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Large-Scale Computer Simulation of Solar Active Phenomena: Summary of a Session at the IAU General Assembly on August 2 - 11, 1988, Baltimore, Maryland, U. S. A.

Published online by Cambridge University Press:  25 April 2016

Abstract

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Type
Chapter V: Reports of Meetings of Commissions
Information
Transactions of the International Astronomical Union , Volume 20 , Issue 2 , 1988 , pp. 157 - 161
Copyright
Copyright © Kluwer 1988

References

Aly, J. J., (1988) ”On the construction of the nonlinear-force-free coronal magnetic field from boundary data”, Solar Phys. (submitted).Google Scholar
Chiuderi, C., and Van Hoven, G., (1979) ”The dynamics of filament formation: the thermal instability in a sheared magnetic field”, Astrophys. J. (Letts.), 232, L69.CrossRefGoogle Scholar
Drake, J. F., Sparks, L., and Van Hoven, G., (1988) ”Radiative instabilities in a sheared magnetic field”, Phys. Fluids, 31, 813.Google Scholar
Dahlburg, R. B., Dahlburg, J. P. and Mariska, J. T., (1988) ”Helical Magnetohydrodynamic Turbulence and the Coronal Heating Problem” Astron. Astrophys., 198, 300.Google Scholar
Einaudi, G., and Demoulin, P., (1988), in preparation. Field, G. B., (1965), ”Thermal Instability”, Astrophys. J., 142, 531.Google Scholar
Forbes, T. G., (1988) ”Shocks Produced by Impulsively Driven Reconnection” Solar Physics (in press).CrossRefGoogle Scholar
Mikic, Z., Barnes, D. C., and Schnack, D. D., (1988a) ”Dynamical evolution of a solar coronal magnetic field arcade”, Astrophys. J., (to appear).Google Scholar
Mikic, Z., Schnack, D.D., and Van Hoven, G., (1988b) ”Creation of current filaments in the solar corona” Astrophys. J., (to appear).Google Scholar
Parker, E. N., (1983) ”Magnetic neutral sheets in evolving fields. I. General theory”, Astrophys. J., 264, 635.CrossRefGoogle Scholar
Sakurai, T., (1981), ”Calculation of force-free magnetic field with non-constant α), Solar Phys., 69, 343.Google Scholar
Van Hoven, G., Sparks, L. and Schnack, D. D., (1987) ”Nonlinear radiative condensation in a sheared magnetic field”, Astrophys. J. (Letts), 317, L91.Google Scholar
Van Hoven, G., Sparks, L. and Tachi, T., (1986) ”Ideal condensations due to perpendicular thermal conduction in a sheared magnetic field”, Astrophys., J., 300, 249.Google Scholar
Wu, S. T., Hu, Y. Q., Nakagawa, Y. and Tandberg-Hanssen, E., (1983) ”Induced Mass and Wave Motions in the Lower Solar Atmosphere. I. Effects of Shear Motion of Flux Tubes”, Astrophys. J., 266, 866.Google Scholar
Wu, S. T., Chang, H. M. and Hagyard, M. J., (1984), ”On the Numerical Computation of Nonlinear Force-Free Magnetic Fields” in Measurements of Solar Vector Magnetic Fields (Hagyard, M. J., ed.) NASA Conference Publ. 2374, pp. 17–26.Google Scholar