2.4.1 spase://CNES/NumericalData/CDPP-AMDA/ULYSSES/FGM/ulys-fgm-rtn all mission 2012-03-06T22:23:03Z This data set contains high resolution samples at about one-second intervals of the interplanetary magnetic field measured by the Ulysses Magnetic Field experiment. Field vector components are given in units of nanoteslas and in RTN coordinates, where R is the sun-s/c axis, T is the cross product of the solar rotation axis and R, and T is 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 averaging 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. Parameter key information given below is specific to the data version at nssdcftp and at the ESA Research and Scientific Support Department site identified below. 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. Please acknowledge the Principal Investigator, A. Balogh of Imperial College, London, UK. and the repository from which you accessed the data. spase://SMWG/Person/Andre.Balogh PrincipalInvestigator spase://SMWG/Person/Joyce.E.Wolf TechnicalContact Ulysses Magnetometer Home Page http://ufa.esac.esa.int/ufa/#instruments Site hosting instrument information, data and plots for Ulysses magnetometer spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA HAPI Server https://amda.irap.omp.eu/service/hapi ulys-fgm-rtn Web Service to this product using the HAPI interface. CSV Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers. spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA Web application https://amda.cdpp.eu Access to Data via CDPP/AMDA Web application. CSV VOTable CDF PNG Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers. CDAWeb UY_1SEC_VHM spase://CNES/Instrument/CDPP-AMDA/Ulysses/FGM MagneticField 1990-10-25T16:50:45Z 2009-06-27T23:59:34Z PT1S Heliosphere.Inner Heliosphere.Outer Heliosphere.NearEarth b_rtn b_ulys_rtn phys.magField nT 1e-9>T Cartesian RTN TimeSeries 3 br 1 b_ulys_rtn(0) bt 2 b_ulys_rtn(1) bn 3 b_ulys_rtn(2) Vector Magnetic |b| b_ulys_mag Scalar magnitude of the magnetic field in nT phys.magField nT 1e-9>T TimeSeries Magnitude Magnetic phi b_ulys_rtn_phi Magnetic field phi angle phys.magField degrees 1e-9>T TimeSeries 1 Magnetic theta b_ulys_rtn_theta Magnetic field theta angle phys.magField degrees 1e-9>T TimeSeries 1 Magnetic