Radio-Wave Propagation in the Non-Gaussian Interstellar Medium

Radio waves propagating from distant pulsars in the interstellar medium (ISM) are refracted by electron density inhomogeneities, so the intensity of observed pulses fluctuates with time. The observed pulse shapes are used to diagnose electron density distribution in the ISM. The theory relating the...

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Veröffentlicht in:	The Astrophysical journal 2005-05, Vol.624 (1), p.213-222
Hauptverfasser:	Boldyrev, Stanislav, Gwinn, Carl R
Format:	Artikel
Sprache:	eng
Online-Zugang:	Volltext bestellen
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