville (UAH) Mobile Integrated Profiling System (MIPS) is a mobile atmospheric profiling system. It includes a 915 MHz Doppler profiler, lidar ceilometer, 12 channel microwave profiling radiometer, Doppler Sodar, Radio Acoustic Sounding System (RASS), Field Mills, and surface observing station. This dataset consists of data from the Electric Field Mills which yield information about the atmospheric electrical fields above the instruments.

Tags: earth-science-atmospheric-electricity-atmosphere-electric-field
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P RSI 1/2/3 COMET ESCORT 3 0972 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 2015-08-20T03:04:35.000 to 2015-08-20T09:56:27.500.

Tags: __
Organization: National Aeronautics and Space Administration
CAMEX-4 HIGH ALTITUDE MMIC SOUNDING RADIOMETER (HAMSR) V1

The CAMEX-4 High Altitude MMIC Sounding Radiometer (HAMSR) dataset was collected by the High Altitude Monolithic Microwave Integrated Circuit (MMIC) Sounding Radiometer (HAMSR), which is a microwave atmospheric sounder recently developed by JPL under the NASA Instrument Incubator Program. Operating with 25 spectral channels in the 50-190 HGz region, it provides measurements that can be used to infer the 3-D distribution of temperature, water vapor, and liquid water in the atmosphere, even in the presence of clouds. HAMSR was mounted in a wing pod of a NASA ER-2 research aircraft.

Tags: earth-science-atmospheric-temperature-atmosphere-surface-temperature-air-temperature, earth-science-atmospheric-water-vapor-atmosphere-water-vapor-indicators-water-vapor, earth-science-clouds-atmosphere-cloud-microphysics-cloud-liquid-water-ice
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSINAC 3 PRL-MTP008 RDR V3.0

This CODMAC level 3 data set contains radiometric calibrated image data in W/m^2/sr/nm, acquired by the OSIRIS Narrow Angle Camera on the Rosetta spacecraft during the PRELANDING mission phase, covering the period from 2014-09-23T10:00:00.000 to 2014-10-24T09:59:59.000. The prime target is comet 67P/Churyumov-Gerasimenko 1 (1969 R1). This version V3.0 supersedes previous deliveries of the same dataset with the following changes since the last version: Lien corrected dataset after the July and October 2018 PSA/PDS external peer reviews. Updated documentation and ancillary files, added document on bandpass filter. Updated SCIENCE_USER_GUIDE_V03.PDF to include one section about FAQ and one section about image data quality. Added shutter backtravel and readout issues to image quality map. Updated DATA_QUALITY_ID keyword in image header. Improved handling of images with missing packets. Included FITs files. Browse products changed to the same size as the original image.

Tags: __
Organization: National Aeronautics and Space Administration
MARS EXPRESS SUN MRS 1/2/3 EXTENDED MISSION 5 3781 V1.0

This is a Mars Express Radio Science data set, collected during the extended mission phase 2015-01-01 to 2016-12-31. It is a Solar Conjunction measurement and covers the time 2015-06-27T11:19:01 to 2015-06-27T14:40:00.

Tags: __
Organization: National Aeronautics and Space Administration
Helios 2 E6 Hourly Particle Fluxes in CDF Format

particle_flux>E6 - Merged proton, electron and alpha particle fluxes. Helios-A and Helios-B Spacecraft were a Pair of Deep Space Probes developed by the Federal Republic of Germany, FRG, in a Cooperative Program with NASA. The Purpose of the Mission was to make pioneering Measurements of the Interplanetary Medium from the Vicinity of the Earth Orbit to 0.3 AU. The Objective of Experiment, E6, was to study High-Energy, Charged, Cosmic Ray Particles of Solar, Planetary, and Galactic Origin in Interplanetary Space. Protons and Alpha Particles with Energies &gt;1.3 MeV/n, and electrons &gt;3.3 MeV were measured within Interplanetary Space over the Range from 0.3 to 1.0 A.U. The Instrument, a Particle Telescope with 55$#176; Field of View, consisted of five Semiconductor Detectors, one Sapphire Cherenkov Counter, and one Scintillation Counter, all enclosed by an Anticoincidence Cylinder. The Telescope was calibrated prior to Launch using Radioactive Sources, Particle Acceletors, and Ground-Level Muons. It measured Protons and Alpha particles in six Channels, 1.3 to 3.3, 3.3 to 13, 13 to 27, 27 to 37, 37 to 45, and &gt;45 MeV/n, and Electrons in five Energy Channels, 0.3 to 0.8, 0.8 to 2, 2 to 3, 3 to 4, and &gt;4 MeV. For more Detail See pages 253-257 of Raumfahrtforschung, Volume 19, Number 5, 1975. The Helios-A Cosmic Ray &apos;.dat&apos; and Helios-B Cosmic Ray &apos;.dat&apos; files contains hourly averaged Fluxes of Electrons, Protons and Alpha Particles in the MeV Ranges. The Files were written in ASCII-Codes. Each Record contains 10 hourly Averages. The Differential Fluxes, (m^2 s sr MeV)^-1, Cover, in several Bands, the Energy Range 0.3 to 2.0 MeV for Electrons, 4.0 to 51 MeV for Protons, and 2.0 to 48 MeV for Alpha Particles. Also provided are the Integral Fluxes of Alphas above 48 MeV, and Protons above 51 MeV. For some of the Energy Channels, the Standard Deviations of the Averages are also provided. Each File is preceded by a Header Record, providing the Start and Stop Times of the Data in the File. The Acronyms for the Rate Channels are composed of a Letter and an Indication of the Energy Range in MeV/n for Protons and Alpha Particles, respectively and MeV for Electrons. The counting Rates are given as (m^2 s sr MeV/n)^-1 except for the Integral Channels P&gt;51 and A&gt;48, which are given as (m^2 s sr)^-1. Note: 1. Negative Rates, -0.99999E+04, indicate Missing or Invalid Data. 2. The Energy Boundaries for the Electron Channels 0.2 to 0.8 and 0.8 to 2 are only rough Estimates.

Tags: energeticparticles
Organization: National Aeronautics and Space Administration
ROSETTA-ORBITER 67P OSINAC 4 PRL-MTP009 RDR V1.0

This CODMAC level 4 data set contains radiometric calibrated and geometric distortion corrected (resampled) image data in W/m^2/sr/nm acquired by the OSIRIS Narrow Angle Camera during the PRELANDING phase of the Rosetta mission, covering the period from 2014-10-24T10:00:00.000 to 2014-11-21T23:24:59.000.

Tags: __
Organization: National Aeronautics and Space Administration
CAMEX-4 NOAA WP-3D CLOUD PHYSICS V1

The CAMEX-4 NOAA WP-3D Cloud Physics dataset used the NOAA WP-3D Orion aircraft, which has multiple meteorological and microphysical sensors. These include, for example, cloud particle imagers and temperature and dewpoint probes. CAMEX-4 focused on the study of tropical cyclone (hurricane) development, tracking, intensification, and landfalling impacts using NASA-funded aircraft and surface remote sensing instrumentation. This dataset includes navigation data as well as the meteorological and microphysical data. For further information and to obtain this data, please contact GHRC at support-ghrc@earthdata.nasa.gov

Tags: earth-science-atmospheric-temperature-atmosphere-upper-air-temperature-dew-point-temperature, earth-science-clouds-atmosphere-cloud-microphysics-cloud-droplet-concentration-size
Organization: National Aeronautics and Space Administration
GALILEO ORBITER A POS IDA FLYBY TRAJ V1.0

Galileo Orbiter 60 second sampled trajectory data from the Ida         flyby in Ida-centric Solar Ecliptic (ISE) and RTN coordinates.         These data cover the interval 1993-08-28 00:00 to         1993-08-28 23:59.

Tags: __
Organization: National Aeronautics and Space Administration
CAMEX-4 NOAA LYMAN-ALPHA HYGROMETER V1

The CAMEX-4 NOAA Lyman-Alpha Hygrometer dataset was collected by the NOAA Lyman-alpha Total Water Hygrometer, which was flown during the fourth field campaign in the CAMEX series (CAMEX-4). CAMEX-4 ran from 16 August to 24 September 2001 and was based out of Jacksonville Naval Air Station, Florida, and included missions in the Gulf of America, Caribbean and Western Atlantic. The experiment focused on the study of tropical cyclone (hurricane) development, tracking, intensification, and landfalling impacts using both NASA-funded aircraft and surface remote sensing instrumentation.

Tags: earth-science-atmospheric-water-vapor-atmosphere-water-vapor-indicators-total-precipitable-wate, earth-science-atmospheric-water-vapor-atmosphere-water-vapor-indicators-water-vapor, earth-science-precipitation-atmosphere-hydrometeors
Organization: National Aeronautics and Space Administration
ULY JUP SCE RAW ODR V1.0

This data set contains raw Radio      Occultation (ROCC) Original Data Records data from the Ulysses (ULY)      Solar Corona Experiment (SCE) obtained during the ULY Jupiter flyby.      The data target the Io Plasma Torus (IPT) and cover the period      1992-02-03 11:20 to 1992-02-09 20:46.

Tags: __
Organization: National Aeronautics and Space Administration
IBEX High Energy Neutral Atom Imager (Hi) Data Release 02, not Compton-Getting corrected, not Survival Probability corrected, Omnidirectional, West Longitude Ecliptic Maps, Level H3 (H3), semiannually averaged Data

* 1: The Interstellar Boundary Explorer (IBEX) has operated in space since 2008 updating our knowledge of the outer heliosphere and its interaction with the local interstellar medium. Start-time: 2008-12-25. There are currently 17 releases of IBEX-HI and/or IBEX-LO data covering 2009-2020.\n* 2: This data set is from the Release 2 (6 months-cadence) IBEX-Hi map data for the year 2009 in the form of omnidirectional ENA (hydrogen) fluxes with no Compton-Getting correction (nocg) of flux spectra for spacecraft motion and no correction for ENA survival probability (nosp) between 1 and 100 AU.\n* 3. The data consist of all-sky maps in Solar Ecliptic Longitude (east and west) and Latitude angles for ENA (hydrogen) fluxes from IBEX-Hi energy bands 2-6 in numerical data form. Energy channels 2-6 have FWHM ranges of 0.52-0.95, 0.84-1.55, 1.36-2.50, 1.99-3.75, 3.13-6.00 keV, respectively. The corresponding center-point energies are 0.71, 1.11, 1.74, 2.73, and 4.29 keV. Details of the data and enabled science from Release 10 are given in the following journal publication:\n* 4: McComas, D. J., et al. (2017), Seven Years of Imaging the Global Heliosphere with IBEX, Astrophys. J. Supp. Ser., 229(2), 41 (32 pp.),\n* 5: http://doi.org/10.3847/1538-4365/aa66d8\n* 6. The following codes are used to define dataset types:\n- cg = Compton-Getting corrections have been applied to the data to account for the speed of the spacecraft relative to the direction of arrival of the ENAs.\n- nocg = no Compton-Getting corrections\n- sp = survival probability corrections have been applied to the data to account for the loss of ENAs due to radiation pressure, photoionization and ionization via charge exchange with solar wind protons as they stream through the heliosphere. This correction scales the data out from IBEX at 1 AU to ~100 AU. In the original data this mode is denoted as Tabular.\n- noSP - no survival probability corrections have been applied to the data.\n- omni = data from all directions.\n- ram = data was collected when the spacecraft was ramming into the incoming ENAs.\n- antiram = data was collected when the spacecraft was moving away from the incoming ENAs.\n* 7. The following list associates Release 2 map numbers (1-2) with mission year 1\n- Map 1: Map2009A, year 1, orbits 11-34, dates 12/25/2008-06/25/2009\n- Map 2: Map2009B, year 1, orbits 35-58, dates 06/25/2009-12/25/2009\n* 8: This particular data set, denoted in the original ascii files as mapN for N=1-2, which indicates a map number, includes pixel map data from all directions (omnidirectional), no CG, no SP, 6 month cadence.

Tags: neutralatomimages
Organization: National Aeronautics and Space Administration
CAMEX-4 MIPS SURFACE STATION 1 V1

The University of Alabama in Huntsville (UAH) Mobile Integrated Profiling System (MIPS) is a mobile atmospheric profiling system. It includes a 915 MHz Doppler profiler, lidar ceilometer, 12 channel microwave profiling radiometer, Doppler Sodar, Radio Acoustic Sounding System (RASS), Field Mills, and surface observing station. This dataset consists of data from Surface Station One containing multiple instruments including an anemometer, rain gauge, thermometer, pyranometer and barometer. Information, collected at 1Hz, includes windspeed and direction as well as precipitation, temperature/humidity, solar radiation, and atmospheric pressure.

Tags: earth-science-atmospheric-pressure-atmosphere-surface-pressure, earth-science-atmospheric-radiation-atmosphere-solar-radiation, earth-science-atmospheric-temperature-atmosphere-surface-temperature-air-temperature, earth-science-atmospheric-water-vapor-atmosphere-water-vapor-indicators-humidity, earth-science-atmospheric-winds-atmosphere-surface-winds, earth-science-precipitation-atmosphere-liquid-precipitation-rain, earth-science-precipitation-atmosphere-precipitation-amount, earth-science-precipitation-atmosphere-precipitation-rate
Organization: National Aeronautics and Space Administration
CAMEX-4 SHARED MOBILE ATMOSPHERIC RESEARCH AND TEACHING RADARS V1

The CAMEX-4 Shared Mobile Atmospheric Research and Teching Radars dataset was collected by the Shared Mobile Atmospheric Research and Teaching Radar (SMART-R), which is a portable 5 cm Doppler radar. All equipment (e.g., antenna, power generator, processors, and readout computers) are truck mounted to provide maximum transportability. Originally located in the Florida Keys during CAMEX-4, the radar was moved to the Venice Florida area for landfall of TS Gabrielle on September 14, 2001.

Tags: earth-science-radar-spectral-engineering-radar-reflectivity
Organization: National Aeronautics and Space Administration
CLEM1-LUN/EAR/SKY-ASTAR/BSTAR/UVVIS/HRES/LWIR/NIR-2-EDR-V1.0

The Clementine EDR (Engineering Data Record) Image Archive contains 88 CD-ROM volumes with more than 1.9 million images. Each volume contains approximately 3 lunar orbits but may vary in the number of orbits depending on the size of each orbit. The first volume in the set begins with orbit number 32--the start of the systematic lunar mapping phase of the mission. The image data products for the engineering checkout and operational rehearsal orbits (orbits 1-31), low Earth orbits, and earth phasing loop orbits are located on the last eight volumes at the end of the volume set.

Tags: __
Organization: National Aeronautics and Space Administration