Evaluation of a Revised Interplanetary Shock Prediction Model: 1D CESE-HD-2 Solar-Wind Model

Author:

Zhang Y.,Du A. M.,Du D.,Sun W.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference31 articles.

1. Geophys. Monogr. Ser.;S.I. Akasofu,2001

2. Detman, T., Smith, Z., Dryer, M., Fry, C.D., Arge, C.N., Pizzo, V.: 2006, A hybrid heliospheric modeling system: background solar wind. J. Geophys. Res. 111, A07102. 10.1029/2005JA011430 .

3. Dryer, M., Smart, D.F.: 1984, Dynamical models of coronal transients and interplanetary disturbances. Adv. Space Res. 4, 291. 10.1016/0273-1177(84)90573-8 .

4. Feng, X.S., Zhang, Y., Yang, L.P., Wu, S.T., Dryer, M.: 2009, An operational method for shock arrival time prediction by 1D CESE-HD solar wind model. J. Geophys. Res. 114, A10103. 10.1029/2009JA014385 .

5. Fry, C.D.: 1985, Three-dimensional structure of the heliosphere: quiet-time and disturbed periods, Ph.D. Thesis, Univ. Alaska.

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