2.2.6 spase://CDPP/NumericalOutput/AMDA/TSYG96/b_t96 B along s/c orbit 2017-08-23T00:00:00Z 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. Model magnetic field can be calculated along a number of spacecraft orbits : select the desired one from the arguments list. Source for input conditions: OMNI 5 min dataset and SYM index dataset. TBD spase://CDPP/Person/Nikolai.Tsyganenko PrincipalInvestigator spase://CDPP/Person/Elena.Budnik TechnicalContact Detailed description http://geo.phys.spbu.ru/~tsyganenko/modeling.html A detailed description along with complete references. spase://SMWG/Repository/CDPP/AMDA Online Open AMDA at CDPP http://amda.cdpp.eu Text.ASCII TBD spase://CDPP/SimulationRun/AMDA/TSYG96/Tsyg96Run MagneticField 1970-01-01T00:00:00Z 1970-01-01T00:00:00Z PTS/C Earth b gse @@ORBIT@@ b_t96gse nT 3 bx Component.I 1 b_t96gse(0) by Component.J 2 b_t96gse(1) bz Component.K 3 b_t96gse(2) NaN Magnetic b gsm @@ORBIT@@ b_t96gsm nT 3 bx Component.I 1 b_t96gsm(0) by Component.J 2 b_t96gsm(1) bz Component.K 3 b_t96gsm(2) NaN Magnetic |b| @@ORBIT@@ b_t96tot TBD nT NaN Magnetic