1997A&A...326.1277O -
Astronomy and Astrophysics, volume 326, 1277-1284 (1997/10-3)
On collimation of the outflows in force-free magnetospheres.
OKAMOTO I.
Abstract (from CDS):
It is pointed out that ``an indeterminacy" claimed to exist in the pulsar equation (Sulkanen & Lovelace,
1990ApJ...350..732S) or a ``free" function B
t{piomega}=β (Appl & Camenzind
1993A&A...270...71A,
1993A&A...274..699A) can be uniquely related to the stream function at the boundary of the force-free region to the load region at infinity (Michel,
1973ApJ...180L.133M: Okamoto,
1974MNRAS.167..457O). The form of β is given by β=-(α/c)(B
p{piomega}
2)
∞ from the plasma conditions at infinity, where α is the angular velocity of field lines. This relation can be interpreted as indicating Ohm's law for the return current from the equatorial region to the polar region on the `sphere at infinity' with finite resistivity R
L=4π/c=377Ohm, thereby ensuring the current closure. The field structure tends to be asymptotically conical, toward the `sphere at infinity' and fields fill all the space there. It is argued that force-free models for purely cylindrical jets cannot self-consistently conserve electric current. The role of the plasma conditions in the black hole equation is mentioned as well.
Abstract Copyright:
∼
Journal keyword(s):
MHD - ISM: jets and outflows - galaxies: jets - Black hole physics - pulsars: general
Simbad objects:
0
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