2.2.6 spase://CNES/NumericalOutput/CDPP-AMDA/KT17/b_kt17 KT17 along s/c orbit 2023-02-17T00:00:00Z Magnetic field along S/C orbit at Mercury is being real-time calculated. S/C, sampling time, distance of Mercury from the Sun (AU) and Anderson et al., 2013 disturbance index should be defined by user. KT17 magnetic field model (Korth et al., 2017) model is used in calculations. James, M. K. - KT17 (v1.0.0) - https://github.com/mattkjames7/KT17/releases/tag/v1.0.0 spase://CNES/Person/CDPP-AMDA/Haje.Korth PrincipalInvestigator spase://CNES/Person/CDPP-AMDA/M.K.James TechnicalContact Korth, H., Johnson, C. L., Philpott, L., Tsyganenko, N. A., Anderson, B. J. (2017). A dynamic model of Mercury's magnetospheric magnetic field. Geophysical Research Letters, 44, 10,147– 10,154. https://doi.org/10.1002/2017GL074699 Model description James, M. K. - KT17 (v1.0.0) https://github.com/mattkjames7/KT17/releases/tag/v1.0.0 Software Anderson, B. J., Johnson, C. L., and Korth, H. (2013), A magnetic disturbance index for Mercury's magnetic field derived from MESSENGER Magnetometer data, Geochem. Geophys. Geosyst., 14, 3875– 3886 https://doi.org/10.1002/ggge.20242 Disturbance index description spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA HAPI Server https://amda.irap.omp.eu/service/hapi b_kt17 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. spase://CNES/SimulationRun/CDPP-AMDA/KT17/KT17Run MagneticField 1970-01-01T00:00:00Z 2030-01-01T00:00:00Z PT1M Mercury b msm @@orbit@@ b_kt17_model nT 3 bx Component.I 1 b_kt17_model(0) by Component.J 2 b_kt17_model(1) bz Component.K 3 b_kt17_model(2) Magnetic |b| b_kt17_model_tot Scalar magnitude of the magnetic field in nT phys.magField nT 1e-9>T TimeSeries Magnitude Magnetic