Radio‐Wave Propagation in the Non‐Gaussian Interstellar Medium
نویسندگان
چکیده
منابع مشابه
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 that 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 observed pulse time-shapes to the electron-density correlation function has developed for 3...
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ژورنال
عنوان ژورنال: The Astrophysical Journal
سال: 2005
ISSN: 0004-637X,1538-4357
DOI: 10.1086/428919