Query: title:(Solar wind-magnetosphere interaction as simulated by a 3D, EM particle code), Author: Buneman

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title:(Solar wind-magnetosphere interaction as simulated by a 3D, EM particle code) Author: Buneman

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title:(Solar AND wind-magnetosphere AND interaction AND as AND simulated AND by AND a AND 3D AND EM AND particle AND code)

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10 items by relevance

1 Conference paper

Solar wind-magnetosphere interaction as simulated by a 3D, EM particle code

Buneman, O.; Neubert, Torsten; Nishikawa, K.-I.

Proceedings of the Fourth International Conferance on Plasma Physics and Controlled Nuclear Fusion — 1993

Year: 1993

Language: English

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2 Preprint article

Solar wind-magnetosphere interaction as simulated by a 3D, EM particle code

Buneman, O.; Neubert, T.; Nishikawa, Ken-Ichi

The results of simulating the solar wind-magnetosphere interaction with a three dimensional, electromagnetic (EM) particle code are presented. Hitherto such global simulations were done with magnetohydrodynamic (MHD) codes while lower dimensional particle or hybrid codes served to account

Year: 1993

Language: Undetermined

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3 Journal article

Solar wind-magnetosphere interaction as simulated by a 3-D EM particle code 10.1109/27.199533

Buneman, O.; Neubert, T.; Nishikawa, K.-I.

Ieee Transactions on Plasma Science — 1992, Volume 20, Issue 6, pp. 810,811,812,813,814,815,816

Results are presented for simulating the solar-wind-magnetosphere interaction with a new three-dimensional electromagnetic particle code. Previously, such global simulations were done with MHD codes while lower-dimensional particle or hybrid codes served to account for microscopic processes and such transport parameters as have to be introduced ad hoc in MHD. The kinetic model presented attempts to combine the macroscopic and microscopic tasks. It relies only on the Maxwell curl equations and the Lorentz equation for particles, which are ideally suited for computers. The preliminary results...

Year: 1992

Language: English

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4 Book chapter

Solar Wind-Magnetosphere Interaction as Simulated by a 3-D EM Particle Code 10.1007/978-94-011-0405-0_23

Nishikawa, Ken-Ichi; Neubert, Torsten; Buneman, Oscar

Plasma Astrophysics and Cosmology — 1995, pp. 265-276

We have studied the solar wind-magnetosphere interaction using a 3-D electromagnetic particle code. The results for an unmagnetized solar wind plasma streaming past a dipole magnetic field show the formation of a magnetopause and a magnetotail, the penetration of energetic particles into cusps

Year: 1995

Language: English

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5 Preprint article

Solar wind-magnetosphere interaction as simulated by a 3-D EM particle code

Neubert, Torsten; Nishikawa, Ken-Ichi; Buneman, Oscar

We present here our first results of simulating the solar wind-magnetosphere interaction with a new three-dimensional electromagnetic particle code. Hitherto such global simulations were done with MHD codes while lower-dimensional particle or hybrid codes served to account for microscopic processes

Year: 1992

Language: Undetermined

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6 Journal article

Solar wind-magnetosphere interaction as simulated by a 3-D em particle code 10.1007/BF00678084