2.2.6
spase://CNES/NumericalOutput/CDPP-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://CNES/Person/Nikolai.Tsyganenko
PrincipalInvestigator
spase://CNES/Person/Elena.Budnik
TechnicalContact
Detailed description
http://geo.phys.spbu.ru/~tsyganenko/modeling.html
A detailed description along with complete references.
spase://SMWG/Repository/CNES/CDPP-AMDA
Online
Open
AMDA at CDPP
http://amda.cdpp.eu
Text.ASCII
TBD
spase://CNES/SimulationRun/CDPP-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