Summary: Astron. Astrophys. 363, 1134­1144 (2000)
ASTRONOMY
AND
ASTROPHYSICS
MHD consistent cellular automata (CA) models
I. Basic features
H. Isliker1
, A. Anastasiadis2
, and L. Vlahos1
1
University of Thessaloniki, Section of Astrophysics, Astronomy and Mechanics, Department of Physics, 54006 Thessaloniki, Greece
(isliker@helios.astro.auth.gr; vlahos@helios.astro.auth.gr)
2
Institute for Space Applications and Remote Sensing, National Observatory of Athens, 15236 Penteli, Greece (anastasi@space.noa.gr)
Received 21 July 2000 / Accepted 18 October 2000
Abstract. A set-up is introduced which can be superimposed
onto the existing solar flare cellular automata (CA) models, and
which specifies the interpretation of the model's variables. It
extends the CA models, yielding the magnetic field, the current,
and an approximation to the electric field, in a way that is con-

Source: Anastasiadis, Anastasios - Institute for Space Applications and Remote Sensing, National Observatory of Athens
Isliker, Heinz - Department of Physics, Aristotle University of Thessaloniki

Collections: Physics