Computer Science – Numerical Analysis
Scientific paper
Aug 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.192..409s&link_type=abstract
Monthly Notices of the Royal Astronomical Society, vol. 192, Aug. 1980, p. 409-416.
Computer Science
Numerical Analysis
4
Elliptic Differential Equations, Numerical Analysis, Parabolic Differential Equations, Pulsar Magnetospheres, Pulsars, Stellar Atmospheres, Boundary Conditions, Boundary Value Problems, Classifications, Neutron Stars, Stellar Magnetic Fields, Stellar Rotation, Variational Principles
Scientific paper
The general structure of the system of pulsar equations derived in an earlier paper is investigated for the magnetosphere of a parallel rotator including particle inertia. The complete system reduces to one parabolic and two elliptic differential equations. The characteristics are found to be the streamlines. Appropriate variational principles are specified and a method for solving the pulsar equations numerically is proposed. Complete boundary conditions are given. First results for the solution within the corotating zone are presented.
Herold Heinz
Rossmanith C.
Ruder Hanns
Schmalz R.
No associations
LandOfFree
On the self-consistent description of axisymmetric pulsar magnetospheres. II - A method of solution 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 On the self-consistent description of axisymmetric pulsar magnetospheres. II - A method of solution, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the self-consistent description of axisymmetric pulsar magnetospheres. II - A method of solution will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1275633