By Abraham C.-L. Chian (auth.), A. C.-L. Chian, I. H. Cairns, S. B. Gabriel, J. P. Goedbloed, T. Hada, M. Leubner, L. Nocera, R. Stening, F. Toffoletto, C. Uberoi, J. A. Valdivia, U. Villante, C.-C. Wu, Y. Yan (eds.)
Advances in house atmosphere learn - quantity I comprises the lawsuits of 2 overseas workshops, the realm area setting discussion board (WSEF2002) and the excessive functionality Computing in house setting study (HPC2002), prepared via the realm Institute for house setting learn (WISER) from 22 July to two August 2002 in Adelaide, Australia.
The articles during this quantity assessment the cutting-edge of the theoretical, computational and observational stories of the actual procedures of Sun-Earth connections and area atmosphere. They disguise six topical components: Sun/Heliosphere, Magnetosphere/Bow surprise, Ionosphere/Atmosphere, house Weather/Space weather, area Plasma Physics/Astrophysics, and Complex/Intelligent platforms.
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Extra info for Advances in Space Environment Research: Volume I
Chou, D. : 2002b, and the TON Team, in this proceedings. A CLASS OF TVD TYPE COMBINED NUMERICAL SCHEME FOR MHD EQUATIONS WITH A SURVEY ABOUT NUMERICAL METHODS IN SOLAR WIND SIMULATIONS XUESHANG FENG1 , S. T. A. Abstract. It has been believed that three-dimensional, numerical, magnetohydrodynamic (MHD) modelling must play a crucial role in a seamless forecasting system. This system refers to space weather originating on the sun; propagation of disturbances through the solar wind and interplanetary magnetic ﬁeld (IMF), and thence, transmission into the magnetosphere, ionosphere, and thermosphere.
A. and Weiss, N. : 1980, Nature 287, 616. Sun, M. , Chou, D. : 2002a, and the TON Team, Solar Phys. 209, 5. Sun, M. , Chou, D. : 2002b, and the TON Team, in this proceedings. A CLASS OF TVD TYPE COMBINED NUMERICAL SCHEME FOR MHD EQUATIONS WITH A SURVEY ABOUT NUMERICAL METHODS IN SOLAR WIND SIMULATIONS XUESHANG FENG1 , S. T. A. Abstract. It has been believed that three-dimensional, numerical, magnetohydrodynamic (MHD) modelling must play a crucial role in a seamless forecasting system. This system refers to space weather originating on the sun; propagation of disturbances through the solar wind and interplanetary magnetic ﬁeld (IMF), and thence, transmission into the magnetosphere, ionosphere, and thermosphere.
In what follows we ﬁrst brieﬂy mention some current used numerical methods in solar wind simulation. Then, based on our analysis, a new combined numerical scheme of TVD type for magnetohydrodynamic equations is introduced. Finally, some conclusions about the properties a high quality numerical scheme of solar wind simulation should have is given. A NEW COMBINED NUMERICAL SCHEME FOR MHD 45 2. Numerical Methods in Solar Wind Modelling In the past three decades, solar-terrestrial physicists have introduced many kinds of numerical schemes used in computational ﬂuid mechanics to the magnetohydrodynamic system in order to simulate various phenomena of solar-terrestrial physics.
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