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1) ACE EPAM PHA Daily-Averaged Spectra maxmize
Resource ID:spase://VEPO/NumericalData/ACE/EPAM/PHA/G122
Start:1997-08-30 00:00:00 Observatory:ACE Cadence:1 day
Stop:2014-10-22 01:00:41 Instrument:ACE Electron Proton Alpha Monitor Resource:NumericalData
Daily-averaged species-separated energy spectra derived from the Pulse Height Analyzer. Data consist of counts and fluxes of each of six species (He, C, O, Ne, Si, Fe) in each of 12 energy bins.

2) ACE Ultra Low Energy Isotope Spectrometer 1-Hour Level 2 Data maxmize
Resource ID:spase://VEPO/NumericalData/ACE/ULEIS/L2_PT1H
Start:1998-02-20 00:00:00 Observatory:ACE Cadence:1 hour
Stop:2014-10-22 01:00:44 Instrument:ACE Electron Proton Alpha Monitor Resource:NumericalData
The Ultra Low Energy Isotope Spectrometer measures ion fluxes over the charge range from H through Ni from about 20 keV/nucleon to 10 MeV/nucleon, thus covering both suprathermal and energetic particle energy ranges. Exploratory measurements of ultra-heavy species (mass range above Ni) will also be performed in a more limited energy range near 0.5 MeV/nucleon. ULEIS will be studying the elemental and isotopic composition of solar energetic particles, and the mechanisms by which these particles are energized in the solar corona. ULEIS will also investigate mechanisms by which supersonic interplanetary shock waves energize ions. To avoid confusion and misunderstanding, it is recommended that users consult with the appropriate ACE team members before publishing work derived from the data. The ACE team has worked hard to ensure that the level 2 data are free from errors, but the team cannot accept responsibility for erroneous data, or for misunderstandings about how the data may be used. This is especially true if the appropriate ACE team members are not consulted before publication. At the very least, preprints should be forwarded to the ACE team before publication.

3) IBEX Background Monitor Counts maxmize
Resource ID:spase://VEPO/NumericalData/IBEX/BM/Counts/PT0.24S
Start:2008-12-25 00:00:00 Observatory: Cadence:1 second
Stop:2009-06-19 00:00:00 Instrument: Resource:NumericalData
Each record captures the counts of >~14 keV protons arriving at the IBEX Background Monitor. Also included are a time tag (seconds since 00:00 UT of January 6, 1980), an arrival direction (R.A. and Dec. in J2000 celestial coordinates), and the IBEX location. Data files are given for each 8-day orbit. The data files are in ASCII.

4) IMAGE FUV SI plots of O/N2 Ratios maxmize
Resource ID:spase://VEPO/DisplayData/IMAGE/FUV/SI/O_N2_Ratios
Start:2000-05-24 00:00:00 Observatory:IMAGE Cadence:2 minutes
Stop:2005-05-18 23:59:59 Instrument:Far Ultraviolet Imager (FUV) Resource:DisplayData
This data set consists of images of thermospheric O/N2 column density ratios at 2-min resolution during times of strong geomagnetic storms (Dst.LT.-80nT) of 2000-2005. The ratios are generated from dayside airglow observations of the IMAGE Far Ultraviolet (FUV) Spectrographic Imager (SI). The SI has a peak response at the OI 135.6 nm oxygen emission line and a bandpass of 131.0 to 140.0 nm which includes the LBH band from N2 molecules. For each O/N2 plot, there is a plot of the SI image from which the O/N2 plot was generated, and there is an IDL saveset of the content of the O/N2 maps. The Information URL of this descriptor identifies detailed discussions of the derivations of O/N2 rations from the SI images.

5) IMP 8 CPME EPE MAG PLS Merge Data Set maxmize
Resource ID:spase://VEPO/NumericalData/IMP8/CPME/EPE/PT20S
Start:1973-10-28 00:00:00 Observatory:IMP 8 Cadence:20 seconds
Stop:2000-12-31 00:00:00 Instrument:Charged Particle Measurements Experiment (CPME) Resource:NumericalData
This data set contains 20.48s IMP8 CPME and EPE energetic particle data, along with IMP8 magnetic field and plasma data to facilitate use of the particle data. CPME data consist of: spin-integrated, 20.48s resolution count rates of protons in ten energy channels (0.29-0.50 to 90-440 MeV), of alpha particles in six channels (0.59-1.14 to 28-52 MeV/n), of Z>=3 particles in five channels (0.70-1.45 to 6-105 MeV/n), of electrons in 3 channels (0.22-2.5 to 0.80-2.5 MeV), of protons and alpha particles mixed in two channels (>35, >50 MeV/n) and uncertainties in all the preceding 20-s rates; spin-integrated, 10.24s count rates of protons in three energy channels (0.29-0.50 to 0.96-2.00 MeV) and of electrons in the three energy channels given above, plus uncertainties and data quality flags for all these 10.24s rates; 10.24s count rates in 8 spin sectors for 0.29-0.50 MeV protons and for 0.22-2.50 MeV electrons and their uncertainties and dataquality flags; 20.48s count rates in 8 spin sectors for 0.59-1.14 and 1.8-4.2 MeV/n alpha particles and for 0.7-3.3 and 3.1-8.8 MeV/n Z>= 3 particles, and their uncertainties anddata quality flags. EPE data consist of 16-sectored, 20.48s counts (not rates) for Z>=1 particles in 0.05-0.22 and 0.22-0.80 MeV/n channels, for electrons in 0.03-0.10 and 0.10-0.20 MeV channels and for Z>=1, E>0.015 MeV/n particles and electrons mixed. Magnetic field data include GSE and GSM cartesian components and direction angles. Plasma data, mainly from the MIT Faraday Cup, include flow velocity, density and temperature. Better sources exist for those desiring only IMP8 magnetic field and/or plasma data. Data are available as daily gzipped ASCII files; spin- integrated, 20.48s CPME count rates are also available with display and subset capability via FTPBrowser.

6) IMP 8 CRNC hourly energetic electron fluxes maxmize
Resource ID:spase://VEPO/NumericalData/IMP8/CRNC/Electrons_PT1H
Start:1973-10-30 00:00:00 Observatory:IMP 8 Cadence:1 hour
Stop:2001-10-26 00:00:00 Instrument:Cosmic Ray Nuclear Composition Resource:NumericalData
This data set contains hourly, spin-averaged fluxes of electrons from the IMP8 Cosmic Ray Nuclear Composition experiment of U. Chicago and UNH. There are fluxes of electrons in three energy bins: 0.7-2.0, 2-12, 12-50 MeV. These fluxes were generated at GSFC/SPDF from count rates accessible from UNH.

7) IMP 8 CRNC hourly count rates of heavy nuclei maxmize
Resource ID:spase://VEPO/NumericalData/IMP8/CRNC/Heavies_PT1H
Start:1973-10-30 00:00:00 Observatory:IMP 8 Cadence:1 hour
Stop:2001-10-26 00:00:00 Instrument:Cosmic Ray Nuclear Composition Resource:NumericalData
This data set contains hourly, spin-averaged count rates of heavy nuclei, and of particles penetrating the anticoincidence sensor, from the IMP8 Cosmic Ray Nuclear Composition experiment of U. Chicago and UNH. Included are rates of CNO nuclei at E.LT.80 MeV/n and E.GT.80 MeV/n, of Z.GT.8 nuclei at "low" and "high" energies, and of penetrating particles (protons with E.GT.106 MeV, etc.)

8) IMP 8 CRNC hourly energetic alpha particle fluxes maxmize
Resource ID:spase://VEPO/NumericalData/IMP8/CRNC/Helium_PT1H
Start:1973-10-30 00:00:00 Observatory:IMP 8 Cadence:1 hour
Stop:2001-10-26 00:00:00 Instrument:Cosmic Ray Nuclear Composition Resource:NumericalData
This data set contains hourly, spin-averaged fluxes of alpha particles from the IMP8 Cosmic Ray Nuclear Composition experiment of U. Chicago and UNH. There are fluxes of alpha particles in 9 energy bins from 10.90-12.89 to 84.32-94.81 MeV/n. These fluxes were generated at GSFC/SPDF from count rates accessible from UNH.

9) IMP 8 CRNC 15-min PHA and coincidence mode counts maxmize
Resource ID:spase://VEPO/NumericalData/IMP8/CRNC/PT15M
Start:1973-10-30 00:00:00 Observatory:IMP 8 Cadence:15 minutes
Stop:2000-09-30 00:00:00 Instrument:Cosmic Ray Nuclear Composition Resource:NumericalData
This 15-min-resolution data set consists of 5 count rates from the Low Energy Telescope, 8 count rates for the main telescope (MT), 4 counts of pulse height analyzed events in each of 4 MT coincidence modes, and 27 box counts corresponding to specific species and energy ranges associated with 3 of the MT coincidence modes. Actually the 13 referenced "count rates" are given as paired counts and accumulation times. Associated documentation suggests algorithms for computation of count rates and fluxes from the MT data given, for electrons in 3 energy bands (0.7-2.0, 2.0-12, 12-50 MeV), protons in 9 bands (11.24-20.00 MeV to 74.50-94.78 MeV), helium nuclei in 10 bands (10.90-12.89 MeV per n to 84.32-94.81 MeV per n), and CNO nuclei in 1 band (25 - 250 Mev per n). There are no azimuthally sectored data in this data set. The data are accessible via ftp and, with higher functionality, via FTPBrowser.

10) IMP 8 CRNC hourly energetic proton fluxes maxmize
Resource ID:spase://VEPO/NumericalData/IMP8/CRNC/Protons_PT1H
Start:1973-10-30 00:00:00 Observatory:IMP 8 Cadence:1 hour
Stop:2001-10-26 00:00:00 Instrument:Cosmic Ray Nuclear Composition Resource:NumericalData
This data set contains hourly, spin-averaged fluxes of protons from the IMP8. Cosmic Ray Nuclear Composition experiment of U. Chicago and UNH. There are are fluxes of protons in 9 energy bins from 11.24-12.62 to 74.50-94.78 MeV. These fluxes were generated at GSFC/SPDF from count rates accessible from UNH.

11) IMP 8 UMD EECA 10.92m Rates, PHA maxmize
Resource ID:spase://VEPO/NumericalData/IMP8/EECA/PT11M
Start:1973-11-01 00:00:00 Observatory:IMP 8 Cadence:11 minutes
Stop:2001-10-26 00:00:00 Instrument:Solid-State Detectors Resource:NumericalData
This data set, from the Electrostatic Energy-Charge Analyzer (EECA) part of the U. Maryland experiment on IMP 8, contains count rate and pulse height data enabling the computation of 10.92-min resolution fluxes of: singly ionized ions in 5 energy/charge windows of lower limits between 130 and 740 keV/Q; doubly charged ions in the same 5 keV/Q windows plus another at 65 keV/Q; ions with charge states between 5 and 8 in the same 6 keV/Q windows as for doubly charged ions plus another at 37 keV/Q; ions with charge states above about 10 at 37 and 65 keV/Q windows; 600-860 keV electrons. Some of the modes are spin integrated while others are given in 90 deg quadrants about the spacecraft spin vector (which is normal to the ecliptic plane). The data set was created at NSSDC from the U.Md.-provided "summary tapes" (NSSDC IDs SPHE-00170 and 73-078A-03C) by dropping engineering data, dropping data from the ULET portion of the overall experiment (the ULET instrument failed in 1978), and converting the remaining time, spacecraft position, and EECA instrument data from binary to ASCII representation. The data are available via ftp in 1- month files of variable lengths in the 3-6 MB size range.

12) IMP 8 GME 30-min energetic particle rates and fluxes maxmize
Resource ID:spase://VEPO/NumericalData/IMP8/GME/PT30M
Start:1973-11-01 00:00:00 Observatory:IMP 8 Cadence:30 minutes
Stop:2001-10-26 00:00:00 Instrument:Solar and Cosmic-Ray Particles Resource:NumericalData
This CDAWeb-accessible data set contains 30-minute, spin-averaged count rates and fluxes, and their statistical uncertainties, of energetic particles from the IMP8 GME experiment. Included are fluxes of: protons in 30 energy bins from 0.88-1.15 to 327-485 MeV; alpha particles in 21 energy bins from 1.14-1.36 to 63.3-81.0 MeV/n; and 0.3-18 MeV electrons. Also included are count rates for each of 7 sensors and for 11 multi-sensor coincidence modes. Proton and alpha particle fluxes, for every other energy bin, are given at the FTPBrowser and MSSP interfaces identified below.

13) Hourly Cosmic Ray Intensities from the Climax Neutron Monitor maxmize
Resource ID:spase://VEPO/NumericalData/NeutronMonitor/Climax/PT1H
Start:1951-01-01 00:00:00 Observatory:Climax Cadence:1 hour
Stop:2006-11-30 23:59:59 Instrument:Climax Neutron Monitor Resource:NumericalData
Hourly averages of relativistic cosmic ray intensities from the Climax Neutron Monitor

14) Daily Average Cosmic Ray Intensities from the Climax, Huancayo, and Haleakala Neutron Monitors maxmize
Resource ID:spase://VEPO/NumericalData/NeutronMonitor/Climax_Huancayo_Haleakala/P1D
Start:1953-01-01 00:00:00 Observatory:Climax Cadence:27 days
Stop:1992-12-31 23:59:59 Instrument:Climax Neutron Monitor Resource:NumericalData
Daily averages of relativistic cosmic ray intensities from the Climax, Huancayo, and Haleakala Neutron Monitors

15) Cosmic Ray Intensities Averaged over Bartels Solar Rotations from the Climax, Huancayo, and Haleakala Neutron Monitors maxmize
Resource ID:spase://VEPO/NumericalData/NeutronMonitor/Climax_Huancayo_Haleakala/P27D
Start:1951-01-18 00:00:00 Observatory:Climax Cadence:27 days
Stop:2006-11-09 23:59:59 Instrument:Climax Neutron Monitor Resource:NumericalData
Bartels Rotation averages of relativistic cosmic ray intensities from the Climax, Huancayo, and Haleakala Neutron Monitors For Climax only, averages are given both including and excluding days with significant contributions from ground level solar particle events.

16) Hourly Cosmic Ray Intensities from Neutron Monitors at Fort Smith, Peawanuck, Nain, and Inuvik maxmize
Resource ID:spase://VEPO/NumericalData/NeutronMonitor/FtSmith_Peawanuck_Nain_Inuvik/PT1H
Start:2000-01-01 00:00:00 Observatory:Fort Smith Cadence:1 hour
Stop:2014-07-22 01:00:54 Instrument:Fort Smith Neutron Monitor Resource:NumericalData
Hourly averages of relativistic cssmic ray intensities from Bartol Research Institute Neutron Monitors at Fort Smith, Peawanuck, Nain, and Inuvik

17) Hourly Cosmic Ray Intensities from the Haleakala Neutron Monitor maxmize
Resource ID:spase://VEPO/NumericalData/NeutronMonitor/Haleakala/PT1H
Start:1953-01-01 00:00:00 Observatory:Haleakala Cadence:1 hour
Stop:1992-12-31 23:59:59 Instrument:Haleakala Neutron Monitor Resource:NumericalData
Hourly averages of relativistic cosmic ray intensities from the Haleakala Neutron Monitor

18) Hourly Cosmic Ray Intensities from the Huancayo Neutron Monitor maxmize
Resource ID:spase://VEPO/NumericalData/NeutronMonitor/Huancayo/PT1H
Start:1953-01-01 00:00:00 Observatory:Huancayo Cadence:1 hour
Stop:1992-12-31 23:59:59 Instrument:Huancayo Neutron Monitor Resource:NumericalData
Hourly averages of relativistic cosmic ray intensities from the Huancayo Neutron Monitor

19) Hourly Cosmic Ray Intensities from Neutron Monitors at McMurdo, Newark, South Pole, and Thule maxmize
Resource ID:spase://VEPO/NumericalData/NeutronMonitor/McMurdo_SwarthmoreNewark_SouthPole_Thule/PT1H
Start:1960-06-24 00:00:00 Observatory:McMurdo Cadence:1 hour
Stop:2014-07-22 01:00:54 Instrument:McMurdo Neutron Monitor Resource:NumericalData
Hourly averages of relativistic cssmic ray intensities from Bartol Research Institute Neutron Monitors at McMurdo, Newark, South Pole, and Thule

20) SAMPEX Polar-Cap-Averaged Fluxes, all instruments maxmize
Resource ID:spase://VEPO/NumericalData/SAMPEX/PCA/PT48M
Start:1992-07-06 00:00:00 Observatory:SAMPEX Cadence:48 minutes
Stop:2004-06-30 23:59:59 Instrument:Mass Spectrometer Telescope (MAST) Resource:NumericalData
This data set contains 17 differential fluxes of protons (mainly), helium ions, Z.GE.6 ions, and electrons, plus one integral flux of protons and electrons, as averaged over polar cap passes of the SAMPEX spacecraft. A polar cap pass covers the time poleward of geomagnetic latitude 70 deg. (Not all orbits have two polar cap passes.). For any given species, the fluxes typically come from more than one of the sensors (LICA, HILT, MAST, PET). Hence the inclusion of all instruments' data in each single record. Differential fluxes are those for (mainly) protons (Z.GE.1 channels at 5-12 and 19-27 MeV/n), helium ions (0.50-6.6, 4-9, 8-15, 9-38 MeV/n), Z.GE.6 ions (0.49-8.3, 8-42, 19.3-22.8, 22.8-31.0, 31.0-51.7, 41-220, 51.7-76.2, 76.2-113, 113-156 MeV/n), and electrons (1.5-6.0 MeV from PET only). One LICA channel measured integral fluxes of ions .GT. 0.8 MeV/n plus electrons .GT. 0.6 MeV). Data available for each polar cap pass are time tags of the begin and end points of the averaging interval, the fluxes, statistical uncertainties in the fluxes, instrument-specific flags, and a flag indicating a north or south polar cap pass. Data are organized in two different ways. Monthly ~500-KB ASCII files with records organized by instrument are available from the SAMPEX Data Center at Caltech and from nssdcftp at GSFC/SPDF, while monthly ~260 KB CDF-formatted files with records organized by species are available from the ftp area underlying CDAWeb. The parameter level information given below in this descriptor corresponds to the CDAWeb organization of data. Format information for the ASCII version is given in the Information URL of this descriptor.

21) SOHO CELIAS 5-min Key Parameter Data maxmize
Resource ID:spase://VEPO/NumericalData/SOHO/CELIAS/KP/PT5M
Start:1995-12-22 00:00:00 Observatory:SOHO Cadence:5 minutes
Stop:2002-01-31 00:00:00 Instrument:Charge, Element, and Isotope Analysis System (CELIAS) Resource:NumericalData
Data include 5-min solar wind speed values, heavy ion fluxes in energy bands 0.02-1. MeV/q and 0.5-50 keV/q, and solar EUV photon fluxes from the CELIAS package on SOHO. They are key parameter data accessible from CDAWeb. Scanning CDAWeb plots for the full 1995-2002 time span suggests that only the solar wind flow speed are useful

22) SOHO COSTEP Key Parameter Data maxmize
Resource ID:spase://VEPO/NumericalData/SOHO/COSTEP/KP/PT5M
Start:1995-12-07 00:00:00 Observatory:SOHO Cadence:5 minutes
Stop:2002-01-31 00:00:00 Instrument:Comprehensive Suprathermal and Energetic Particle Instrument (COSTEP) Resource:NumericalData
Data include 5-min differential fluxes of protons at seven energies between 0.54 and 47 MeV, of electrons at four energies between 0.5 and 7.4 MeV and of alpha particles at four energies between 6.1 and 47 MeV/n. They are key parameter data accessible from CDAWeb.

23) SOHO ERNE Key Parameter Data maxmize
Resource ID:spase://VEPO/NumericalData/SOHO/ERNE/KP/PT128S
Start:1995-12-11 00:00:00 Observatory:SOHO Cadence:128 seconds
Stop:2000-02-09 00:00:00 Instrument:Energetic and Relativistic Nuclei and Electrons (ERNE) Resource:NumericalData
Data include 128s differential fluxes of protons and He4 nuclei, each at six energies between 3 and 96 MeV and of electrons at two energies (4-16 and >16 MeV). They are key parameter data accessible from CDAWeb. Data are very sparse after January, 1997.

24) Voyager-1 CRS Cruise Mode daily averages maxmize
Resource ID:spase://VEPO/NumericalData/Voyager1/CRS/FLUX/P1D
Start:1977-09-07 00:00:00 Observatory:Voyager 1 Cadence:1 day
Stop:2012-08-19 00:00:00 Instrument:Cosmic Ray System (CRS) Resource:NumericalData
daily averages of selected fluxes

25) Voyager-1 CRS Cruise Mode 15-minute averages maxmize
Resource ID:spase://VEPO/NumericalData/Voyager1/CRS/FLUX/PT15M
Start:1977-09-07 00:00:00 Observatory:Voyager 1 Cadence:15 minutes
Stop:2012-08-19 00:00:00 Instrument:Cosmic Ray System (CRS) Resource:NumericalData
15-minute averages of selected fluxes

26) Voyager 1 CRS Cruise Mode 6-hour averages maxmize
Resource ID:spase://VEPO/NumericalData/Voyager1/CRS/FLUX/PT6H
Start:1977-09-05 00:00:00 Observatory:Voyager 1 Cadence:6 hours
Stop:2011-10-01 00:00:00 Instrument:Cosmic Ray System (CRS) Resource:NumericalData
6-hour averages of selected fluxes

27) Voyager-2 CRS Cruise Mode daily averages maxmize
Resource ID:spase://VEPO/NumericalData/Voyager2/CRS/FLUX/P1D
Start:1977-08-24 00:00:00 Observatory:Voyager 2 Cadence:1 day
Stop:2012-08-19 00:00:00 Instrument:Cosmic Ray System (CRS) Resource:NumericalData
daily averages of selected fluxes

28) Voyager-2 CRS Cruise Mode 15-minute averages maxmize
Resource ID:spase://VEPO/NumericalData/Voyager2/CRS/FLUX/PT15M
Start:1977-08-24 00:00:00 Observatory:Voyager 2 Cadence:15 minutes
Stop:2012-08-19 00:00:00 Instrument:Cosmic Ray System (CRS) Resource:NumericalData
15-minute averages of selected fluxes

29) Voyager 2 CRS Cruise Mode 6-hour averages maxmize
Resource ID:spase://VEPO/NumericalData/Voyager2/CRS/FLUX/PT6H
Start:1977-08-22 00:00:00 Observatory:Voyager 2 Cadence:6 hours
Stop:2011-10-01 00:00:00 Instrument:Cosmic Ray System (CRS) Resource:NumericalData
6-hour averages of selected fluxes

30) Wind EPACT/LEMT 1-Hr H,He,O,Fe Anisotropies for Events maxmize
Resource ID:spase://VEPO/NumericalData/Wind/EPACT/LEMT/Events/A1S/PT1H
Start:1997-11-03 00:00:00 Observatory:Wind Cadence:1 hour
Stop:2006-12-17 00:00:00 Instrument:Energetic Particle Acceleration, Composition and Transport (EPACT) Resource:NumericalData
This data set contains hourly resolution anisotropies in spacecraft and solar wind frames for 2.5-5 MeV/n H, He, O and Fe nuclei, plus 5-8 MeV/n He nuclei. First-, second- and third-order spacecraft-frame anisotropies, and the magnitude and direction angles, relative to the mean magnetic field, of the spacecraft-frame first-order anisotropy vectors are given. Ion spectral parameters used in anisotropy determinations, namely spectral power law index (gamma), mean energy of ions in sampled energy range, and ion flux at the mean energy, are given. Many solar wind parameter averages are given, including magnetic field magnitude and direction, solar wind density and flow speed and azimuthal angle. Standard deviations in all hourly averages are also given. See Tan et al, Ap.J.,661, 1297-1310, 2007, for discussions of anisotropies, reference frames, etc. As of 10/2011, the data cover 39 1997-2006 multi- day intervals that include energetic solar particle events. ASCII data words are comma-separated. For a given particle event, there are species-specific files. File naming uses the convention XX_a1s_YYYYMMDD, where XX = H (or Hng), He2 (2.5-5 MeV/n), He5 (5-8 MeV/n), O or Fe, and where YYYYMMDD is the day of the first record of the file. "Hng" means hydrogen - no gamma (as obtained from IMP 8 GME data); but see the readme file cited below on the use of EPACT/LEMT He data as providing an alternative power law index.

31) Wind EPACT/LEMT 1-Hr Omnidirectional He,O,Fe Fluxes for Events maxmize
Resource ID:spase://VEPO/NumericalData/Wind/EPACT/LEMT/Events/OMNI/PT1H
Start:1997-11-03 00:00:00 Observatory:Wind Cadence:1 hour
Stop:2006-12-17 00:00:00 Instrument:Energetic Particle Acceleration, Composition and Transport (EPACT) Resource:NumericalData
This data set contains hourly-averaged fluxes of He, O and Fe nuclei, each in 6 energy bins in the general range 2-9 MeV/n, for (as of 10/2011) 39 1997-2006 multi-day intervals that include energetic solar particle events. Poisson uncertainties are given for each flux. ASCII data words are comma-separated. For a given particle event, there are species-specific files. File naming uses the convention XX_omn_YYYYMMDD, where XX = He, O or Fe, and where YYYYMMDD is the day of the first record of the file. Each file starts with a column header which includes (in the flux columns) the range in MeV/n for each of the six bands for the relevant species (although the species is not named within the file) and uncertainties designated as dJn for that associated with the flux of the n'th energy band. Energy bands for the various species are: He: 1.65-2.00, 2.00-2.40, 2.40-3.00, 3.00-3.70, 3.70-4.53, 4.53-6.00 MeV/n O: 2.56-3.17, 3.17-3.88, 3.88-4.68, 4.68-6.00, 7.00-7.40, 7.40-9.20 MeV/n Fe: 2.40-3.00, 3.00-3.95, 3.95-4.80, 4.80-5.90, 5.90-7.80, 7.80-9.30 MeV/n

32) Wind EPACT/LEMT 1-Hr Spin-Sectored H,He,O,Fe Counts for Events maxmize
Resource ID:spase://VEPO/NumericalData/Wind/EPACT/LEMT/Events/SEC/PT1H
Start:1997-11-03 00:00:00 Observatory:Wind Cadence:1 hour
Stop:2006-12-17 00:00:00 Instrument:Energetic Particle Acceleration, Composition and Transport (EPACT) Resource:NumericalData
This data set contains hourly counts of H, He, O and Fe nuclei in 16 look directions about the spacecraft spin axis. Counts for each of the four species are given at 2.5-5 MeV/n, and an additional count is given for 5-8 MeV/n He. As of 10/2011, the data cover 39 1997-2006 multi-day intervals that include energetic solar particle events. ASCII data words are comma-separated. For a given particle event, there are species-specific files. File naming uses the convention XX_sec_YYYYMMDD, where XX = H, He2 (2.5-5 MeV/n), He5 (5-8 MeV/n), O or Fe, and where YYYYMMDD is the day of the first record of the file. Sectoring is defined with respect to the ecliptic plane projection of the concurrently measured magnetic field vector. The edge of sector #1 is coincided with the projection of B on the ecliptic plane, so phi value of the center of sector i is phiB+11.25+(i-1)*22.5 deg, where phiB is the longitudinal angle of B.

33) Wind EPACT 92s KP Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Wind/EPACT/PT92S
Start:1994-11-16 00:00:00 Observatory:Wind Cadence:92 seconds
Stop:2014-10-22 01:00:45 Instrument:Energetic Particle Acceleration, Composition and Transport (EPACT) Resource:NumericalData
This set of key parameter flux data from the Wind EPACT (Energetic Particles: Acceleration, Composition and Transport) telescopes contains fluxes of protons (19-72 MeV in 2 energy bins), He nuclei (0.08-72 MeV/n in 5 bins), CNO nuclei (80-640 MeV/n in 2 bins), O nuclei (3.2-6.2 MeV/n in 1 bin), Fe nuclei (0.08-6.2 MeV/n in 3 bins) and 1-10 MeV electrons, each averaged over 92 seconds.

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