Author:
- V. Pavlidou, Department of Astronomy, University of Illinois at Urbana-Champaign, Urbana, USA, and Section of Astrophysics, Astronomy and Mechanics, Department of Physics, University of Tessaloniki, Greece.
- J. Kuijpers, Astronomical Institute, Utrecht University, The Netherlands, and Department of Astrophysics, University of Nijmegen, The Netherlands.
- L. Vlahos, Section of Astrophysics, Astronomy and Mechanics, Department of Physics, University of Tessaloniki, Greece.
- H. Isliker, Section of Astrophysics, Astronomy and Mechanics, Department of Physics, University of Tessaloniki, Greece.
- Accepted 15 February 2001
Content:
In this paper we attempt, for the first time, to simulate the magnetic activity of an accretion disc using a probabilistic cellular automaton model. Our model is based on three free parameters, the probabilities of spontaneous and stimulated generation of magnetic flux below the surface of the disc, and the probability of diffusive disappearance of flux below the surface (D).
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