2.3.2 spase://NASA/NumericalData/Ulysses/MAGandPLS/PT1H Ulysses hourly merged magnetic field and plasma data 2021-04-27T15:38:11Z This is an hourly resolution, merged magnetic field and plasma data set created at NSSDC for COHOWeb. Magnetic field vectors and plasma flow direction angles are given in RTN coordinates. Spacecraft position data are given in Heliographic inertial (HGI) coordinates. Please acknowledge the magnetic field and plasma Principal Investigators, Drs. A. Balogh and D. McComas, and NSSDC or GSFC-SPDF spase://SMWG/Person/Andre.Balogh PrincipalInvestigator spase://SMWG/Person/David.J.McComas PrincipalInvestigator spase://SMWG/Person/Natalia.E.Papitashvili GeneralContact Readme file at SPDF https://spdf.gsfc.nasa.gov/pub/data/ulysses/merged/ulymgd.txt SWOOPS data users' guide https://spdf.gsfc.nasa.gov/pub/data/ulysses/plasma/swoops/ion/swoops_ion_users_guide_update_20030214.txt spase://VHO/NumericalData/Ulysses/MAGandPLS/PT1H spase://VSPO/NumericalData/Ulysses/MAGandPLS/PT1H spase://SMWG/Repository/NASA/GSFC/SPDF Online Open FTPS from SPDF (not with most browsers) ftps://spdf.gsfc.nasa.gov/pub/data/ulysses/merged/ for annual files via ftp HTTPS from SPDF https://spdf.gsfc.nasa.gov/pub/data/ulysses/merged/ In CDF via HTTP from SPDF CDAWeb https://cdaweb.gsfc.nasa.gov/cgi-bin/eval2.cgi?dataset=UY_COHO1HR_MERGED_MAG_PLASMA&index=sp_phys UY_COHO1HR_MERGED_MAG_PLASMA access to subset, plot, and list functionalities from CDAWeb COHOWeb plots and lists https://omniweb.sci.gsfc.nasa.gov/coho/form/ulysses.html Ulysses-specific page for plots and lists COHOweb top page https://omniweb.sci.gsfc.nasa.gov/coho/ Plots, lists, scatter plots, regressions, distributions, means, etc. Text 1 MB P1Y Please acknowledge the magnetic field and plasma Principal Investigators, Drs. A. Balogh and D. McComas, and NSSDC or GSFC-SPDF spase://SMWG/Repository/NASA/GSFC/SPDF Online Open CDAWeb HAPI Server https://cdaweb.gsfc.nasa.gov/hapi UY_COHO1HR_MERGED_MAG_PLASMA Web Service to this product using the HAPI interface. CSV Please acknowledge the magnetic field and plasma Principal Investigators, Drs. A. Balogh and D. McComas, and NSSDC or GSFC-SPDF spase://SMWG/Instrument/Ulysses/FGM spase://SMWG/Instrument/Ulysses/SWOOPS MagneticField ThermalPlasma 1990-10-25T00:00:00 2008-10-18T00:00:00 Plasma data do not start until Nov. 18, 1990. As of 12/31/2008, magnetic field data end on Feb. 29, 2008. Plasma data become quite sparse after ~May 19, 2008. Data may be extended. PT1H Heliosphere.Outer Magnetic Field Magnitude Column10 Hourly average of fine time scale magnetic field magnitudes PT1H nT 999.99 Magnitude Magnetic Magnetic Field Vector Hourly averages of RTN components of fine time scale magnetic field vectors PT1H nT Cartesian RTN 3 R,T,N components R component Component.I 1 Column07 T component Component.J 2 Column08 N component Component.K 3 Column09 999.99 Vector Magnetic Flow speed Column12 Hourly averaged solar wind plasma flow speed PT1H km/s 9999.9 Proton Average FlowSpeed Flow elevation angle Column13 Hourly averaged solar wind plasma flow elevation angle PT1H deg Spherical RTN 9999.9 Proton DirectionAngle.ElevationAngle FlowVelocity Flow azimuth angle Column14 Hourly averaged solar wind plasma flow azimuthal angle PT1H Spherical RTN 9999.9 Proton DirectionAngle.AzimuthAngle FlowVelocity Proton density Column15 Hourly averaged solar wind proton plasma density PT1H n/cc 99.99999 Proton Average NumberDensity Alpha particle density Column16 Hourly averaged solar wind alpha particle plasma density PT1H n/cc 99.99999 AlphaParticle Average NumberDensity Large Temperature Column17 Hourly averaged solar wind plasma temperature deteremined as the integral of the distribution in three-dimensional velocity space over all energy channels and angle bins that are statistically above noise PT1H degK 9999999. Proton Average Temperature Small Temperature Column18 Hourly averaged solar wind plasma temperature estimated by summing over angle the observations at a fixed energy. The moments of the resulting one dimensional plasma spectrum are then summed and the resulting RR (radial) component of the temperature tensor is used as the estimate of proton temperature. PT1H degK 9999999. Proton Average Temperature Ulysses radial distance Column04 Heliocentric radial distance of Ulysses in AU PT1H AU Positional Ulysses latitude Column05 Heliographic Inertial elevation angle of Ulysses in deg PT1H deg Spherical HGI Positional Ulysses longitude Column06 Heliographic Inertial azimuthal angle of Ulysses in deg PT1H deg Spherical HGI Positional