cometadata/datacite-titles-descriptions-related-identifiers huggingface dataset:
DOI: 10.48322/njhg-7j22
title: Van Allen Probe B Radiation Belt Storm Probes Ion Composition Experiment (RBSPICE) Time of Flight × Pulse Height, Low-Energy Resolution, High-Time Resolution Proton Intensities and Pressures sorted by Pitch Angles, Level 3 (L3), 10.9 s Data

description: Van Allen Probe B, Radiation Belt Storm Probes Ion Composition Experiment, RBSPICE, Low Energy Resolution, High Time Resolution, Time of Flight × Pulse Height Proton, TOFxPHHLEHT, Pitch Angles and Pressures, PAP, Level 3 Data Product. Proton Differential Flux Intensities and Pressures sorted by Pitch Angle. This Data Set contains Van Allen Probe B Radiation Belt Storm Probes Ion Composition Experiment, RBSPICE, Level 3 Data, Time of Flight × Pulse Height (TOF×PH) Proton Flux Intensities and Pressures that are sorted by Pitch Angles. The Data include Unidirectional Differential Proton Fluxes (FPDU) that are measured at Low-Energy Resolution, High-Time Resolution by 6 Telescopes in 28 Channels from ~0.01 MeV to 2.0 MeV. The Data are listed by Telescope in Sector Order, with Spin Accumulation. plotted at the End of Accumulation. Also available are Percentage Error of Measurement, Quality Flag for the each Measurement Pitch Angle Bin and Time Step, calculated Perpendicular and Parallel Partial Pressure, Number Density calculated by integrating the Distribution Function and Pitch Angle, Total Flux Intensity observed during the Spin by intergrating over Energy and Pitch Angle, and Omnidirectional Total Flux Intensity per Spin. In addition, the Data Set contains Orbit Number, Spacecraft Position of the Spacecraft in GEO, SM, and GSM Coordinates, current Sector Number where each Spin is divided into 36 Sectors, Duration of the Accumulation, current Spin Number of the Spacecraft, Orbit Number, Dipole L Values in different Reference Frames. Level 3 Data include all Level 2 Data plus Spacecraft Positions, Pitch Angles of the six Telescopes based upon the measured Magnetic Field received from the Electric and Magnetic Field Instrument Suite and Integrated Science, EMFISIS, Instrument. This Processing is done in a Series of algorithmic Steps in which the EMFISIS Magnetic Field Data are loaded, the Energetic Particle, Composition and Thermal Plasma Suite, ECT, Magnetic Ephemeris Data are loaded, the Level 2 Flux Intensity Data File is copied, and the Pitch Angles are calculated and placed. Finally, the calculated Pitch Angles are written out along with the Level 2 Data Parameters to create the Level 3 RBSPICE Data Files.
DOI: 10.48322/bwm7-5m36
title: Van Allen Probe B Radiation Belt Storm Probes Ion Composition Experiment (RBSPICE) Time of Flight × Pulse Height, Low-Energy Resolution, High-Time Resolution Oxygen Intensities and Pressures sorted by Pitch Angles, Level 3 (L3), 10.9 s Data

description: Van Allen Probe B, Radiation Belt Storm Probes Ion Composition Experiment, RBSPICE, Low Energy Resolution, High Time Resolution, Time of Flight × Pulse Height Oxygen, TOFxPHOLEHT, Pitch Angles and Pressures, PAP, Level 3 Data Product. Oxygen Differential Flux Intensities and Pressures sorted by Pitch Angle. This Data Set contains Van Allen Probe B Radiation Belt Storm Probes Ion Composition Experiment, RBSPICE, Level 3 Data, Time of Flight × Pulse Height (TOF×PH) Oxygen Flux Intensities and Pressures that are sorted by Pitch Angles. The Data include Unidirectional Differential Oxygen Fluxes (FPDU) that are measured at Low-Energy Resolution, High-Time Resolution by 6 Telescopes in 28 Channels from ~0.01 MeV to 2.0 MeV. The Data are listed by Telescope in Sector Order, with Spin Accumulation. plotted at the End of Accumulation. Also available are Percentage Error of Measurement, Quality Flag for the each Measurement Pitch Angle Bin and Time Step, calculated Perpendicular and Parallel Partial Pressure, Number Density calculated by integrating the Distribution Function and Pitch Angle, Total Flux Intensity observed during the Spin by intergrating over Energy and Pitch Angle, and Omnidirectional Total Flux Intensity per Spin. In addition, the Data Set contains Orbit Number, Spacecraft Position of the Spacecraft in GEO, SM, and GSM Coordinates, current Sector Number where each Spin is divided into 36 Sectors, Duration of the Accumulation, current Spin Number of the Spacecraft, Orbit Number, Dipole L Values in different Reference Frames. Level 3 Data include all Level 2 Data plus Spacecraft Positions, Pitch Angles of the six Telescopes based upon the measured Magnetic Field received from the Electric and Magnetic Field Instrument Suite and Integrated Science, EMFISIS, Instrument. This Processing is done in a Series of algorithmic Steps in which the EMFISIS Magnetic Field Data are loaded, the Energetic Particle, Composition and Thermal Plasma Suite, ECT, Magnetic Ephemeris Data are loaded, the Level 2 Flux Intensity Data File is copied, and the Pitch Angles are calculated and placed. Finally, the calculated Pitch Angles are written out along with the Level 2 Data Parameters to create the Level 3 RBSPICE Data Files.
DOI: 10.48322/hrv9-ec37
title: Van Allen Probe B Radiation Belt Storm Probes Ion Composition Experiment (RBSPICE) Time of Flight × Pulse Height, High-Energy Resolution, Low-Time Resolution Oxygen Intensities and Pressures sorted by Pitch Angles, Level 3 (L3), 10.9 s Data

description: Van Allen Probe B, Radiation Belt Storm Probes Ion Composition Experiment, RBSPICE, High Energy Resolution, Low Time Resolution, Time of Flight × Pulse Height Oxygen, TOFxPHOHELT, Pitch Angles and Pressures, PAP, Level 3 Data Product. Oxygen Differential Flux Intensities and Pressures sorted by Pitch Angle. This Data Set contains Van Allen Probe B Radiation Belt Storm Probes Ion Composition Experiment, RBSPICE, Level 3 Data, Time of Flight × Pulse Height (TOF×PH) Oxygen Flux Intensities and Pressures that are sorted by Pitch Angles. The Data include Unidirectional Differential Oxygen Fluxes (FODU) that are measured at High-Energy Resolution, Low-Time Resolution by 6 Telescopes in 28 Channels from ~0.01 MeV to 2.0 MeV. The Data are listed by Telescope in Sector Order, with Spin Accumulation. plotted at the End of Accumulation. Also available are Percentage Error of Measurement, Quality Flag for the each Measurement Pitch Angle Bin and Time Step, calculated Perpendicular and Parallel Partial Pressure, Number Density calculated by integrating the Distribution Function and Pitch Angle, Total Flux Intensity observed during the Spin by intergrating over Energy and Pitch Angle, and Omnidirectional Total Flux Intensity per Spin. In addition, the Data Set contains Orbit Number, Spacecraft Position of the Spacecraft in GEO, SM, and GSM Coordinates, current Sector Number where each Spin is divided into 36 Sectors, Duration of the Accumulation, current Spin Number of the Spacecraft, Orbit Number, Dipole L Values in different Reference Frames. Level 3 Data include all Level 2 Data plus Spacecraft Positions, Pitch Angles of the six Telescopes based upon the measured Magnetic Field received from the Electric and Magnetic Field Instrument Suite and Integrated Science, EMFISIS, Instrument. This Processing is done in a Series of algorithmic Steps in which the EMFISIS Magnetic Field Data are loaded, the Energetic Particle, Composition and Thermal Plasma Suite, ECT, Magnetic Ephemeris Data are loaded, the Level 2 Flux Intensity Data File is copied, and the Pitch Angles are calculated and placed. Finally, the calculated Pitch Angles are written out along with the Level 2 Data Parameters to create the Level 3 RBSPICE Data Files.
DOI: 10.48322/1qnv-8c11
title: Van Allen Probe B RBSPICE TOF x Energy Ion Rates converted Level-3 data

description: This Level-3 data set contains Van Allen Probe B RBSPICE (Radiation Belt Storm Probes Ion Composition Experiment) TOF x (Time of Flight) energy ion fluxes that are measured at high-energy and low-time resolution by 6 telescopes in 64 channels from ~0.02-1.0 MeV and are available in physical units (counts/(s*sr*cm^2*MeV) by telescope in sector order. Also available are percentage error of measurement, quality flag, current sector number where each spin is dividied into 36 sectors, duration of the accumulation, current spin number of the spacecraft, orbit number, dipole L value using the SM reference frame, and position of the spacecraft in SM coordinates. Level 3 data include the pitch angles of the six telescopes, based upon the measured magnetic field received from the EMFISIS (Electric and Magnetic Field Instrument Suite and Integrated Science) instrument. This processing is done in a series of algorithmic steps in which the EMFISIS magnetic field data is loaded, the ECT Magnetic Ephemeris data is loaded, the Level 2 intensity data file is copied, and the pitch angles are calculated and placed into the copied Level 2 file, creating a Level 3 file.
DOI: 10.48322/6crc-aj02
title: Van Allen Probe B RBSPICE TOF x Energy Hydrogen Rates converted Level-3 data

description: This Level-3 data set contains Van Allen Probe B RBSPICE (Radiation Belt Storm Probes Ion Composition Experiment) TOF x energy proton rates that are measured at high-energy and low-time resolution by 6 telescopes in 14 channels from ~0.02-1.0 MeV are available in physical units (counts/(s*sr*cm^2*MeV) by telescope in sector order. Also available are percentage error of measurement, quality flag, current sector number where each spin is dividied into 36 sectors, duration of the accumulation, current spin number of the spacecraft, orbit number, dipole L value using the SM reference frame, and position of the spacecraft in SM coordinates. Level 3 data include the pitch angles of the six telescopes, based upon the measured magnetic field received from the EMFISIS (Electric and Magnetic Field Instrument Suite and Integrated Science) instrument. This processing is done in a series of algorithmic steps in which the EMFISIS magnetic field data is loaded, the ECT Magnetic Ephemeris data is loaded, the Level 2 intensity data file is copied, and the pitch angles are calculated and placed into the copied Level 2 file, creating a Level 3 file.
DOI: 10.48322/w7nq-kz93
title: Van Allen Probe B RBSPICE TOF x Energy non Hydrogen (Helium and Oxygen) Rates converted Level-3 data

description: This Level-3 data set contains Van Allen Probe B RBSPICE (Radiation Belt Storm Probes Ion Composition Experiment) TOF x (Time of Flight) energy of heavy ions (i.e., helium and oxygen) that are measured at high-energy and low-time resolution by 6 telescopes in 28 channels from ~0.02-1.0 MeV and are available in physical units (counts/(s*sr*cm^2*MeV) by telescope in sector order. Also available are percentage error of measurement, quality flag, current sector number where each spin is dividied into 36 sectors, duration of the accumulation, current spin number of the spacecraft, orbit number, dipole L value using the SM reference frame, and position of the spacecraft in SM coordinates. Level 3 data include the pitch angles of the six telescopes, based upon the measured magnetic field received from the EMFISIS (Electric and Magnetic Field Instrument Suite and Integrated Science) instrument. This processing is done in a series of algorithmic steps in which the EMFISIS magnetic field data is loaded, the ECT Magnetic Ephemeris data is loaded, the Level 2 intensity data file is copied, and the pitch angles are calculated and placed into the copied Level 2 file, creating a Level 3 file.
DOI: 10.48322/6wj8-zz20
title: Van Allen Probe B RBSPICE TOF x PH High Energy Low Time Resolution Hydrogen Rates converted Level-3 data

description: This data set contains Van Allen Probe B RBSPICE (Radiation Belt Storm Probes Ion Composition Experiment) Level 3 data, with TOF x (Time of Flight) pulse height hydrogen and oxygen fluxes that are measured at high-energy and low-time resolution by 6 telescopes in 28 channels from ~0.01-2.0 MeV. Data are available in physical units (counts/(s*sr*cm^2*MeV)) by telescope in sector order, with spin accumulations plotted at the end of accumulation. Also available are percentage error of measurement, quality flag, current sector number where each spin is dividied into 36 sectors, duration of the accumulation, current spin number of the spacecraft, orbit number, dipole L value using the SM reference frame, and position of the spacecraft in SM coordinates. Level 3 data include all level 2 data plus spacecraft positions, pitch angles of the six telecopses, and derived magnetic field values. The processing is done in a series of algorithmic steps in which the EMFISIS (Electric and Magnetic Field Instrument Suite and Integrated Science) magnetic field data is loaded, the ECT (Energetic Particle, Composition and Thermal Plasma Suite) magnetic ephemeris data is loaded, the Level 2 intensity data file is copied, and the pitch angles are calculated and placed into the copied Level 2 file, creating a Level 3 file.
DOI: 10.48322/9f4c-2b63
title: Van Allen Probe B RBSPICE TOF x PH Low Engergy High Time Resolution Hydrogen Rates converted Level-3 data

description: This data set contains Van Allen Probe B RBSPICE (Radiation Belt Storm Probes Ion Composition Experiment) Level 3 data, with TOF x (Time of Flight) pulse height proton rates converted to physical intensity (counts/(s*sr*cm^2*MeV)). Hydrogen and oxygen fluxes are measured by 6 telescopes in 28 channels from ~0.01-2.0 MeV at low energy resolution and high time resolution in sector order, with spin accumulations plotted at the end of accumulation. Also available are percentage error of measurement, quality flag, current sector number where each spin is dividied into 36 sectors, duration of the accumulation, current spin number of the spacecraft, orbit number, dipole L value using the SM reference frame, and position of the spacecraft in SM coordinates. Level 3 data include all level 2 data plus spacecraft positions, pitch angles of the six telecopses, and derived magnetic field values. The processing is done in a series of algorithmic steps in which the EMFISIS (Electric and Magnetic Field Instrument Suite and Integrated Science) magnetic field data is loaded, the ECT (Energetic Particle, Composition and Thermal Plasma Suite) magnetic ephemeris data is loaded, the Level 2 intensity data file is copied, and the pitch angles are calculated and placed into the copied Level 2 file, creating a Level 3 file.
DOI: 10.48322/b5me-tj22
title: Van Allen Probe B Proton Spectrometer Belt Research - Relativistic Proton Spectrometer (PSBR-RPS) Energies from ~60 MeV to ~2 GeV, Level 2 (L2), 0.058 s Data

description: Van Allen Probe B, Relativistic Proton Spectrometer, RPS, Proton Spectrometer Belt Research, PSBR, Data. The RPS instrument is a solid state detector telescope combined with a Cherenkov radiator. It measures protons with energies from about 60 MeV to about 2 GeV. For more information, see http://rbsp.aerospace.org/. For a complete description of the instrument, see Mazur et al., 2012, The Relativistic Proton Spectrometer (RPS) for the Van Allen Probes Mission (formerly known as Radiation Belt Storm Probes, RBSP), Space Science Reviews. DOI 10.1007/s11214-012-9926-9, http://www.springerlink.com/content/p84680786570g7qp/. The instrument PI, Joseph Mazur, can be reached at Joseph.E.Mazur@aero.org.
DOI: 10.48322/0qyz-h276
title: RBSP Energetic Particle, Composition, and Thermal Plasma Suite (ECT) Relativistic Electron Proton Telescope (REPT) Selenick Radiation Belt Proton Intensity Model, Level 3 (L3), Monthly Data

description: The Files associated with the Van Allen Probes Selenick Model Data Product contain Model Radiation Belt Proton Intensity derived from Data taken by the Van Allen Probes REPT Instruments using the Method described by: Selesnick, R.S., Baker, D.N., Kanekal, S.G., Hoxie, V.C., and X. Li, (2018). Modeling the Proton Radiation Belt with Van Allen Probes Relativistic Electron-Proton Telescope Data. J. Geophys. Res.: Space Phys., 123. https://doi.org/10.1002/2017JA024661. Each File contains average Intensity, as a Function of Kinetic Energy, Equatorial Pitch Angle, and L-Shell, derived from one Month of Data.
DOI: 10.48322/r0b5-m046
title: Van Allen Probe B Proton Spectrometer Belt Research - Relativistic Proton Spectrometer (PSBR-RPS) Energies from ~60 MeV to ~2 GeV, Level 2 (L2), 1 min Data

description: Van Allen Probe B, Relativistic Proton Spectrometer, RPS, Proton Spectrometer Belt Research, PSBR, Data. The RPS Instrument is a Solid State Detector Telescope combined with a Cherenkov Radiator. It measures Protons with Energies from about 60 MeV to about 2 GeV. For more Information, see http://rbsp.aerospace.org/. For a complete Description of the Instrument, see Mazur et al., 2012, The Relativistic Proton Spectrometer (RPS) for the Van Allen Probes Mission (formerly known as Radiation Belt Storm Probes, RBSP), Space Science Reviews. DOI 10.1007/s11214-012-9926-9, http://www.springerlink.com/content/p84680786570g7qp/. The instrument PI, Joseph Mazur, can be reached at Joseph.E.Mazur@aero.org.
DOI: 10.15468/dl.dbgkpq
title: Occurrence Download

description: A dataset containing 49 species occurrences available in GBIF matching the query:
{
 "and" : [
 "Country is one of (China, Hong Kong, Macao, Chinese Taipei)",
 "TaxonKey is Tamarix gracilis"
 ]
}

 The dataset includes 49 records from 2 constituent datasets; see https://api.gbif.org/v1/occurrence/download/0068899-251120083545085/datasets/export for details.
 
Data from some individual datasets included in this download may be licensed under less restrictive terms.
DOI: 10.15468/6vvpcb
title: Review of the genera and subgenera of the subtribe Aspilotina (Hymenoptera, Braconidae, Alysiinae), with a new illustrated key

description: This dataset contains the digitized treatments in Plazi based on the original journal article Peris-Felipo, Francisco Javier, Santa, Fernando, van Achterberg, Cornelis, Belokobylskij, Sergey A. (2025): Review of the genera and subgenera of the subtribe Aspilotina (Hymenoptera, Braconidae, Alysiinae), with a new illustrated key. ZooKeys 1229: 133-200, DOI: 10.3897/zookeys.1229.142489AbstractThe genera and subgenera of the subtribe Aspilotina are reviewed. A new illustrated key to all accepted supraspecies taxa is provided. Grandilota Fischer, 2002, stat. nov. is proposed as subgenus of Aspilota Foerster, 1863. Carinthilota Fischer, 1975, syn. nov. is synonymised with Alitha Cameron, 1906, stat. nov. and the latter is treated as subgenus of Dinotrema Foerster, 1863; Eudinostigma Tobias, 1986, syn. nov. is considered a synonym of Dinotrema Foerster, 1863. Moreover, the new subgenus Pseudoprosapha subgen. nov. (type species: Dinostigma stenosoma van Achterberg, 1988) is described. Additionally, Synaldotrema Belokobylskij & Tobias, 2002, stat. nov. is treated as a separate genus. The following new combinations are proposed: Aspilota (Aspilota) ruficollis Stelfox & Graham, 1950, comb. nov., Dinotrema (Alitha) lada (Belokobylskij, 1998), comb. nov., D. (A.) longipennis (Cameron, 1906), comb. nov., D. (A.) mavka (Belokobylskij, 1998), comb. nov., D. (A.) parapsidalis (Fischer, 1975), comb. nov., D. (A.) vechti (van Achterberg, 1988), comb. nov., Dinotrema (Dinotrema) alox (van Achterberg, 1988), comb. nov., D. (D.) entabeniense (Fischer, 2009), comb. nov., D. (D.) latum (Chen & Wu, 1994), comb. nov., D. (D.) planiceps (Fischer, Tormos & Pardo, 2006), comb. nov., D. (D.) subpulvinatum (Fischer, 2009), comb. nov., D. (Pseudoprosapha) stenosoma (van Achterberg, 1988), comb. nov., D. (Synaldis) bienesae (Fischer, Tormos & Pardo, 2006), comb. nov., D. (S.) fischeri (Tobias, 1986), comb. nov., D. (S.) latistigma (Fischer, 1962), comb. nov., D. (S.) planiceps (Fischer, Tormos & Pardo, 2006), comb. nov., D. (Synaldis) cespitator (Belokobylskij, 2004), comb. nov., D. (S.) perfidum (Fischer, 1970), comb. nov., D. (S.) trematosum (Fischer, 1967), comb. nov. and Panerema fulvicornis (Haliday, 1838), comb. nov.
DOI: 10.5281/zenodo.18091240
title: EDGES-2 Calibration Data for Bowman+2018

description: This repository contains the raw data used to calibrate the receiver in the Bowman+2018 EDGES-2 results (https://www.nature.com/articles/nature25792).
DOI: 10.5281/zenodo.16881868
title: EDGES-2 Calibration Data for Bowman+2018

description: This repository contains the raw data used to calibrate the receiver in the Bowman+2018 EDGES-2 results (https://www.nature.com/articles/nature25792).
DOI: 10.5281/zenodo.15025094
title: Japanese Long and Short Vowel Acoustic Data

description: This dataset contains the acoustic data and reading materials used in Yazawa and Kondo (2019).
DOI: 10.48322/3jya-jk44
title: SDO/AIA 94 Angstrom FITS Data

description: The SDO/AIA 94 Å Level 1 FITS Data. The 94 Å channel observes the Fe XVIII line from 6.3 MK flaring plasma.  

The Atmospheric Imaging Assembly (AIA) onboard Solar Dynamics Observatory (SDO) focuses on the evolution of the magnetic environment in the Sun’s atmosphere, and its interaction with embedded and surrounding plasma. The AIA investigation covers a broad range of science objectives that focus on five core research themes that both advance solar and heliospheric physics in general and provide advanced warning of coronal and inner-heliospheric disturbances of interest to the Living With a Star (LWS) program, i.e., global change, space weather, human exploration of space, and technological infrastructure in space and on Earth.

AIA provides the following essential capabilities: i) A view of the entire Sun in 4k x 4k resolution (pixel size of 0.6 arcseconds), with full thermal coverage of the corona; ii) A high signal-to-noise ratio for two- to three-second exposures that reaches 100 in quiescent conditions for the low-temperature coronal-imaging channels and during flaring in the higher-temperature channels, with a dynamic range of up to 10,000; iii) Essentially uninterrupted viewing for months at a temporal cadence of 12 seconds in seven extreme UV (EUV) band passes (94, 131, 171, 193, 211, 304 and 335 Å), and 24 seconds for two UV channels (1600 and 1700 Å) band passes; iv) In special observing modes, AIA can capture images of the Sun at higher cadence while keeping within the instrument allocated telemetry by using a subset of bandpass channels, and/or using a crop table.
DOI: 10.48322/pbyp-4d90
title: SDO/AIA 131 Angstrom FITS Data

description: The SDO/AIA 131 Å Level 1 FITS Data. The 131 Å channel observes the Fe xx and Fe xxiii lines from 10 MK and 16 MK flaring plasma, respectively. 

The Atmospheric Imaging Assembly (AIA) onboard Solar Dynamics Observatory (SDO) focuses on the evolution of the magnetic environment in the Sun’s atmosphere, and its interaction with embedded and surrounding plasma. The AIA investigation covers a broad range of science objectives that focus on five core research themes that both advance solar and heliospheric physics in general and provide advanced warning of coronal and inner-heliospheric disturbances of interest to the Living With a Star (LWS) program, i.e., global change, space weather, human exploration of space, and technological infrastructure in space and on Earth.

AIA provides the following essential capabilities: i) A view of the entire Sun in 4k x 4k resolution (pixel size of 0.6 arcseconds), with full thermal coverage of the corona; ii) A high signal-to-noise ratio for two- to three-second exposures that reaches 100 in quiescent conditions for the low-temperature coronal-imaging channels and during flaring in the higher-temperature channels, with a dynamic range of up to 10,000; iii) Essentially uninterrupted viewing for months at a temporal cadence of 12 seconds in seven extreme UV (EUV) band passes (94, 131, 171, 193, 211, 304 and 335 Å), and 24 seconds for two UV channels (1600 and 1700 Å) band passes; iv) In special observing modes, AIA can capture images of the Sun at higher cadence while keeping within the instrument allocated telemetry by using a subset of bandpass channels, and/or using a crop table.