Force-free magnetic field explained
In plasma physics, a force-free magnetic field is a magnetic field in which the Lorentz force is equal to zero and the magnetic pressure greatly exceeds the plasma pressure such that non-magnetic forces can be neglected. For a force-free field, the electric current density is either zero or parallel to the magnetic field.
Definition
When a magnetic field is approximated as force-free, all non-magnetic forces are neglected and the Lorentz force vanishes. For non-magnetic forces to be neglected, it is assumed that the ratio of the plasma pressure to the magnetic pressure—the plasma β—is much less than one, i.e.,
. With this assumption, magnetic pressure dominates over plasma pressure such that the latter can be ignored. It is also assumed that the magnetic pressure dominates over other non-magnetic forces, such as
gravity, so that these forces can similarly be ignored.
In SI units, the Lorentz force condition for a static magnetic field
can be expressed as
where
is the
current density and
is the
vacuum permeability. Alternatively, this can be written as
These conditions are fulfilled when the current vanishes or is parallel to the magnetic field.
[1] Zero current density
:
The substitution of this into
results in
Laplace's equation,
which can often be readily solved, depending on the precise boundary conditions. In this case, the field is referred to as a
potential field or
vacuum magnetic field.
Nonzero current density
If the current density is not zero, then it must be parallel to the magnetic field, i.e.,
where
is a scalar function known as the
force-free parameter or
force-free function. This implies that
The force-free parameter can be a function of position but must be constant along field lines.
Linear force-free field
When the force-free parameter
is constant everywhere, the field is called a
linear force-free field (LFFF). A constant
allows for the derivation of a vector
Helmholtz equation
by taking the curl of the nonzero current density equations above.
Nonlinear force-free field
When the force-free parameter
depends on position, the field is called a
nonlinear force-free field (NLFFF). In this case, the equations do not possess a general solution, and usually must be solved numerically.
[2] [3] Physical examples
In the Sun's upper chromosphere and lower corona, the plasma β can locally be of order 0.01 or lower allowing for the magnetic field to be approximated as force-free.[4] [5] [6]
See also
Further reading
- Book: Marsh . Gerald E. . Force-free magnetic fields: solutions, topology and applications . 1996 . World Scientific . 981-02-2497-4 . 10.1142/2965.
Notes and References
- Wiegelmann . Thomas . Sakurai . Takashi . Solar force-free magnetic fields . Living Reviews in Solar Physics . December 2021 . 18 . 1 . 1 . 10.1007/s41116-020-00027-4 . 232107294 . 18 May 2022.
- Book: Bellan . Paul Murray . Fundamentals of plasma physics . 2006 . Cambridge University Press . Cambridge . 0521528003.
- Book: Parker . E. N. . Cosmical Magnetic Fields: Their Origin and Their Activity . 2019 . Clarendon Press . Oxford . 978-0-19-882996-6.
- Amari . T. . Aly . J. J. . Luciani . J. F. . Boulmezaoud . T. Z. . Mikic . Z. . Reconstructing the Solar Coronal Magnetic Field as a Force-Free Magnetic Field . Solar Physics . 1997 . 174 . 129–149 . 10.1023/A:1004966830232 . 1997SoPh..174..129A.
- Low . B. C. . Lou . Y. Q. . Modeling Solar Force-Free Magnetic Fields . The Astrophysical Journal . March 1990 . 352 . 343 . 10.1086/168541 . 1990ApJ...352..343L.
- Peter . H. . Warnecke . J. . Chitta . L. P. . Cameron . R. H. . Limitations of Force-Free Magnetic Field Extrapolations: Revisiting Basic Assumptions . Astronomy & Astrophysics . November 2015 . 584 . 10.1051/0004-6361/201527057 . 2015A&A...584A..68P . 1510.04642.