2.4.1 spase://CNES/NumericalData/CDPP-AMDA/Cluster/Cluster2/Models/c2-t96-model T96 field model Tsyganenko96 geomagnetospheric magnetic field model 2023-12-10T21:07:59Z A data-based Tsyganenko96 model computes the geomagnetospheric magnetic field with an explicitly defined realistic magnetopause, large-scale Region 1 and 2 Birkeland current systems, and the IMF penetration across the boundary. The model uses the following inputs : * solar wind ram pressure * IMF Y and Z-component * Dst index When a parameter 'T96 model field along a spacecraft orbit' is calculated, the input data above are fetched in the AMDA database and averaged on 20 min (fixed interval) before computation. The original ephemeris time resolution is finally used for the resolution of the computed magnetic field. Source for input conditions: OMNI 5 min dataset and SYM index dataset. TBD spase://CNES/Person/CDPP-AMDA/Nikolai.Tsyganenko PrincipalInvestigator Detailed description http://geo.phys.spbu.ru/~tsyganenko/modeling.html A detailed description along with complete references. clust2-orb-all spase://SMWG/Repository/CDPP/AMDA Online Open CDPP/AMDA HAPI Server https://amda.irap.omp.eu/service/hapi c2-t96-model 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. IRAP spase://CNES/Instrument/CDPP-AMDA/Cluster2/Models MagneticField 2000-08-22T00:00:00Z 2023-11-26T00:00:00Z PT1M Earth b_gse b_t96gse_c2_xyz_gse nT 3 bx Component.I 1 b_t96gse_c2_xyz_gse(0) by Component.J 2 b_t96gse_c2_xyz_gse(1) bz Component.K 3 b_t96gse_c2_xyz_gse(2) Vector Magnetic b_gsm b_t96gsm_c2_xyz_gse nT 3 bx Component.I 1 b_t96gsm_c2_xyz_gse(0) by Component.J 2 b_t96gsm_c2_xyz_gse(1) bz Component.K 3 b_t96gsm_c2_xyz_gse(2) Vector Magnetic |b| b_t96tot_c2_xyz_gse Average Magnetic Field magnitude phys.magField nT TimeSeries Magnitude Magnetic