Matter penetration and motion through the magnetosphere of neutron star

Details Matter penetration and motion through the magnetosphere of neutron star Matter penetration and motion through the magnetosphere of neutron star

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990esasp.311..221j&link_type=abstract

In ESA, Plasma Astrophysics p 221-225 (SEE N91-15046 06-90)

Astronomy and Astrophysics

Astrophysics

Distribution Functions, Interstellar Matter, Neutron Stars, Penetration, Pulsar Magnetospheres, Stellar Magnetic Fields, Stellar Mass Accretion, Adiabatic Conditions, Equations Of Motion, Magnetohydrodynamic Stability, Momentum, Perturbation, Pulsars, Statistical Distributions

Scientific paper

The adiabatic invariant is shown to be conserved through the whole polar column of the neutron star. In the strong magnetic field of pulsars the smoothing process of particles longitudinal and transversal momentum components is therefore highly slowed down. The interface plasma magnetic field is shown to be almost always stable due to the presence of a strong gradient of magnetic field.

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