2.4.1 spase://CNES/NumericalData/CDPP-AMDA/ULYSSES/URAP/ulys-urap-mag magnetic field 2012-03-06T22:15:53Z The B magnitude measurements are given in nanoTesla and are obtained by the detection of power spectrum relative minima at the harmonics of the gyrofrequency (firstly published in Meyer et al., J. Geophys. Res., 98, 21163-21176,1993 and references therein) . The given acquisition time is the elapsed time (UT) of the sweeping receiver at the highest harmonic acquisition. spase://SMWG/Person/Elena.Budnik GeneralContact uly-urap-lesia PartOf io torus QTN spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA HAPI Server https://amda.irap.omp.eu/service/hapi ulys-urap-mag 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. LESIA spase://CNES/Instrument/CDPP-AMDA/Ulysses/URAP MagneticField 1992-02-08T15:44:21Z 1992-02-08T22:42:01Z PT104S PT324S Jupiter |b| ulys_urap_bmag phys.magField nT TimeSeries Magnitude Magnetic