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The interplanetary shock propagation model : a model for predicting solar-flare-caused geomagnetic storms, based on the 2 1/2 D, MHD numerical simulation results from the interplanetary global model (2D IGM)

CITE Title : The interplanetary shock propagation model : a model for predicting solar-flare-caused geomagnetic storms, based on the 2 1/2 D, MHD numerical simulation results from the interplanetary global model (2D IGM) Personal Author(s) : Smith, Zdenka K.;Dryer, Murray; Corporate Authors(s) : Space Environment Laboratory Published Date : 1995 Series : NOAA technical memorandum ERL SEL ; 89 URL : /view/noaa/19035 Smith, Zdenka K. and Dryer, Murray (1995). The interplanetary shock propagation model : a model for predicting solar-flare-caused geomagnetic storms, based on the 2 1/2 D, MHD numerical simulation results from the interplanetary global model (2D IGM). Smith, Zdenka K. and Dryer, Murray "The interplanetary shock propagation model : a model for predicting solar-flare-caused geomagnetic storms, based on the 2 1/2 D, MHD numerical simulation results from the interplanetary global model (2D IGM)" (1995) Smith, Zdenka K. and Dryer, Murray "The interplanetary shock propagation model : a model for predicting solar-flare-caused geomagnetic storms, based on the 2 1/2 D, MHD numerical simulation results from the interplanetary global model (2D IGM)" , 1995 Export RIS Citation Information.

:

Smith, Zdenka K. ;

Dryer, Murray

1995 | NOAA technical memorandum ERL SEL ; 89

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