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Global Modeling of Disturbances in the Corona-Interplanetary Space

Published online by Cambridge University Press:  14 August 2015

Tyan Yeh
Tyan Yeh*
Affiliation:
Department of Mathematics, Metropolitan State College Denver, Colorado 80204, U.S.A.

Extract

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In the past few years, numerical studies of corona-interplanetary dynamics have been undertaken by many investigators. The results, as summarized by Wu et al. (1977), indicate that this approach seems very promising and worthy of further pursuit. So far, the calculations have been performed on two-dimensional codes, to simulate magneto-hydrodynamic flow in a meridional plane or in the equatorial plane. In order to fully account for the global features of the corona-interplanetary phenomenon, it is necessary to do three-dimensional calculations. Here we discuss some groundwork for the formulation of a time-dependent three-dimensional code.

Type
Part VI. Coronal and Interplanetary Responses to Short Time Scale Phenomena: - Theoretical Considerations
Information
Symposium - International Astronomical Union , Volume 91: Solar and Interplanetary Dynamics , 1980 , pp. 503 - 506
Copyright
Copyright © Reidel 1980 

References

McIntosh, P. S.: 1979, Annotated Atlas of Hα Synoptic Charts for Solar Cycle 20 (1964-1974), World Data Center A for Solar-Terrestrial Physics, NOAA, Boulder, Colorado.Google Scholar
Wu, S. T., Nakagawa, Y., and Dryer, M.: 1977, Study of Travelling Interplanetary Phenomena (ed. Shea, M. A., Smart, D. F. and Wu, S. T.), pp. 43–62, D. Reidel Publishing Co., Dordrecht-Holland.Google Scholar
Yeh, T.: 1978, Solar Phys. 56, pp. 439–447.Google Scholar
Yeh, T. and Pneuman, G. W.: 1977, Solar Phys. 54, pp. 419–430.Google Scholar