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1) Ulysses COSPIN/AT Ion 10-Minute Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/COSPIN/AT/Fluxes/PT10M
Start:1990-10-22 00:00:00 Observatory:Ulysses Cadence:10 minutes
Stop:2014-01-24 01:00:51 Instrument:Anisotropy Telescopes Resource:NumericalData
10-Minute cadence proton and helium spin-averaged coincidence fluxes from the COSPIN Anisotropy Telescopes (AT1 and AT2). The two telescopes differ only by their orientation 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.

2) High Energy Telescope (HET) Housekeeping Parameters maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/COSPIN/HET/FullResolution/House
Start:1990-10-22 00:00:00 Observatory:Ulysses Cadence:
Stop:2009-06-29 23:59:59 Instrument:High Energy Telescope Resource:NumericalData
A directory containing daily ftp-downloadable files containing readout-by-readout listings of HET housekeeping paramaters (Voltages, Temperatures, Offsets). The naming convention of the files is uly_het_full_house_YYYDDD.txt, where YYY indicates the three-digit year since 1900 (e.g. YYY=090 for 1990, and YYY=102 for 2002) and DDD indicates the three digit day of year (Jan. 1 = 1). In each file, following a detailed description of the format, the data consist of a a listing of HET housekeeping parameters measured at the time listed in the first 4 columns of each line. Each line contains data for one readout of the parameters. The first 4 columns give the time of the measurement as fractional year (to 12 decimal places) and as year since 1900, day of year, and ms of day. At the most common science telemetry rate, 2048 bps, each parameter in this file is read out once every 256 seconds. The measurements are instantaneous, and do not represent an average of values over the interval since the last readout. The sole function of these parameters is to monitor instrument health. No noise-removal or despiking has been done, so caution must be used in interpreting isolated large increases or decreases in the measured parameters.

3) Ulysses COSPIN/HET High Energy Telescope Pulse Height Analyzed Events maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/COSPIN/HET/FullResolution/PHA
Start:1990-10-22 00:00:00 Observatory:Ulysses Cadence:
Stop:2009-06-29 23:59:59 Instrument:High Energy Telescope Resource:NumericalData
A directory containing daily ftp-downloadable files containing full information for every non-zero HET pulse-height event returned in telemetry, including raw channels and discriminator states, the energy deposits corresponding to the channels, and certain derived quantities including particle charge and trajectory through the telescope. Pulse height analysis is performed for electrons and nuclei with penetrating power equivalent to that of protons with energy greater than 14 MeV. The naming convention of the files is uly_het_full_pha_YYYDDD.txt, where YYY indicates the three-digit year since 1900 (e.g. YYY=090 for 1990, and YYY=102 for 2002) and DDD indicates the three digit day of year (Jan. 1 = 1). At the start of each file there isa detailed description of the format, in which each event is represented by a line with 54 columns that provide complete information about the event. The first 4 columns give the time of the opening of the window in which the event was recorded as fractional year (to 12 decimal places) and as year since 1900, day of year, and ms of day. At the most common science telemetry rate, 2048 bps, six events are collected in every 32 second telemetry format. Because of the large geometrical factor of the telescope, almost every available pha slot contains an event. Since far more events are recorded in the telescope than can be returned as pha events in the telemetry, only a sample of the events incident on the telescope can be sent down as pha events. With the pha data for an event, the particle's charge, mass, kinetic energy, and trajectory through the telescope can be determined. While most of the nuclei incident on the HET are protons, a three-level priority system selects events for pulse-height analyis and return in the telemetry so as to assure capture of almost all of the relatively rare heavy element nuclei that stop in the telescope. The lowest priority (P3) events are those that satisfy the most basic criteria for being an analyzable event, as determined by the combination of discriminators on various detectors in the telescope that fire. A higher priority (P2) is given to events that stop in the telescope, and the highest priority (P1) is given to events that stop in the telescope and that are identified as heavy nuclei by the size of their energy deposits in the detectors. The highest priority event that occurs in each window for accumulation of pha events is selected for inclusion in the telemetry data returned to the ground. Thus, in large solar energetic particle events with abundant heavy nuclei, few protons may be included in the pha events transmitted via telemetry. The counting rates, however, count every event, and in such cases it can usually be assumed the counting rates that respond to protons are dominated by the proton flux. Absolute fluxes for individual elements may be derived by identifying pha events that would contribute to counting rates (i.e. that have the same discriminator configuration as one of the counting rates) and determining the ratio between events counted by the rate and returned in telemetry during a given interval. Appropriate counting rates exist that match each of the three pha priority states. The priority levels corresponding to the counting rates are listed in Table 7 of Simpson et al. (Astron. Astrophys., 92, 365-399, 1972). *** N.B. Three corrections are necessary in Table 7 of Simpson et al. (1972). *** 1) The (H) discrimator logic should include the discriminator K6H orred with the other seven discriminators listed. 2) the middle term of the P2 (medium priority) logic should include D4 as well as D1, D2, and D6 as required detectors. 3) Because of an error in the logic design counting rate H3, listed as responding to P3 (lowest priority) events, also includes P2 events which satisfy the first term in the P2 logic. Thus H3 should not be used for deriving absolute fluxes of P3 events from PHA data.

4) Ulysses COSPIN/HET readout by readout counts and accumulation times for spin-averaged counting rates H1-H9 maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/COSPIN/HET/FullResolution/Rates/Omni1
Start:1990-10-22 00:00:00 Observatory:Ulysses Cadence:
Stop:2009-06-29 23:59:59 Instrument:High Energy Telescope Resource:NumericalData
A directory containing daily ftp-downloadable files containing readout-by-readout listings of the counts accumulated in the H1-H9 spin-averaged counting rates. These counting rates respond primarily to protons (H1-H5, H9) in the approximate energy ranges 5.4-14, 14-19, 24-31, 34-68, 68-92, and >92 MeV, respectively, and to electrons (H6-8) in the very approximate energy ranges 1-3, 5-10, and 3-5 MeV, respectively. The naming convention for the daily files is uly_het_full_rat_omni1_YYYDDD.txt, where YYY indicates the three-digit year since 1900 (e.g. YYY=090 for 1990, and YYY=102 for 2002) and DDD indicates the three digit day of year (Jan. 1 = 1). In each file, following a detailed description of the format, the data consist of a listing of counts accumulated in the H1-H9 spin-averaged counting rates during the intervals between successive readouts, organized into columns as described below. The first 4 columns give the start time of the counting rate accumulation period as fractional year (to 12 decimal places) and as year since 1900, day of year, and ms of day at the start of the accumulation, followed by 1 column giving the duration of the accumulation period in milli-seconds (it is the same for all 9 rates), and 9 columns giving the counts accumulated in that period for each rate. All fields except for the fractional year are in integer format. Each line contains data for one single readout of the rates H1-H9, and all readouts where at least one of the rates has a non-fill value are included. Where fill does occur it is indicated by -1. Since the accumulation period for each readout is forced to include an integral number of spacecraft spins in order to produce pure spin-averaged measurements, the lengths of the accumulation periods vary in a cyclic manner as the period of the telemetry cycle beats with the spacecraft spin period. All counting rates in this file are read out twice per spacecraft format. At the most common science telemetry bit rate (2048 bps) this corresponds to an average interval between readouts of 16 seconds. Thus, with a typical 5 rpm spacecraft spin rate the accumulation intervals vary in a repeating cycle of 12, 12, 24, 12, 12, 24, 12, etc. seconds. At lower bit rates the average interval is equal to 16x(2048/BR) seconds and the cycle automatically adjusts to produce this average accumulation. No noise-removal or despiking has been done, so caution must be used in interpreting isolated large increases or decreases in the counting rates.

5) Ulysses COSPIN/HET readout by readout counts and accumulation times for spin-averaged counting rates H10-H27. maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/COSPIN/HET/FullResolution/Rates/Omni2
Start:1990-10-22 00:00:00 Observatory:Ulysses Cadence:
Stop:2009-06-29 23:59:59 Instrument:High Energy Telescope Resource:NumericalData
A directory containing daily ftp-downloadable files containing readout-by-readout listings of the counts accumulated in the H1-H27 spin-averaged counting rates. The rates H10-H13 are coincidence counting rates corresponding primarily to heavy nuclei (Z>2) with penetrating power equivalent to carbon-12 nuclei in the approximate energy ranges 26-36, 44-127, 127-173, and >173 MeV/nucleon, resspectively. H14-H27 are single detector counting rates giving, in order, the total number of counts above the lowest level discriminator thresholds of detectors D1-D6, K1-K6 (or D7-D12), A (or D13), and the anti-coincidence scintillator S. The single detector counting rates are provided simply to assess the health of the detectors and are of little use scientifically. The naming convention for the daily files is uly_het_full_rat_omni2_YYYDDD.txt, where YYY indicates the three-digit year since 1900 (e.g. YYY=090 for 1990, and YYY=102 for 2002) and DDD indicates the three digit day of year (Jan. 1 = 1). In each file, following a detailed description of the format, the data consist of a listing of counts accumulated in the H10-H27 spin-averaged counting rates during the intervals between successive readouts, organized into columns as described below. The first 4 columns give the start time of the counting rate accumulation period as fractional year (to 12 decimal places) and as year since 1900, day of year, and ms of day at the start of the accumulation, followed by 1 column giving the duration of the accumulation period in milli-seconds (it is the same for all rates except H13, which is read out twice in each accumulation period, and is thus represented as H13a and H13b - see below and embedded documentation in each daily file), and 19 columns giving the counts accumulated in that period for each rate. All fields except for the fractional year are in integer format. The start time for H13a is the time given as the start time for the line, but (to sufficient accuracy) its accumulation period is half the period given under "coverage". Again, to sufficient accuracy, the start time for H13b is the time given plus half the accumulation period, and the accumulation period for H13b is half the period given under "coverage". Each line contains data for one single readout of the rates H10-H12, H13a, H13b, and H14-H27. All readouts where at least one of the rates has a non-fill value are included. Where fill does occur it is indicated by -1. Since the accumulation period for each readout is forced to include an integral number of spacecraft spins in order to produce pure spin-averaged measurements, the lengths of the accumulation periods vary in a cyclic manner as the period of the telemetry cycle beats with the spacecraft spin period. At the most common science telemetry rate, 2048 bps, each rate in this file is read out on average once every 128 seconds, except for H13 which is readout on average twice in every 128 seconds. At 2048 bps, the cycle of accumulation periods is 132, 132, 120, 132, 132,, 120, 132, ... seconds. No noise-removal or despiking has been done, so caution must be used in interpreting isolated large increases or decreases in the counting rates.

6) Ulysses COSPIN/HET readout by readout counts and accumulation times for the 8-sectored counting rate H7S. maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/COSPIN/HET/FullResolution/Rates/Sect1
Start:1990-10-22 00:00:00 Observatory:Ulysses Cadence:
Stop:2009-06-29 23:59:59 Instrument:High Energy Telescope Resource:NumericalData
A directory containing daily ftp-downloadable files containing readout-by-readout listings of the counts accumulated in each spin-sector of the 8-sectored H7S counting rate. Aside from its division of counts into spin-sectors, H7S is a coincidence counting rate with coincidence logic requirements identical to the spin-averaged counting rate H7. Therefore both the H7 and the H7S counting rates respond primarily to electrons in the very approximate energy range ~5-10 MeV. The naming convention for the daily files is uly_het_full_rat_sect1_YYYDDD.txt, where YYY indicates the three-digit year since 1900 (e.g. YYY=090 for 1990, and YYY=102 for 2002) and DDD indicates the three digit day of year (Jan. 1 = 1). In each file, following a detailed description of the format, the data consist of a readout by readout listing of counts accumulated in the eight 45 degree spin sectors of the sectored counting rate H7S during the intervals between successive readouts, organized into columns as described below. The first 4 columns give the start time of the counting rate accumulation period for sector 7 of the rate as fractional year (to 12 decimal places) and as year since 1900, day of year, and ms of day at the start of the accumulation, followed by 1 column (labeled cov) giving the duration of the total accumulation period for all 8 sectors in milli-seconds. Thus the accumulation period in each of the sectors is the value given in the "cov" column divided by 8. The accumulation in each of the successive sectors 7,8,1,2,3,4,5, and 6 starts cov/8 milliseconds after the start of the accumulation in the previous sector. Columns 6-13 then give the counts accumulated in each of the eight sectors during the accumulation period. Each line contains data for one single readout accumulation of the 8 sectors of H7S. Since the accumulation period for each readout is forced to include an integral number of spacecraft spins in order to produce equal coverage in all sectors, the lengths of the accumulation periods vary in a cyclic manner as the period of the telemetry cycle beats with the spacecraft spin period. The H7S counting rate is fully read out every 64 seconds at the most common science telemetry bit rate (2048 bps). Thus, with a typical 5 rpm spacecraft spin rate the accumulation intervals vary in a repeating cycle of 60, 60, 72, 60, 60, 72, 60, etc. seconds. At lower bit rates the average interval is equal to 64x(2048/BR) seconds and the cycle automatically adjusts to produce this average accumulation. The spin plane of the Ulysses spacecraft, in which the sectors are defined, is normal to the spin axis (spacecraft +Z axis), which is maintained within 1-2 degrees of Earth-pointing at all times. Viewed from Earth the spacecraft spins counter-clockwise. The start of sector 1 is defined by the spacecraft-generated Sun Pulse, which is issued when the sun crosses the +X/+Z quadrant of the X/Z plane. The HET telescope axis is parallel to the +X axis and normal to the Z axis. No noise-removal or despiking has been done, so caution must be used in interpreting isolated large increases or decreases in the counting rates.

7) Ulysses COSPIN/HET readout by readout counts and accumulation times for the 8-sectored counting rate H45S maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/COSPIN/HET/FullResolution/Rates/Sect2
Start:1990-10-22 00:00:00 Observatory:Ulysses Cadence:
Stop:2009-06-29 23:59:59 Instrument:High Energy Telescope Resource:NumericalData
A directory containing daily ftp-downloadable files containing readout-by-readout listings of the counts accumulated in each spin-sector of the 8-sectored H45S counting rate. Aside from its division of counts into spin-sectors, H45S is a coincidence counting rate with coincidence logic requirements satisfying the logical inclusive OR of the H4 and H5 spin- averaged counting rates. Therefore the H45S counting rate responds primarily to protons in the approximate energy range 34-92 MeV. The naming convention for the daily files is uly_het_full_rat_sect2_YYYDDD.txt, where YYY indicates the three-digit year since 1900 (e.g. YYY=090 for 1990, and YYY=102 for 2002) and DDD indicates the three digit day of year (Jan. 1 = 1). In each file, following a detailed description of the format, the data consist of a readout by readout listing of counts accumulated in the eight 45 degree spin sectors of the sectored counting rate H45S during the intervals between successive readouts, organized into columns as described below. The first 4 columns give the start time of the counting rate accumulation period for sector 7 of the rate as fractional year (to 12 decimal places) and as year since 1900, day of year, and ms of day at the start of the accumulation, followed by 1 column (labeled cov) giving the duration of the total accumulation period for all 8 sectors in milli-seconds. Thus the accumulation period in each of the sectors is the value given in the "cov" column divided by 8. The accumulation in each of the successive sectors 7,8,1,2,3,4,5, and 6 starts cov/8 milliseconds after the start of the accumulation in the previous sector. Columns 6-13 then give the counts accumulated in each of the eight sectors during the accumulation period. Each line contains data for one single readout accumulation of the 8 sectors of H45S. Since the accumulation period for each readout is forced to include an integral number of spacecraft spins in order to produce equal coverage in all sectors, the lengths of the accumulation periods vary in a cyclic manner as the period of the telemetry cycle beats with the spacecraft spin period. The H45S counting rate is fully read out every 128 seconds at the most common science telemetry bit rate (2048 bps). Thus, with a typical 5 rpm spacecraft spin rate the accumulation intervals vary in a repeating cycle of 132, 132, 120, 132, 132, 120, etc. seconds. At lower bit rates the average interval is equal to 128x(2048/BR) seconds and the cycle automatically adjusts to produce this average accumulation. The spin plane of the Ulysses spacecraft, in which the sectors are defined, is normal to the spin axis (spacecraft +Z axis), which is maintained within 1-2 degrees of Earth-pointing at all times. Viewed from Earth the spacecraft spins counter-clockwise. The start of sector 1 is defined by the spacecraft-generated Sun Pulse, which is issued when the sun crosses the +X/+Z quadrant of the X/Z plane. The HET telescope axis is parallel to the +X axis and normal to the Z axis. No noise-removal or despiking has been done, so caution must be used in interpreting isolated large increases or decreases in the counting rates.

8) Ulysses COSPIN/HET Daily Average Proton and Helium Fluxes in ASCII Format maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/COSPIN/HET/PH_Fluxes/P1D
Start:1990-10-23 00:00:00 Observatory:Ulysses Cadence:1 day
Stop:2009-06-30 23:59:59 Instrument:High Energy Telescope Resource:NumericalData
Daily average PHA-based proton and helium fluxes and errors from the COSPIN High Energy Telescope (HET) in the approximate energy ranges 39-70 MeV/n and 71-94 MeV/n from Day 296, 1990 through Day 181, 2009

9) Ulysses COSPIN/HET Ion and Electron 10-Minute Spin-Averaged Rate maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/COSPIN/HET/Rates/PT10M
Start:1990-10-22 00:00:00 Observatory:Ulysses Cadence:10 minutes
Stop:2014-01-24 01:00:51 Instrument:High Energy Telescope Resource:NumericalData
10-Minute average ion and electron spin-averaged coincidence counting rates from the COSPIN High Energy Telescope (HET). The parameter keys in the parameter-level segments below are specifically relevant to the UFA-accessible versions of the data.

10) Ulysses COSPIN/HET Ion and Electron 10-Minute Average Sectored Rate Data in ASCII Format maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/COSPIN/HET/Sectored-Rates/PT10M
Start:1990-10-22 00:00:00 Observatory:Ulysses Cadence:10 minutes
Stop:2014-01-24 01:00:52 Instrument:High Energy Telescope Resource:NumericalData
10-Minute average ion and electron 8-sectored coincidence counting rates from the COSPIN High Energy Telescope (HET). These data provide a measure of the anisotropy of particle arrival directions in the spacecraft spin plane

11) Ulysses COSPIN/HFT nominal 10 minute average fluxes of protons and heavier nuclei maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/COSPIN/HFT/Fluxes/PT10M
Start:1990-10-22 00:00:00 Observatory:Ulysses Cadence:10 minutes
Stop:2007-04-20 23:59:00 Instrument:High Flux Telescope Resource:NumericalData
Nominal 10 minute average spin-averages and sectored counting-rate-based fluxes of energetic protons and heavier nuclei from the Ulysses COSPIN High Flux Telescope. The parameter keys in the parameter-level segments below are specifically relevant to the UFA-accessible versions of the data.

12) Ulysses COSPIN/KET Proton, Helium and Electron Daily Average PHA Counr Rates in ASCII Format maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/COSPIN/KET/PHA/P1D
Start:1990-10-23 00:00:00 Observatory:Ulysses Cadence:1 day
Stop:2008-12-31 23:59:59 Instrument:Kiel Electron Telescope Resource:NumericalData
this set contains daily averaged PHA derived fluxes of protons (34.1-125.0, 125.0-320.0, 320.0-2100.0, >2100.0 MeV) alpha particles (34.2-125.0, 125.0-320.0, 320.0-2100.0, >2100.0 MeV/n) and electrons (2.5-7.0 Mev, 2.5 GV) and the Poisson uncertainties in those fluxes

13) Ulysses COSPIN/KET Proton, Helium and Electron 10-Minute Average Rates Data maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/COSPIN/KET/RATES/PT10M
Start:1990-10-23 00:00:00 Observatory:Ulysses Cadence:10 minutes
Stop:2008-12-31 23:59:59 Instrument:Kiel Electron Telescope Resource:NumericalData
This data set contains 10-Minute averages of: (a) spin-integrated count rates of protons (2.7-5.4, 5.4-23.1, 34.1-125.0, 125.0-320.0, 320.0-2100 and >2100.0 MeV), alpha particles (6.0-20.4, 34.2-125.0, 125.0-320.0, 320.0-2100.0 and >2100.0 MeV/n) and electrons (2.5-7.0, 7.0-170.0 and >170.0 MeV). (b) 8-sectored count rates of protons (5.4-23.1 MeV) and electrons (2.5-7.0 MeV); (c) count rates of D10, D20, C10, C20 and A01 single detector sensors. The parameter keys in the parameter-level segments below are specifically relevant to the UFA-accessible versions of the data.

14) Ulysses COSPIN/LET Proton and Helium Daily Average PHA Derived Fluxes in ASCII Format maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/COSPIN/LET/PHA/P1D
Start:1990-10-23 00:00:00 Observatory:Ulysses Cadence:1 day
Stop:2008-12-31 23:59:59 Instrument:Low Energy Telescope Resource:NumericalData
this set contains daily averaged PHA derived fluxes of protons (2-4, 4-6, 6-8, 8-16, 16-20 MeV) and alpha particles (4-6, 6-9, 11-20 MeV/n), and the Poisson uncertainties in those fluxes

15) Ulysses COSPIN/LET Oxygen, Nitrogen and Neon 20-Day Average PHA Derived Fluxes in ASCII Format maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/COSPIN/LET/PHA/P20D
Start:1990-10-23 00:00:00 Observatory:Ulysses Cadence:20 days
Stop:2008-12-31 23:59:59 Instrument:Low Energy Telescope Resource:NumericalData
this set contains 20-day averaged PHA derived fluxes of oxygen (4-8, 8-12, 12-16, 16-20 MeV/n), nitrogen (4-7, 8-20 MeV/n) and neon (4-8, 9-30 MeV/n) nuclei, and the Poisson uncertainties in those fluxes

16) Ulysses COSPIN/LET Ion and Electron 10-Minute Average Rates Data maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/COSPIN/LET/RATES/PT10M
Start:1990-10-23 00:00:00 Observatory:Ulysses Cadence:10 minutes
Stop:2008-12-31 23:59:59 Instrument:Low Energy Telescope Resource:NumericalData
This data set contains 10-Minute averages of: (a) spin-integrated fluxes of protons (0.9-1.2, 1.2-3.0, 1.8-3.8, 3.8-8.0 and 8.0-19.0 MeV), alpha particles (1.0-5.0, 1.9-3.7, 3.7-8.4 and 8.4-19.0 MeV/n), Li,Be,B nuclei (1.9-4.9 and 4.9-26 MeV/n), C,N,O nuclei (2.6-7.1 and 7.1-39 MeV/n)MeV/n), Z GE 10 nuclei (3.0-9.0 MeV/n), 10 LE Z LE 20 nuclei (9.0-50 MeV/n) and Z GE 20 nuclei (12-75 MeV/n); (b) 8-sectored proton fluxes (1.8-3.8 and 3.8-8.0 MeV); (c) count rates of electrons (0.3-1.0 MeV) and D1, D2, D3, D4 and D5 single detector sensors. The parameter keys in the parameter-level segments below are specifically relevant to the UFA-accessible versions of the data.

17) 17-min-Averaged Sectored Ulysses/HISCALE LEMS30 MFSA Z>1 Ion Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G100-17M
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:17 minutes
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
17-min-averaged sectored Z>1 ion fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE LEMS30 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the spacecraft rest frame.

18) Daily-Averaged Sectored Ulysses/HISCALE LEMS30 MFSA Z>1 Ion Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G100-1D
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:1 day
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
Daily-averaged sectored Z>1 ion fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE LEMS30 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the spacecraft rest frame.

19) Hourly-Averaged Sectored Ulysses/HISCALE LEMS30 MFSA Z>1 Ion Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G100-1H
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:1 hour
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
Hourly-averaged sectored Z>1 ion fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE LEMS30 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the spacecraft rest frame.

20) 17-min-Averaged Sectored Ulysses/HISCALE LEFS60 MFSA Z>1 Ion Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G101-17M
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:17 minutes
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
17-min-averaged sectored Z>1 ion fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE LEFS60 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the spacecraft rest frame.

21) Daily-Averaged Sectored Ulysses/HISCALE LEFS60 MFSA Z>1 Ion Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G101-1D
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:1 day
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
Daily-averaged sectored Z>1 ion fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE LEFS60 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the spacecraft rest frame.

22) Hourly-Averaged Sectored Ulysses/HISCALE LEFS60 MFSA Z>1 Ion Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G101-1H
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:1 hour
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
Hourly-averaged sectored Z>1 ion fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE LEFS60 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the spacecraft rest frame.

23) 17-min-Averaged Sectored Ulysses/HISCALE LEMS120 MFSA Z>1 Ion Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G102-17M
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:17 minutes
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
17-min-averaged sectored Z>1 ion fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE LEMS120 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the spacecraft rest frame.

24) Daily-Averaged Sectored Ulysses/HISCALE LEMS120 MFSA Z>1 Ion Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G102-1D
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:1 day
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
Daily-averaged sectored Z>1 ion fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE LEMS120 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the spacecraft rest frame.

25) Hourly-Averaged Sectored Ulysses/HISCALE LEMS120 MFSA Z>1 Ion Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G102-1H
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:1 hour
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
Hourly-averaged sectored Z>1 ion fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE LEMS120 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the spacecraft rest frame.

26) 17-min-Averaged Sectored Ulysses/HISCALE LEFS150 MFSA Z>1 Ion Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G103-17M
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:17 minutes
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
17-min-averaged sectored Z>1 ion fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE LEFS150 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the spacecraft rest frame.

27) Daily-Averaged Sectored Ulysses/HISCALE LEFS150 MFSA Z>1 Ion Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G103-1D
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:1 day
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
Daily-averaged sectored Z>1 ion fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE LEFS150 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the spacecraft rest frame.

28) Hourly-Averaged Sectored Ulysses/HISCALE LEFS150 MFSA Z>1 Ion Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G103-1H
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:1 hour
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
Hourly-averaged sectored Z>1 ion fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE LEFS150 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the spacecraft rest frame.

29) 17-min-Averaged Sectored Ulysses/HISCALE LEFS60 MFSA Electron Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G104-17M
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:17 minutes
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
17-min-averaged sectored electron fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE LEFS60 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the spacecraft rest frame.

30) Daily-Averaged Sectored Ulysses/HISCALE LEFS60 MFSA Electron Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G104-1D
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:1 day
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
Daily-averaged sectored electron fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE LEFS60 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the spacecraft rest frame.

31) Hourly-Averaged Sectored Ulysses/HISCALE LEFS60 MFSA Electron Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G104-1H
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:1 hour
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
Hourly-averaged sectored electron fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE LEFS60 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the spacecraft rest frame.

32) 17-min-Averaged Sectored Ulysses/HISCALE LEFS150 MFSA Electron Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G105-17M
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:17 minutes
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
17-min-averaged sectored electron fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE LEFS150 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the spacecraft rest frame.

33) Daily-Averaged Sectored Ulysses/HISCALE LEFS150 MFSA Electron Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G105-1D
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:1 day
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
Daily-averaged sectored electron fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE LEFS150 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the spacecraft rest frame.

34) Hourly-Averaged Sectored Ulysses/HISCALE LEFS150 MFSA Electron Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G105-1H
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:1 hour
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
Hourly-averaged sectored electron fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE LEFS150 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the spacecraft rest frame.

35) 17-min-Averaged Ulysses/HISCALE Spin-Averaged MFSA Proton Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G80-17M
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:17 minutes
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
17-min-averaged proton fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the solar wind rest frame.

36) Daily-Averaged Ulysses/HISCALE Spin-Averaged MFSA Proton Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G80-1D
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:1 day
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
Daily-averaged proton fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the solar wind rest frame.

37) Hourly-Averaged Ulysses/HISCALE Spin-Averaged MFSA Proton Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G80-1H
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:1 hour
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
Hourly-averaged proton fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the solar wind rest frame.

38) 17-min-Averaged Ulysses/HISCALE Spin-Averaged MFSA Electron Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G81-17M
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:17 minutes
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
17-min-averaged electron fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the solar wind rest frame.

39) Daily-Averaged Ulysses/HISCALE Spin-Averaged MFSA Electron Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G81-1D
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:1 day
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
Daily-averaged electron fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the solar wind rest frame.

40) Hourly-Averaged Ulysses/HISCALE Spin-Averaged MFSA Electron Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G81-1H
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:1 hour
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
Hourly-averaged electron fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the solar wind rest frame.

41) 17-min-Averaged Ulysses/HISCALE Spin-Averaged MFSA Z>1 Ion Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G82-17M
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:17 minutes
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
17-min-averaged ion fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the solar wind rest frame.

42) Daily-Averaged Ulysses/HISCALE Spin-Averaged MFSA Z>1 Ion Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G82-1D
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:1 day
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
Daily-averaged ion fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the solar wind rest frame.

43) Hourly-Averaged Ulysses/HISCALE Spin-Averaged MFSA Z>1 Ion Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G82-1H
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:1 hour
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
Hourly-averaged ion fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the solar wind rest frame.

44) 17-min-Averaged Sectored Ulysses/HISCALE LEMS30 MFSA Proton Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G83-17M
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:17 minutes
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
17-min-averaged sectored proton fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE LEMS30 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the solar wind rest frame.

45) Daily-Averaged Sectored Ulysses/HISCALE LEMS30 MFSA Proton Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G83-1D
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:1 day
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
Daily-averaged sectored proton fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE LEMS30 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the solar wind rest frame.

46) Hourly-Averaged Sectored Ulysses/HISCALE LEMS30 MFSA Proton Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G83-1H
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:1 hour
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
Hourly-averaged sectored proton fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE LEMS30 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the solar wind rest frame.

47) 17-min-Averaged Sectored Ulysses/HISCALE LEFS60 MFSA Proton Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G84-17M
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:17 minutes
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
17-min-averaged sectored proton fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE LEFS60 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the solar wind rest frame.

48) Daily-Averaged Sectored Ulysses/HISCALE LEFS60 MFSA Proton Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G84-1D
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:1 day
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
Daily-averaged sectored proton fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE LEFS60 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the solar wind rest frame.

49) Hourly-Averaged Sectored Ulysses/HISCALE LEFS60 MFSA Proton Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G84-1H
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:1 hour
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
Hourly-averaged sectored proton fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE LEFS60 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the solar wind rest frame.

50) 17-min-Averaged Sectored Ulysses/HISCALE LEMS120 MFSA Proton Fluxes maxmize
Resource ID:spase://VEPO/NumericalData/Ulysses/HISCALE/MFSA/G85-17M
Start:1990-01-01 00:00:00 Observatory:Ulysses Cadence:17 minutes
Stop:2007-12-31 23:59:59 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
17-min-averaged sectored proton fluxes from the MF Spectrum Analyzer of the Ulysses/HISCALE LEMS120 instrument. All energies thresholds take into account the incident particle type, shielding, and inactive dead-layer of the solid state detector. All fluxes are background corrected and are in the solar wind rest frame.

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