Adiabatic Invariant Trapped Radiation Shells and Cosmic Ray Cutoffs in Models of the Magnetosphere Distorted by the Solar Wind Plasma |
Contents
II REVIEW OF PREVIOUS WORK | 7 |
III THE SECOND APPROXIMATION TO THE LAGRANGES | 37 |
IV TRAPPED RADIATION | 58 |
1 other sections not shown
Common terms and phrases
adiabatic invariants Alfen motion APPENDIX approximate axial symmetry B-independent charged particle coefficients components computed constant along lines coordinates CORNELL CORNELL CORNELL UNIVERSITY cose Cosmic Ray Cutoffs defined derivative dipole dipole field drift velocity earth radii earth's field energy equatorial evaluated field model Figure Finch and Leaton function geomagnetic field given guiding center Integral Invariant invariant shells invariant surfaces Lagrange's Equation Lagrangian Larmour radius line of force magnetic equator magnetic moment magnetic scalar potential magnetosphere McIlwain mirror point parameter partial differential equation particle's predicts relativistic relativistic mass result right hand side second term solar wind spherical harmonic static magnetic field Størmer Størmer Theory subroutine sufficiently low Surface of constant trajectory trapped particle trapped radiation UNIVERSITY CORNELL UNIVERSITY LIBRARY CORNELL V₂ vector vector potential vertical cutoff rigidity WALLS OF HONES θα να ав ба