On the theory of large-scale micropulse structure of pulsar radio radiation

Details On the theory of large-scale micropulse structure of pulsar radio radiation On the theory of large-scale micropulse structure of pulsar radio radiation

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990esasp.311..251o&link_type=abstract

In ESA, Plasma Astrophysics p 251-253 (SEE N91-15046 06-90)

Astronomy and Astrophysics

Astrophysics

2

Astronomical Models, Cnoidal Waves, Mathematical Models, Micropulsations, Pulsars, Pulsed Radiation, Stellar Radiation, Elliptic Functions, Jacobi Integral, Low Frequencies, Magnetic Fields, Magnetohydrodynamic Stability, Two Dimensional Models, Wave Propagation

Scientific paper

Large scale microstructure of pulsar radiation is shown to be
explainable as a result of self interaction of low frequency nonlinear
cnoidal waves propagated in inner polar regions along a magnetic field
of a neutron star. Stability of these cnoidal waves with respect to two
dimensional long wavelength perturbations is discussed.

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