{ "id": "UY_M0_AT1", "url": "http://hpde.io/VEPO/NumericalData/Ulysses/COSPIN/AT/Fluxes/PT10M", "data-file": "./data/spase_hpde_io/info/UY_M0_AT1.json", "data": { "Spase": { "xmlns": "http://www.spase-group.org/data/schema", "xmlns:xsi": "http://www.w3.org/2001/XMLSchema-instance", "xsi:schemaLocation": "http://www.spase-group.org/data/schema http://www.spase-group.org/data/schema/spase-2_2_2.xsd'", "Version": "2.2.2", "NumericalData": { "ResourceID": "spase://VEPO/NumericalData/Ulysses/COSPIN/AT/Fluxes/PT10M", "ResourceHeader": { "ResourceName": "Ulysses COSPIN/AT Ion 10-Minute Fluxes", "AlternateName": "COSPIN-AT-Fluxes-PT10M", "ReleaseDate": "2016-08-19T00:00:00", "Description": "10-Minute cadence proton and helium spin-averaged coincidence fluxes from the \n COSPIN Anisotropy Telescopes (AT1 and AT2). The two telescopes differ only by their orientation \n with respect to the spacecraft spin axis. The parameter keys in the parameter-level segments below are specifically relevant to the UFA-accessible versions of the data. ", "Acknowledgement": "Please acknowledge the COSPIN AT lead investigators \n (AT Group Leader: Dr. Andre Balogh, and Co-Investigator: Dr. Silvia Dalla) ", "Contact": [ { "PersonID": "spase://SMWG/Person/Andre.Balogh", "Role": [ "CoInvestigator", "TeamLeader" ] }, { "PersonID": "spase://SMWG/Person/Silvia.Dalla", "Role": [ "CoInvestigator", "DataProducer" ] }, { "PersonID": "spase://SMWG/Person/Cecil.Tranquille", "Role": "ArchiveSpecialist" } ], "InformationURL": { "Name": "Usernotes file for COSPIN/AT data files", "URL": "http://ufa.esac.esa.int/ufa/#instruments", "Description": "\n\t The UserNotes file at the Ulysses Final Archive (UFA) describes the\n\t format of the ASCII data files containing 10-minute average proton\n\t and helium spin-averaged and sectored fluxes for the \n\t dual COSPIN Anisotropy Telescopes (AT1 and AT2), and caveats for their use.\n\t A description of the AT Telescopes may be found in \n\t Simpson et al., Astron. Astrophys. 92, 365-399, 1992. An electronic copy of\n this paper is available at\n\t http://helio.estec.esa.nl/ulysses/ftp/cdroms/uls_02_a/Docs/Cospin/Cospin.htm\n (Note: in this paper, the pointing directions of the AT1 and AT2 are interchanged.\n The correct pointing directions are given below.)\n " } }, "AccessInformation": [ { "RepositoryID": "spase://SMWG/Repository/ESA/ESAC/UlyssesFinalArchive", "Availability": "Online", "AccessRights": "Open", "AccessURL": { "Name": "Ulysses Final Archive", "URL": "http://ufa.esac.esa.int/ufa/#data", "Description": "\n Parent directory containing yearly downloadable .zip compressed subdirectories with naming \n convention cosatNYY.zip. Here and below N=1 or 2 to identify which of the two identical AT \n telescopes is the source of the data, and YY indicates the two digit year corresponding to \n the data in the subdirectory. \n Each subdirectory contains daily ascii files with naming convention ucosatNrYYDOY.uly where \n N and YY are as above, and DOY is the three digit day of year (Jan. 1 = 1). \n Each file contains nominally 1-minute averages of the COSPIN/AT spin-averaged and sectored\n fluxes based on counting rates which respond primarily to protons and helium nuclei. \n Electron response is strongly suppressed by discriminator thresholds set on the 30 micron \n thick front detector, D1, which is required to fire for all events registered by the counting \n rates. Times given are the center point of the nominal 10 minute averaging interval, and the \n data entries are given in units of flux, (s cmsq sr MeV)^-1. (NB. MeV, not MeV/n.) For\n channels which respond to both protons and helium, the flux is computed using the energy range\n appropriate for protons, normally the dominant species in the channel. \n For each AT, the data are presented in the following format, where channels are named as in \n Table 5 of Simpson et al. (1992) and the energy ranges are given in MeV (not MeV/n). \n Energies listed are in the frame of the spacecraft. In the range of energies measured by \n the AT telescopes, the energy shifts resulting from convection of the nuclei by the \n solar wind are significant, and for study of anisotropies in the solar wind frame, appropriate\n corrections are necessary. Telescope AT1 points at 60 degrees to the spacecraft spin axis \n and telescope AT2 points at 145 degrees to the spacecraft spin axis. The Ulysses spacecraft \n spin axis is maintained within 1 degree of earth-pointing at all times. \n --------------------------------------------------------------------\n\t Field Fortran\tDefinition\t\tProtons\t\tHelium\n\t Format\t\t\t\t(MeV)\t\t(MeV)\n --------------------------------------------------------------------\n\t 1\t i4\t\t4 digitYear, e.g. 1992\n\t 2\t i3\t\tDay of year (Jan 1 = 1)\n\t 3\t i2\t\tHour of day\n\t 4 i2\t\tMinute of hour\n\t 5\t i2\t\tSecond of minute\n\t 6\t e11.4\t\tA1_N spin-averaged\t0.7-0.9\t\t2.3-2.5\n\t 7\t e11.4\t\tA2_N spin-averaged\t0.9-1.3\t\t2.5-2.7\n\t 8\t e11.4\t\tA3_N spin-averaged\t1.3-2.2\t\t2.7-3.0\n\t 9\t e11.4\t\tA4_N spin-averaged\t2.2-3.6\t\tno resp\n\t 10\t e11.4\t\tA5_N spin-averaged 3.6-6.5\t\t24.0-28.0\n\t 11\t e11.4\t\tA38_N spin-averaged\tno resp\t\t3.0-7.5\n\t 12\t e11.4\t\tA39_N spin-averaged\tno resp\t\t7.5-12.0\n\t 13\t e11.4\t\tA40_N spin-averaged\tno resp\t\t12.0-26.0\n\t 14\t e11.4\t\tA6_N (A3 sector 1)\t1.3-2.2\t\t2.7-3.0\n\t 15\t e11.4\t\tA7_N (A3 sector 2)\t \"\t\t \"\n\t 16\t e11.4\t\tA8_N (A3 sector 3)\t \"\t\t \"\t \n\t 17\t e11.4\t\tA9_N (A3 sector 4)\t \"\t\t \"\n\t 18\t e11.4\t\tA10_N (A3 sector 5)\t \"\t\t \"\n\t 19\t e11.4\t\tA11_N (A3 sector 6)\t \"\t\t \"\n\t 20\t e11.4\t\tA12_N (A3 sector 7)\t \"\t\t \"\n\t 21\t e11.4\t\tA13_N (A3 sector 8)\t \"\t\t \"\n\t 22\t e11.4\t\tA14_N (A4 sector 1)\t2.2-3.6\t\tno resp\n\t 23\t e11.4\t\tA15_N (A4 sector 2)\t \"\t\t \"\t\t\n\t 24\t e11.4\t\tA16_N (A4 sector 3)\t \"\t\t \"\n\t 25\t e11.4\t\tA17_N (A4 sector 4)\t \"\t\t \"\n\t 26\t e11.4\t\tA18_N (A4 sector 5)\t \"\t\t \"\n\t 27\t e11.4\t\tA19_N (A4 sector 6)\t \"\t\t \"\n\t 28\t e11.4\t\tA20_N (A4 sector 7)\t \"\t\t \"\n\t 29\t e11.4\t\tA21_N (A4 sector 8)\t \"\t\t \"\n\t 30\t e11.4\t\tA22_N (A5 sector 1)\t3.6-6.5\t\t24.0-28.0\n\t 31\t e11.4\t\tA23_N (A5 sector 2)\t \"\t\t \"\n\t 32\t e11.4\t\tA24_N (A5 sector 3)\t \"\t\t \"\n\t 33\t e11.4\t\tA25_N (A5 sector 4)\t \"\t\t \"\n\t 34\t e11.4\t\tA26_N (A5 sector 5)\t \"\t\t \"\n\t 35\t e11.4\t\tA27_N (A5 sector 6)\t \"\t\t \"\n\t 36\t e11.4\t\tA28_N (A5 sector 7)\t \"\t\t \"\n\t 37\t e11.4\t\tA29_N (A5 sector 8)\t \"\t\t \"\n \n The actual accumulation intervals contributing to an average consist of an integral number of \n telemetry subcomm sequences, and correspond to all subcomm sequences which start in the nominal\n 10 minute reporting interval. The minimum time corresponding to one subcomm sequence is 256\n seconds at 1024 bps, the most common science telemetry rate. Thus the actual start time of the \n accumulation may be up to 256 seconds later than the start time of the nominal\n interval. Similarly, the end time of the accumulation may extend up to 256 seconds beyond the \n end of the nominal interval. These data are therefore not useful for highly accurate timing\n studies. \n Information on the definition the spin sectors and the sectoring process is given below in the\n description of the A3 sectored data (channels 14-21 in the table above). \n " }, "Format": "Text", "Encoding": "ZIP", "Acknowledgement": "Dr. Silvia Dalla, University of Central Lancashire, UK" }, { "RepositoryID": "spase://SMWG/Repository/NASA/GSFC/SPDF", "Availability": "Online", "AccessRights": "Open", "AccessURL": { "Name": "FTP access to AT1 CDFs at SPDF", "URL": "ftp://spdf.gsfc.nasa.gov/pub/data/ulysses/particle/cospin_cdaweb/at1/", "Description": "AT1 data via ftp in CDF from SPDF." }, "Format": "CDF", "Acknowledgement": "Space Physics Data Facility at NASA/GSFC" }, { "RepositoryID": "spase://SMWG/Repository/NASA/GSFC/SPDF", "Availability": "Online", "AccessRights": "Open", "AccessURL": { "Name": "HTTP access to AT1 CDFs at SPDF", "URL": "http://spdf.gsfc.nasa.gov/pub/data/ulysses/particle/cospin_cdaweb/at1/", "Description": "In CDF via HTTP from SPDF" }, "Format": "CDF", "Acknowledgement": "Space Physics Data Facility at NASA/GSFC" }, { "RepositoryID": "spase://SMWG/Repository/NASA/GSFC/SPDF", "Availability": "Online", "AccessRights": "Open", "AccessURL": { "Name": "CDAWeb", "URL": "http://cdaweb.gsfc.nasa.gov/cdaweb/sp_phys/", "ProductKey": "UY_M0_AT1", "Description": "subset, plot, list via CDAWeb" }, "Format": "Text", "Acknowledgement": "CDAWeb or nssdcftp, as appropriate, from NASA/GSFC/SPDF" }, { "RepositoryID": "spase://SMWG/Repository/NASA/GSFC/SPDF", "Availability": "Online", "AccessRights": "Open", "AccessURL": { "Name": "FTP access to AT1 ASCII files at SPDF", "URL": "ftp://spdf.gsfc.nasa.gov/pub/data/ulysses/particle/cospin/at1/10min_new/", "Description": "AT1 data via ftp in ASCII from SPDF." }, "Format": "Text", "Acknowledgement": "CDAWeb or nssdcftp, as appropriate, from NASA/GSFC/SPDF" }, { "RepositoryID": "spase://SMWG/Repository/NASA/GSFC/SPDF", "Availability": "Online", "AccessRights": "Open", "AccessURL": { "Name": "HTTP access to AT1 ASCII files at SPDF", "URL": "http://spdf.gsfc.nasa.gov/pub/data/ulysses/particle/cospin/at1/10min_new/", "Description": "AT1 data via http in ASCII from SPDF." }, "Format": "Text", "Acknowledgement": "CDAWeb or nssdcftp, as appropriate, from NASA/GSFC/SPDF" }, { "RepositoryID": "spase://SMWG/Repository/NASA/GSFC/SPDF", "Availability": "Online", "AccessRights": "Open", "AccessURL": { "Name": "FTP access to AT2 CDFs at SPDF", "URL": "ftp://spdf.gsfc.nasa.gov/pub/data/ulysses/particle/cospin_cdaweb/at2/", "Description": "AT2 data via ftp in CDF from SPDF." }, "Format": "CDF", "Acknowledgement": "Space Physics Data Facility at NASA/GSFC" }, { "RepositoryID": "spase://SMWG/Repository/NASA/GSFC/SPDF", "Availability": "Online", "AccessRights": "Open", "AccessURL": { "Name": "HTTP access to AT2 CDFs at SPDF", "URL": "http://spdf.gsfc.nasa.gov/pub/data/ulysses/particle/cospin_cdaweb/at2/", "Description": "In CDF via HTTP from SPDF" }, "Format": "CDF", "Acknowledgement": "Space Physics Data Facility at NASA/GSFC" }, { "RepositoryID": "spase://SMWG/Repository/NASA/GSFC/SPDF", "Availability": "Online", "AccessRights": "Open", "AccessURL": { "Name": "CDAWeb", "URL": "http://cdaweb.gsfc.nasa.gov/cdaweb/sp_phys/", "ProductKey": "UY_M0_AT2", "Description": "subset, plot, list via CDAWeb" }, "Format": "Text", "Acknowledgement": "CDAWeb or nssdcftp, as appropriate, from NASA/GSFC/SPDF" }, { "RepositoryID": "spase://SMWG/Repository/NASA/GSFC/SPDF", "Availability": "Online", "AccessRights": "Open", "AccessURL": { "Name": "FTP access to AT2 ASCII files at SPDF", "URL": "ftp://spdf.gsfc.nasa.gov/pub/data/ulysses/particle/cospin/at2/10min_new/", "Description": "AT2 data via ftp in ASCII from SPDF." }, "Format": "Text", "Acknowledgement": "CDAWeb or nssdcftp, as appropriate, from NASA/GSFC/SPDF" }, { "RepositoryID": "spase://SMWG/Repository/NASA/GSFC/SPDF", "Availability": "Online", "AccessRights": "Open", "AccessURL": { "Name": "HTTP access to AT2 ASCII files at SPDF", "URL": "http://spdf.gsfc.nasa.gov/pub/data/ulysses/particle/cospin/at2/10min_new/", "Description": "AT1 data via http in ASCII from SPDF." }, "Format": "Text", "Acknowledgement": "CDAWeb or nssdcftp, as appropriate, from NASA/GSFC/SPDF" } ], "InstrumentID": "spase://SMWG/Instrument/Ulysses/COSPIN/AT", "MeasurementType": "EnergeticParticles", "TemporalDescription": { "TimeSpan": { "StartDate": "1990-10-22T00:00:00.000", "RelativeStopDate": "P9M" }, "Cadence": "PT10M" }, "ObservedRegion": "Heliosphere.Outer", "Parameter": { "Columns 1-5": { "Name": "Interval Start Time", "ParameterKey": "Columns 1-5", "Description": "\n Nominal Midpoint Time for the average given in year, day of year, \n hour, min, second.\n ", "Cadence": "PT10M", "Structure": { "Size": "5", "Element": [ { "Name": "Year", "Index": "1", "ValidMin": "1990", "ValidMax": "2009", "FillValue": "Null" }, { "Name": "Day of year", "Index": "2", "ValidMin": "1", "ValidMax": "366", "FillValue": "Null" }, { "Name": "Hour of day", "Index": "3", "ValidMin": "0", "ValidMax": "23", "FillValue": "Null" }, { "Name": "Minute of hour", "Index": "4", "ValidMin": "0", "ValidMax": "59", "FillValue": "Null" }, { "Name": "Seconds of minute", "Index": "5", "ValidMin": "0", "ValidMax": "59", "FillValue": "Null" } ] }, "Support": { "SupportQuantity": "Temporal" } }, "Column_6": { "Name": "COSPIN/ATN 0.7-0.9 MeV Proton Spin-Averaged Flux based on counting rate A1_N", "ParameterKey": "Column_6", "Description": "\n Nominal 10-minute average ATN spin-averaged flux based on counting rate A1_N responding \n primarily to 0.7-0.9 MeV protons.\n ", "Caveats": "\n 2.3 - 2.5 MeV helium nuclei, and possibly other high energy nuclei with\n similar energy losses in the front detector and similar ranges in Si may \n also contribute to this flux.\n ", "Cadence": "PT10M", "Units": "(counts/(s*cm^2*sr*MeV))", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35", "Particle": { "ParticleType": "Proton", "Qualifier": "Average", "ParticleQuantity": "NumberFlux", "EnergyRange": { "Low": "0.7", "High": "0.9", "Units": "MeV" } } }, "Column_7": { "Name": "COSPIN/ATN 0.9-1.3 MeV Proton Spin-Averaged Flux based on counting rate A2_N", "ParameterKey": "Column_7", "Description": "\n Nominal 10-minute average ATN spin-averaged flux based on counting rate A2_N responding \n primarily to 0.9-1.3 MeV protons.\n ", "Caveats": "\n 2.5 - 2.7 MeV helium nuclei, and possibly other high energy nuclei with\n similar energy losses in the front detector and similar ranges in Si may \n also contribute to this flux.\n ", "Cadence": "PT10M", "Units": "(counts/(s*cm^2*sr*MeV))", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35", "Particle": { "ParticleType": "Proton", "Qualifier": "Average", "ParticleQuantity": "NumberFlux", "EnergyRange": { "Low": "0.9", "High": "1.3", "Units": "MeV" } } }, "Column_8": { "Name": "COSPIN/ATN 1.3-2.2 MeV Proton Spin-Averaged Flux based on Counting Rate A3_N", "ParameterKey": "Column_8", "Description": "\n Nominal 10-minute average ATN spin-averaged based on counting rate A3_N responding \n primarily to 1.3-2.2 MeV protons.\n ", "Caveats": "\n 2.7 - 3.0 MeV helium nuclei, and possibly other high energy nuclei with\n similar energy losses in the front detector and similar ranges in Si may \n also contribute to this flux.\n ", "Cadence": "PT10M", "Units": "(counts/(s*cm^2*sr*MeV))", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35", "Particle": { "ParticleType": "Proton", "Qualifier": "Average", "ParticleQuantity": "NumberFlux", "EnergyRange": { "Low": "1.3", "High": "2.2", "Units": "MeV" } } }, "Column_9": { "Name": "COSPIN/ATN 2.2-3.6 MeV Proton Spin-Averaged Flux based on Counting Rate A4_N", "ParameterKey": "Column_9", "Description": "\n Nominal 10-minute average ATN spin-averaged flux based on counting rate A4_N responding \n to 2.2-3.6 MeV protons.\n ", "Caveats": "\n Discriminator and coincidence requirements exclude nuclei heavier than \n protons from contributing to this flux.\n ", "Cadence": "PT10M", "Units": "(counts/(s*cm^2*sr*MeV))", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35", "Particle": { "ParticleType": "Proton", "Qualifier": "Average", "ParticleQuantity": "NumberFlux", "EnergyRange": { "Low": "2.2", "High": "3.6", "Units": "MeV" } } }, "Column_10": { "Name": "COSPIN/ATN 3.6-6.5 MeV Proton Spin-Averaged flux based on Counting Rate A5_N", "ParameterKey": "Column_10", "Description": "\n Nominal 10-minute average ATN spin-averaged flux based on counting rate A5_N responding \n primarily to 3.6-6.5 MeV protons.\n ", "Caveats": "\n 24.0 - 28.0 MeV helium nuclei, and possibly other high energy nuclei with\n similar energy losses in the front detector and similar ranges in Si may \n also contribute to this flux.\n ", "Cadence": "PT10M", "Units": "(counts/(s*cm^2*sr*MeV))", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35", "Particle": { "ParticleType": "Proton", "Qualifier": "Average", "ParticleQuantity": "NumberFlux", "EnergyRange": { "Low": "3.6", "High": "6.5", "Units": "MeV" } } }, "Column_11": { "Name": "COSPIN/ATN 3.0-7.5 MeV Helium Spin-Averaged flux based on Counting Rate A38_N", "ParameterKey": "Column_11", "Description": "\n Nominal 10-minute average ATN spin-averaged flux based on counting rate A38_N responding \n primarily to 3.0-7.5 MeV helium nuclei (alpha particles).\n ", "Caveats": "\n Other, heavier nuclei with similar energy losses in the front \n\t detector and similar ranges in Si may also contribute to this flux.\n ", "Cadence": "PT10M", "Units": "(counts/(s*cm^2*sr*MeV))", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35", "Particle": { "ParticleType": "AlphaParticle", "Qualifier": "Average", "ParticleQuantity": "NumberFlux", "EnergyRange": { "Low": "3.0", "High": "7.5", "Units": "MeV" } } }, "Column_12": { "Name": "COSPIN/ATN 7.5-12.0 MeV Helium Spin-Averaged Counting Rate (A39_N)", "ParameterKey": "Column_12", "Description": "\n Nominal 10-minute average ATN spin-averaged counting rate responding \n primarily to 7.5-12.0 MeV helium nuclei (alpha particles).\n ", "Caveats": "\n Other, heavier nuclei with similar energy losses in the front \n\t detector and similar ranges in Si may also contribute to this counting rate.\n ", "Cadence": "PT10M", "Units": "(counts/(s*cm^2*sr*MeV))", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35", "Particle": { "ParticleType": "AlphaParticle", "Qualifier": "Average", "ParticleQuantity": "NumberFlux", "EnergyRange": { "Low": "7.5", "High": "12.0", "Units": "MeV" } } }, "Column_13": { "Name": "COSPIN/ATN 12.0-26.0 MeV Helium Spin-Averaged Flux based on Counting Rate A40_N", "ParameterKey": "Column_13", "Description": "\n Nominal 10-minute average ATN spin-averaged flux based on counting rate A40_N responding \n primarily to 12.0-26.0 MeV helium nuclei (alpha particles).\n ", "Caveats": "\n Other, heavier nuclei with similar energy losses in the front \n\t detector and similar ranges in Si may also contribute to this flux.\n ", "Cadence": "PT10M", "Units": "(counts/(s*cm^2*sr*MeV))", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35", "Particle": { "ParticleType": "AlphaParticle", "Qualifier": "Average", "ParticleQuantity": "NumberFlux", "EnergyRange": { "Low": "12.0", "High": "26.0", "Units": "MeV" } } }, "Columns_14-21": { "Name": "COSPIN/ATN 10-Minute Average Sectored Proton flux based on \n Counting Rate A3_NS", "ParameterKey": "Columns_14-21", "Description": "\n Nominal 10-minute average ATN 8-sectored fluxs based on the \n counting rate A3_NS responding primarily to 1.3-2.2 MeV protons.\n The rate has 8 elements, each corresponding to a 45 degree range of the \n spacecraft spin plane. The start of sector 1 (0 degrees) is coincident \n with the spacecraft-generated Sun-pulse, and the start of each \n subsequent sector is shifted by 45 degrees with respect to the preceding \n sector. For example, A3_N1 covers the azimuthal range 0-45 degrees, \n A3_N2 covers the azimuthal range 45-90 degrees, etc. In each sector,\n counts are registered only when the axis of the telescope view cone is \n within that sector.\n Data from multiple spacecraft spins contribute to the fluxes \n recorded for each sector, and the total accumulation time for the set of \n A3_N1-A3_N8 fluxes is required to be an integral number of spacecraft \n spins. Therefore the total accumulation time in each of the 8 sectors is \n 1/8 of the total time interval for the average.\n ", "Caveats": "\n 2.7 - 3.0 MeV helium nuclei, and possibly other high energy nuclei with\n similar energy losses in the front detector and similar ranges in Si may \n also contribute to these fluxes.\n ", "Cadence": "PT10M", "Structure": { "Size": "8", "Element": [ { "Name": "A3_N1", "Index": "1", "Units": "counts/(s*cm^2*sr*MeV)", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35" }, { "Name": "A3_N2", "Index": "2", "Units": "counts/(s*cm^2*sr*MeV)", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35" }, { "Name": "A3_N3", "Index": "3", "Units": "counts/(s*cm^2*sr*MeV)", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35" }, { "Name": "A3_N4", "Index": "4", "Units": "counts/(s*cm^2*sr*MeV)", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35" }, { "Name": "A3_N5", "Index": "5", "Units": "counts/(s*cm^2*sr*MeV)", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35" }, { "Name": "A3_N6", "Index": "6", "Units": "counts/(s*cm^2*sr*MeV)", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35" }, { "Name": "A3_N7", "Index": "7", "Units": "counts/(s*cm^2*sr*MeV)", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35" }, { "Name": "A3_N8", "Index": "8", "Units": "counts/(s*cm^2*sr*MeV)", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35" } ] }, "Particle": { "ParticleType": "Proton", "Qualifier": "Average", "ParticleQuantity": "NumberFlux", "EnergyRange": { "Low": "1.3", "High": "2.2", "Units": "MeV" } } }, "Columns_22-29": { "Name": "COSPIN/ATN 10-Minute Average Sectored Proton Fluxes based on Counting Rate \n A4_NS", "ParameterKey": "Columns_22-29", "Description": "\n Nominal 10-minute average ATN 8-sectored Proton Fluxes based on the Counting \n Rate A4_NS responding primarily to 2.2-3.6 MeV protons.\n The rate has 8 elements, each corresponding to a 45 degree range of the \n spacecraft spin plane. The start of sector 1 (0 degrees) is coincident \n with the spacecraft-generated Sun-pulse, and the start of each \n subsequent sector is shifted by 45 degrees with respect to the preceding \n sector. For example, A4_N1 covers the azimuthal range 0-45 degrees, \n A4_N2 covers the azimuthal range 45-90 degrees, etc. In each sector,\n counts are registered only when the axis of the telescope view cone is \n within that sector.\n Data from multiple spacecraft spins contribute to the fluxes \n recorded for each sector, and the total accumulation time for the set of \n A4_N1-A4_N8 fluxes is required to be an integral number of spacecraft \n spins. Therefore the total accumulation time in each of the 8 sectors is \n 1/8 of the total time interval for the average.\n ", "Caveats": "\n Discriminator and coincidence requirements exclude nuclei heavier than \n protons from contributing to these fluxes.\n ", "Cadence": "PT10M", "Structure": { "Size": "8", "Element": [ { "Name": "A4_N1", "Index": "1", "Units": "counts/(s*cm^2*sr*MeV)", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35" }, { "Name": "A4_N2", "Index": "2", "Units": "counts/(s*cm^2*sr*MeV)", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35" }, { "Name": "A4_N3", "Index": "3", "Units": "counts/(s*cm^2*sr*MeV)", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35" }, { "Name": "A4_N4", "Index": "4", "Units": "counts/(s*cm^2*sr*MeV)", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35" }, { "Name": "A4_N5", "Index": "5", "Units": "counts/(s*cm^2*sr*MeV)", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35" }, { "Name": "A4_N6", "Index": "6", "Units": "counts/(s*cm^2*sr*MeV)", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35" }, { "Name": "A4_N7", "Index": "7", "Units": "counts/(s*cm^2*sr*MeV)", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35" }, { "Name": "A4_N8", "Index": "8", "Units": "counts/(s*cm^2*sr*MeV)", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35" } ] }, "Particle": { "ParticleType": "Proton", "Qualifier": "Average", "ParticleQuantity": "NumberFlux", "EnergyRange": { "Low": "2.2", "High": "3.6", "Units": "MeV" } } }, "Columns_30-37": { "Name": "COSPIN/ATN 10-Minute Average Sectored Proton Fluxes based on \n Counting Rate A5_NS", "ParameterKey": "Columns_30-37", "Description": "\n Nominal 10-minute average ATN 8-sectored fluxes based on counting rate \n A5_NS responding primarily to 3.6-6.5 MeV protons.\n The rate has 8 elements, each corresponding to a 45 degree range of the \n spacecraft spin plane. The start of sector 1 (0 degrees) is coincident \n with the spacecraft-generated Sun-pulse, and the start of each \n subsequent sector is shifted by 45 degrees with respect to the preceding \n sector. For example, A5_N1 covers the azimuthal range 0-45 degrees, \n A5_N2 covers the azimuthal range 45-90 degrees, etc. In each sector,\n counts are registered only when the axis of the telescope view cone is \n within that sector.\n Data from multiple spacecraft spins contribute to the fluxes \n recorded for each sector, and the total accumulation time for the set of \n A5_N1-A5_N8 fluxes is required to be an integral number of spacecraft \n spins. Therefore the total accumulation time in each of the 8 sectors is \n 1/8 of the total time interval for the average.\n ", "Caveats": "\n 24.0-28.0 MeV helium nuclei, and possibly other high energy nuclei with\n similar energy losses in the front detector and similar ranges in Si may \n also contribute to these fluxes.\n ", "Cadence": "PT10M", "Structure": { "Size": "8", "Element": [ { "Name": "A5_N1", "Index": "1", "Units": "counts/(s*cm^2*sr*MeV)", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35" }, { "Name": "A5_N2", "Index": "2", "Units": "counts/(s*cm^2*sr*MeV)", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35" }, { "Name": "A5_N3", "Index": "3", "Units": "counts/(s*cm^2*sr*MeV)", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35" }, { "Name": "A5_N4", "Index": "4", "Units": "counts/(s*cm^2*sr*MeV)", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35" }, { "Name": "A5_N5", "Index": "5", "Units": "counts/(s*cm^2*sr*MeV)", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35" }, { "Name": "A5_N6", "Index": "6", "Units": "counts/(s*cm^2*sr*MeV)", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35" }, { "Name": "A5_N7", "Index": "7", "Units": "counts/(s*cm^2*sr*MeV)", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35" }, { "Name": "A5_N8", "Index": "8", "Units": "counts/(s*cm^2*sr*MeV)", "ValidMin": "0.0", "ValidMax": "1.00E+06", "FillValue": "-1.000E+35" } ] }, "Particle": { "ParticleType": "Proton", "Qualifier": "Average", "ParticleQuantity": "NumberFlux", "EnergyRange": { "Low": "3.6", "High": "6.5", "Units": "MeV" } } } } } } } }