We study the effect of nova magnetodipole fields on the dynamics and struct
ure of ejected shells by using a numerical model based on the kinetic-hydro
dynamic description of plasma dynamics. Our calculations show that characte
ristic nonuniformities appear in the distribution of field and plasma pertu
rbations during super-Alfven shell expansion in the circumstellar medium. (
C) 2000 MAIK "Nauka/Interperiodica".