Decoding solar wind‐magnetosphere coupling

We employ a new NARMAX (Nonlinear Auto‐Regressive Moving Average with eXogenous inputs) code to disentangle the time‐varying relationship between the solar wind and SYM‐H. The NARMAX method has previously been used to formulate a Dst model, using a preselected solar wind coupling function. In this w...

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Veröffentlicht in:	Space Weather 2016-10, Vol.14 (10), p.724-741
Hauptverfasser:	Beharrell, M. J., Honary, F.
Format:	Artikel
Sprache:	eng
Schlagworte:	Algorithms Charged particles Cost function Coupling Decoding Delay Disturbance Electric fields Fluctuations geomagnetic storms Geomagnetic tail Geomagnetism Graphics processing units Interplanetary magnetic field Interplanetary magnetic fields Iterative methods Magnetic fields Magnetic flux Magnetopause Magnetopause currents Magnetosphere Magnetospheres Magnetotails Mathematical models Nonlinearity numerical modeling Particulate composites Programming Ring currents Solar physics Solar wind solar wind coupling Solar wind-magnetosphere coupling Space weather Wind power generation
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