Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998apj...506..341w&link_type=abstract
The Astrophysical Journal, Volume 506, Issue 1, pp. 341-346.
Astronomy and Astrophysics
Astronomy
38
Instabilities, Plasmas, Stars: Pulsars: General, Radiation Mechanisms: Nonthermal
Scientific paper
The plasma wave turbulence emission mechanism is studied to make predictions for the temporal characteristics of pulsar radio emission. The turbulent emission process consists of a cycle of electrostatic wave growth and modulational conversion into radiative modes. The onset of plasma wave turbulence is marked by explosive spatial collapse of regions of high electric field and bursts of radiation. Intrinsic time structure is found on subnanosecond to 10 ns timescales. The pulse exhibits an unusual spectral signature because of the coupling of the electromagnetic modes to the underlying electrostatic pump wave. This prediction can be tested with ultrashort timescale observations.
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