HR: 14:15h
AN: SM43B-03 [Abstracts]
TI: Relation Between Magnetic Fields and Electric Currents in Cosmic Plasmas
AU: * Vasyli\=unas, V M
EM: vasyliunas@linmpi.mpg.de
AF: Max-Planck-Institut f\"ur Sonnensystemforschung, Max-Planck-Str. 2, Katlenburg-Lindau, 37191
Germany
AB:
Maxwell's equations allow the magnetic field ${\bf B}$
to be calculated if the electric current density
${\bf J}$ is assumed to be completely known as
a function of space and time. The charged particles
that constitute the current, however, are subject to
Newton's laws as well, and ${\bf J}$ can be changed
by forces acting on charged particles. Particularly
in plasmas, where the concentration of charged particles
is high, the effect of the electromagnetic field
calculated from a given ${\bf J}$ on ${\bf J}$ itself
cannot be ignored. Whereas in ordinary laboratory physics
one is accustomed to take ${\bf J}$ as primary and
${\bf B}$ as derived from ${\bf J}$, in plasmas ${\bf B}$ may be
viewed as primary and ${\bf J}$ as derived from ${\bf B}$ simply
as $(c/4\pi )\nabla \times {\bf B}$ -- a view proposed by
Cowling (1957) and
Dungey (1958) and in recent years strongly argued
by Parker. Here I investigate the relation between
$\nabla \times {\bf B}$ and ${\bf J}$ in the same terms
and by the same method as previously applied to the MHD
relation between electric field and plasma bulk flow
[Vasyli\=unas, {\it Geophys. Res. Lett.},
{\it 28}, 2177--2180, 2001]: assume that one but not the other
is present initially, and calculate what happens. The result
is that, for all
configurations with spatial scales much larger than the
electron inertial length, (1) a given $\nabla \times {\bf B}$
produces the corresponding ${\bf J}$, (2) a given
${\bf J}$ does not produce any $\nabla \times {\bf B}$ but
disappears instead. The result can be understood by noting that
$\nabla \times {\bf B} \neq (4\pi/c){\bf J}$
implies a time-varying electric field (displacement current)
which acts to change both terms (in order to bring them toward equality);
the changes of the two terms, however, proceed on different time scales,
light travel time for ${\bf B}$ and electron plasma period for ${\bf J}$,
and clearly the term changing much more slowly is the one that survives.
(The electron inertial length, by definition, is where
the two time scales are equal.)
Some illustrative simple examples will be discussed,
together with implications for determining
magnetic fields in space plasmas.
DE: 2409 Current systems (2708)
DE: 2708 Current systems (2409)
DE: 2740 Magnetospheric configuration and dynamics
DE: 2756 Planetary magnetospheres (5443, 5737, 6030)
SC: SPA-Magnetospheric Physics [SM]
MN: 2004 AGU Fall Meeting