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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:2015-12-14 07:55:42 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:2015-12-14 07:55:42 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:2015-12-14 07:55:42 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) Ulysses COSPIN ion and electron fluxes, plots maxmize
Resource ID:spase://VSPO/DisplayData/Ulysses/COSPIN/PLOTS
Start:1990-10-23 00:00:00 Observatory:Ulysses Cadence:
Stop:2008-08-31 00:00:00 Instrument:Cosmic Ray and Solar Particles (SIM/COSPIN) Resource:DisplayData
Plots of ion (many Z) and electron fluxes, various resolutions

18) Ulysses Dust Detection System Data maxmize
Resource ID:spase://VSPO/NumericalData/Ulysses/DUST/PT1M
Start:1990-10-27 18:53:00 Observatory:Ulysses Cadence:1 minute
Stop:1992-12-31 23:18:00 Instrument:Cosmic Dust (GRU/DUST) Resource:NumericalData
This data set contains information collected by the Ulysses Cosmic Dust instrument on the dust environment in interplanetary space within the inner solar system, between Jupiter and the Sun, and at high polar latitudes of the Sun. Both interplanetary and interstellar dust particles have been detected. This information is collected with a dust impact experiment, from which may be inferred direction of motion, mass, velocity and charge (see ULYDINST.CAT). The data presented in this dataset include instrumental readouts, inferred metadata, calibration information and a calendar of events.

19) Ulysses EPAC full-resolution rates and fluxes at SPDF maxmize
Resource ID:spase://VSPO/NumericalData/Ulysses/EPAC/GSFC/SPDF/PT1H
Start:1991-01-01 00:00:00 Observatory:Ulysses Cadence:1 hour
Stop:2008-08-31 00:00:00 Instrument:Ulysses Energetic Particle Composition (EPAC) Experiment Resource:NumericalData
Full resolution proton and electron fluxes, plus many count rates in annual files

20) Ulysses EPAC hourly rates and fluxes, CDAWeb maxmize
Resource ID:spase://VSPO/NumericalData/Ulysses/EPAC/GSFC/SPDF/PT3600.00S
Start:1991-01-01 00:00:00 Observatory:Ulysses Cadence:3600.00 seconds
Stop:1997-12-31 00:00:00 Instrument:Ulysses Energetic Particle Composition (EPAC) Experiment Resource:NumericalData
Hourly proton and electron fluxes with spectral and directional information

21) Ulysses EPAC flux plots maxmize
Resource ID:spase://VSPO/DisplayData/Ulysses/EPAC/PLOTS
Start:1990-10-19 00:00:00 Observatory:Ulysses Cadence:
Stop:1998-12-31 00:00:00 Instrument:Ulysses Energetic Particle Composition (EPAC) Experiment Resource:DisplayData
27-day and annual plots of selected proton and electron fluxes, plus some count rates

22) Ulysses EPAC daily pulse height data maxmize
Resource ID:spase://VSPO/NumericalData/Ulysses/EPAC/UFA/PHA/PT1H
Start:1990-10-19 00:00:00 Observatory:Ulysses Cadence:1 hour
Stop:1998-12-31 00:00:00 Instrument:Ulysses Energetic Particle Composition (EPAC) Experiment Resource:NumericalData
Daily accumulations of pulse height analysis data in annual files

23) Ulysses EPAC full-resolution rates and fluxes maxmize
Resource ID:spase://VSPO/NumericalData/Ulysses/EPAC/UFA/PT1H
Start:1991-01-01 00:00:00 Observatory:Ulysses Cadence:1 hour
Stop:2008-08-31 00:00:00 Instrument:Ulysses Energetic Particle Composition (EPAC) Experiment Resource:NumericalData
Full resolution proton and electron fluxes, plus many count rates in annual files

24) Ulysses Trajectory Data in Geocentric Coordinates maxmize
Resource ID:spase://VSPO/NumericalData/Ulysses/Ephemeris/Geocentric/P1D
Start:1990-11-04 00:00:00 Observatory:Ulysses Cadence:1 day
Stop:2001-12-12 00:00:00 Instrument:Ulysses Positions Resource:NumericalData
Daily Ulysses position data for cruise, prime and extenxed mission in geocentric coordinates.

25) Ulysses Trajectory Data in Heliocentric Coordinates maxmize
Resource ID:spase://VSPO/NumericalData/Ulysses/Ephemeris/Heliocentric/P1D
Start:1990-11-04 00:00:00 Observatory:Ulysses Cadence:1 day
Stop:2001-12-12 00:00:00 Instrument:Ulysses Positions Resource:NumericalData
Daily Ulysses position data for cruise, prime and extenxed mission in heliocentric coordinates.

26) Ulysses Trajectory Data During Encounter with Jupiter 1992-1995 maxmize
Resource ID:spase://VSPO/NumericalData/Ulysses/Ephemeris/Jupiter/P1D
Start:1992-01-05 00:00:00 Observatory:Ulysses Cadence:1 day
Stop:1995-10-31 00:00:00 Instrument:Ulysses Positions Resource:NumericalData
Daily Ulysses position during encounter with Jupiter in 1992-1995 as daily and SPICE data.

27) Ulysses Trajectory Data SEDR maxmize
Resource ID:spase://VSPO/NumericalData/Ulysses/Ephemeris/P1D
Start:1990-10-01 00:00:00 Observatory:Ulysses Cadence:1 day
Stop:2009-06-30 00:00:00 Instrument:Ulysses Positions Resource:NumericalData
This trajectory data set is provided by NSSDC. NSSDC has been actively supporting the Ulysses mission from the start by providing up-to-date trajectory-related data and graphics to the investigator community and the cognizant NASA Headquarters personnel. Soon after the launch, NSSDC generated (and later updated after Jupiter encounter) and loaded online for public access a list file of daily coordinates for Ulysses, along with software to manipulate these Cartesian coordinates into other sets, notably the heliographic latitude/longitude/radial distance. Similar online files of all other heliospheric spacecraft enable computations of their relative locations. The NSSDC Report 91-08, "Trajectories of Inner and Outer Heliospheric Spacecraft," has been requested often. (Higher resolution data may be obtained by executing the online code in DECnet: RUN NSSDCA::ANON_DIR:[ACTIVE.HELIO]HELICOOR.

28) Ulysses magnetic field 1-min data maxmize
Resource ID:spase://VSPO/NumericalData/Ulysses/FGM/GSFC/SPDF/PT1M
Start:1990-10-25 00:00:00 Observatory:Ulysses Cadence:1 minute
Stop:2009-06-30 00:00:00 Instrument:Magnetic Field (HED/VHM/FGM) Resource:NumericalData
This data set contains high resolution samples at about one-minute intervals of the interplanetary magnetic field measured by the Ulysses Magnetic Field experiment. Field vector components are given in units ofnanoteslas and in RTN coordinates, where R is the radial component or the sun-s/c axis, T is the transverse (along-track) component or the cross product of the solar rotation axis and R, and N is the normal (cross-track) component or the cross product of R and T. The field magnitudes in nT are averages of scalar magnitudes at higher time resolution. Times are computed at the mid-point of each minute interval and expressed in Spacecraft Event Time - UT (SCET-UT). Data gaps have not been flagged in any way - if there were no available data in a particular hour then there is no data record for that hour. No data from the Feb. 1992 encounter with Jupiter are included. Each file includes one day of data. Further details on the magnetic field measurements can be found in the following reference: Balogh, A., et al., Astron. Astrophys. Suppl. Ser., 92(2), 221, 1992.

29) Ulysses magnetic field 1-hr data maxmize
Resource ID:spase://VSPO/NumericalData/Ulysses/FGM/GSFC/SPDF/PT3600S
Start:1990-10-25 00:00:00 Observatory:Ulysses Cadence:3600 seconds
Stop:2009-06-30 23:59:59 Instrument:Magnetic Field (HED/VHM/FGM) Resource:NumericalData
This data set contains high resolution samples at about one-hour intervals 1hrof the interplanetary magnetic field measured by the Ulysses Magnetic Field experiment. Field vector components are given in units ofnanoteslas and in RTN coordinates, where R is the radial component or the sun-s/c axis, T is the transverse (along-track) component or the cross product of the solar rotation axis and R, and N is the normal (cross-track) component or the cross product of R and T. The field magnitudes in nT are averages of scalar magnitudes at higher time resolution. Times are computed at the mid-point of each minute interval and expressed in Spacecraft Event Time - UT (SCET-UT). Data gaps have not been flagged in any way - if there were no available data in a particular hour then there is no data record for that hour. No data from the Feb. 1992 encounter with Jupiter are included. Each file includes one day of data. Further details on the magnetic field measurements can be found in the following reference: Balogh, A., et al., Astron. Astrophys. Suppl. Ser., 92(2), 221, 1992.

30) Ulysses magnetic field data plots at ESA maxmize
Resource ID:spase://VSPO/DisplayData/Ulysses/FGM/PLOTS
Start:1990-10-25 00:00:00 Observatory:Ulysses Cadence:
Stop:2008-08-31 00:00:00 Instrument:Magnetic Field (HED/VHM/FGM) Resource:DisplayData
1-min and 1-hour Ulysses magnetic field data at ESA, also 1-sec data for 1990-3

31) Ulysses magnetic field data files at ESA maxmize
Resource ID:spase://VSPO/NumericalData/Ulysses/FGM/UFA/PT1M
Start:1990-10-25 00:00:00 Observatory:Ulysses Cadence:1 minute
Stop:2008-08-31 00:00:00 Instrument:Magnetic Field (HED/VHM/FGM) Resource:NumericalData
1-min and 1-hour Ulysses magnetic field data at ESA, also 1-sec data for 1990-3; field magnitude and RTN components

32) Ulysses GAS UV Full-Sky Data maxmize
Resource ID:spase://VSPO/NumericalData/Ulysses/GAS/Full-Sky/PT24H
Start:1990-10-27 00:00:00 Observatory:Ulysses Cadence:24 hours
Stop:2007-08-18 23:59:59 Instrument:Ulysses Interstellar Neutral Gas (GAS) Experiment Resource:NumericalData
This Ulysses GAS experiment data set consists of pixel map data and image files for sky maps generated from GAS measurements in a mode primarily sensitive to ultraviolet photons. The accumulated counts and Ecliptic (spacecraft-centered) angle coordinates for each sky map pixel are given in the ascii files *.TXT. The positions of the Sun and the planets vary with time and with the position of the spacecraft along its trajectory, while the positions of stars remain fixed. The full images are provided in GIF (*.GIF files) and postscript (*.PS files) format, the GIF files being easily viewed on-line (see below) with an Internet web browser. The actual positions of Sun, Earth, and Jupiter are indicated by yellow, green, and white dots, respectively. The area around the Sun is excluded from observation to avoid damaging intensities from direct sunlight. The files USER_GUIDE.TXT, FORMAT.TXT, and REFERENCE.TXT, respectively, give an overall description of the various datatypes, the record format for the DATA datatype, and a list of GAS-related publications. The users guide defines the nomenclature of the file names.

33) Ulysses GAS Interstellar Helium Maps maxmize
Resource ID:spase://VSPO/NumericalData/Ulysses/GAS/Interstellar-Helium/PT24H
Start:1990-10-27 00:00:00 Observatory:Ulysses Cadence:24 hours
Stop:2007-11-25 23:59:59 Instrument:Ulysses Interstellar Neutral Gas (GAS) Experiment Resource:NumericalData
This Ulysses GAS experiment data set consists of pixel map data and image files for sky maps generated from GAS measurements in the mode primarily sensitive to neutral helium atoms from inflow of interstellar gas into the heliosphere. The accumulated counts and Ecliptic (spacecraft-centered) angle coordinates for each sky map pixel are given in the ascii files *.TXT. The positions of the Sun and the planets vary with time and with the position of the spacecraft along its trajectory, while the positions of stars remain fixed. The full images are provided in GIF (*.GIF files) and postscript (*.PS files) format, the GIF files being easily viewed on-line (see below) with an Internet web browser. The actual positions of Sun, Earth, and Jupiter are indicated by yellow, green and white dots, respectively. The area around the Sun is excluded from observation to avoid damaging intensities from direct sunlight. The files USER_GUIDE.TXT, FORMAT.TXT, and REFERENCE.TXT, respectively, give an overall description of the various datatypes, the record format for the DATA datatype, and a list of GAS-related publications. The users guide defines the nomenclature of the file names. Further details about the data and the experiment may be found in Witte et al., Astron. Astrophys. Suppl. Ser., 92, No. 2, 333-348, 1992 (NSSDC TRF # B40459-000A). Data analysis methods for interstellar helium are described in Banaszkiewicz et al., Astron. Astrophys. Suppl. Ser., 120, 587-602, 1996 (B45706-000A).

34) Ulysses HISCALE ion and electron fluxes at Funtech maxmize
Resource ID:spase://VSPO/NumericalData/Ulysses/HISCALE/FTECS/PT12S
Start:1990-11-14 00:00:00 Observatory:Ulysses Cadence:12 seconds
Stop:2008-08-31 00:00:00 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
Ion and electron fluxes, various time resolutions, spin-sectored and spin-averaged, ASCII files accessible directly from Fundamental Technologies or through the Virtual Energetic Particle Observatory (VEPO).

35) Ulysses HISCALE LEM120 ion and electron counts maxmize
Resource ID:spase://VSPO/NumericalData/Ulysses/HISCALE/GSFC/SPFD/ELECTRON120_COUNTS/PT2M
Start:1990-11-14 00:00:00 Observatory:Ulysses Cadence:2 minutes
Stop:2008-12-31 00:00:00 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
This data set contains 1-hour spin averaged count rates of the ion and electron from the Ulysses Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies (HI-SCALE) Low Energy Foil Spectrometer at 120 degrees to the spacecraft spin axis. Count rate units are /s. For references, see Astron. Astrophys. Suppl. Ser., 92(2), 349-363, 1992.

36) Ulysses HISCALE LEFS150 ion and electron counts maxmize
Resource ID:spase://VSPO/NumericalData/Ulysses/HISCALE/GSFC/SPFD/ELECTRON150_COUNTS/PT2M
Start:1990-11-14 00:00:00 Observatory:Ulysses Cadence:2 minutes
Stop:2008-12-31 00:00:00 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
This data set contains 1-hour spin averaged count rates of the ion and electron from the Ulysses Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies (HI-SCALE) Low Energy Foil Spectrometer at 150 degrees to the spacecraft spin axis. Count rate units are /s. For references, see Astron. Astrophys. Suppl. Ser., 92(2), 349-363, 1992.

37) Ulysses HISCALE LEMSDE deflected electron counts maxmize
Resource ID:spase://VSPO/NumericalData/Ulysses/HISCALE/GSFC/SPFD/ELECTRON30D_COUNTS/PT2M
Start:1990-11-14 00:00:00 Observatory:Ulysses Cadence:2 minutes
Stop:2008-12-31 00:00:00 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
This data set contains 1-hour spin averaged count rates of the deflected electron from the Ulysses Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies (HI-SCALE) Low Energy Foil Spectrometer at 30 degrees to the spacecraft spin axis. Count rate units are /s. For references, see Astron. Astrophys. Suppl. Ser., 92(2), 349-363, 1992.

38) Ulysses HISCALE LEMS30 ion and electron counts maxmize
Resource ID:spase://VSPO/NumericalData/Ulysses/HISCALE/GSFC/SPFD/ELECTRON30_COUNTS/PT2M
Start:1990-11-14 00:00:00 Observatory:Ulysses Cadence:2 minutes
Stop:2008-12-31 00:00:00 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
This data set contains 1-hour spin averaged count rates of the ion and electron from the Ulysses Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies (HI-SCALE) Low Energy Foil Spectrometer at 30 degrees to the spacecraft spin axis. Count rate units are /s. For references, see Astron. Astrophys. Suppl. Ser., 92(2), 349-363, 1992.

39) Ulysses HISCALE LEFS60 ion and electron counts maxmize
Resource ID:spase://VSPO/NumericalData/Ulysses/HISCALE/GSFC/SPFD/ELECTRON60_COUNTS/PT2M
Start:1990-11-14 00:00:00 Observatory:Ulysses Cadence:2 minutes
Stop:2008-12-31 00:00:00 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
This data set contains 1-hour spin averaged count rates of the ion and electron from the Ulysses Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies (HI-SCALE) Low Energy Foil Spectrometer at 60 degrees to the spacecraft spin axis. Count rate units are /s. For references, see Astron. Astrophys. Suppl. Ser., 92(2), 349-363, 1992.

40) Ulysses HISCALE 1-hour ion counts maxmize
Resource ID:spase://VSPO/NumericalData/Ulysses/HISCALE/GSFC/SPFD/ION60_COUNTS/PT2M
Start:1990-11-14 00:00:00 Observatory:Ulysses Cadence:2 minutes
Stop:2008-12-31 00:00:00 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
This data set contains 1-hour spin averaged count rates of the ion data from the Ulysses Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies (HI-SCALE) Composition Aperture Telescope at 60 degrees to the spacecraft spin axis. Count rate units are /s. For references, see Astron. Astrophys. Suppl. Ser., 92(2), 349-363, 1992.

41) Ulysses HISCALE 1-hour proton counts maxmize
Resource ID:spase://VSPO/NumericalData/Ulysses/HISCALE/GSFC/SPFD/PROTON60_COUNTS/PT2M
Start:1990-11-14 00:00:00 Observatory:Ulysses Cadence:2 minutes
Stop:2008-12-31 00:00:00 Instrument:Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies Resource:NumericalData
This data set contains 1-hour spin averaged count rates of proton data from the Ulysses Heliosphere Instrument for Spectra, Composition and Anisotropy at Low Energies (HI-SCALE) Composition Aperture Telescope at 60 degrees to the spacecraft spin axis. Count rate units are /s. For references, see Astron. Astrophys. Suppl. Ser., 92(2), 349-363, 1992.

42) 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.

43) 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.

44) 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.

45) 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.

46) 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.

47) 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.

48) 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.

49) 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.

50) 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.

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