Simulation of Space Plasma Allowing for the Hall Effect: Magnetic Reconnection

Author:

Filippychev D. S.

Publisher

Springer Science and Business Media LLC

Subject

Computational Mathematics

Reference121 articles.

1. D. S. Filippychev, “Hybrid simulation of space plasma: models with massless fluid representation of electrons. 1. Collisionless shocks,” in: Prikladnaya Matematika i Inforormatika [in Russian], No. 1, Dialog-MGU, Moscow (1999), pp. 20–50.

2. D. S. Filippychev, “Hybrid simulation of space plasma: models with massless fluid representation of electrons. 2. Slow and intermediate shocks,” in: Prikladnaya Matematika i Inforormatika [in Russian], No. 2, Dialog-MGU, Moscow (1999), pp. 5–33.

3. D. S. Filippychev, “Hybrid simulation of space plasma: models with massless fluid representation of electrons. 3. Shockless dis-continuities,” in: Prikladnaya Matematika i Inforormatika [in Russian], No. 4, Maks Press, Moscow (2000), pp. 5–56.

4. D. S. Filippychev, “Hybrid simulation of space plasma: models with massless fluid representation of electrons. 4. Kelvin-Helmholtz instability,” in: Prikladnaya Matematika I Inforormatika [in Russian], No. 7, Maks Press, Moscow (2001), pp. 19–55.

5. D. S. Filippychev, “Hybrid simulation of space plasma: models with massless fluid representation of electrons. 5. Reconnection of magnetic field lines,” in: Prikladnaya Matematika i Inforormatika [in Russian], No. 8, Maks Press, Moscow (2001), pp. 5–54.

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