Astronomy and Astrophysics – Astrophysics
Scientific paper
2003-09-23
Phys.Rev.Lett. 91 (2003) 131101
Astronomy and Astrophysics
Astrophysics
4 pages, 3 figures
Scientific paper
10.1103/PhysRevLett.91.131101
Observations of radio signals from distant pulsars provide a valuable tool for investigation of interstellar turbulence. The time-shapes of the signals are the result of pulse broadening by the fluctuating electron density in the interstellar medium. While the scaling of the shapes with the signal frequency is well understood, the observed anomalous scaling with respect to the pulsar distance has remained a puzzle for more than 30 years. We propose a new model for interstellar electron density fluctuations, which explains the observed scaling relations. We suggest that these fluctuations obey Levy statistics rather than Gaussian statistics, as assumed in previous treatments of interstellar scintillations.
Boldyrev Stanislav
Gwinn Carl R.
No associations
LandOfFree
Levy model for interstellar scintillations does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Levy model for interstellar scintillations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Levy model for interstellar scintillations will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-182548