Bounce-averaged Hamiltonian for charged particles in an axisymmetric but nondipolar model magnetosphere

Computer Science – Numerical Analysis

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

7

Charged Particles, Earth Magnetosphere, Hamiltonian Functions, Magnetic Fields, Mathematical Models, Adiabatic Conditions, Functional Analysis, Harmonic Oscillation, Numerical Analysis, Polynomials, Symmetry

Scientific paper

In order to facilitate bounce-averaged guiding center simulations of geomagnetically trapped particles, we express the kinetic energy of a particle with magnetic coordinates (L,phi) as an analytic function of the first two adiabatic invariants (M,J) and the L value of the field line. The magnetic field model is axisymmetric, consisting of a dipolar vector-B field plus a uniform southward magnetic field parallel to the dipole moment mu(sub E). This model magnetosphere is surrounded by a circular equatorial neutral line whose radius b is an adjustable parameter. Our formulation provides a computationally efficient method for tracing the bounce-averaged adiabatic motion (conserving all three invariants) and nonadiabatic transport (violating the third invariant while conserving the first two invariants) of geomagnetically trapped particles in the model magnetosphere.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Bounce-averaged Hamiltonian for charged particles in an axisymmetric but nondipolar model magnetosphere does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Bounce-averaged Hamiltonian for charged particles in an axisymmetric but nondipolar model magnetosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Bounce-averaged Hamiltonian for charged particles in an axisymmetric but nondipolar model magnetosphere will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1829955

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.