Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.192..799h&link_type=abstract
Monthly Notices of the Royal Astronomical Society, vol. 192, Sept. 1980, p. 799-804.
Astronomy and Astrophysics
Astronomy
37
Electron Density Profiles, Frequency Response, Interstellar Matter, Pulsars, Scintillation, Diffraction Patterns, Kolmogoroff Theory, Plasma Density, Solar Wind, Time Dependence, Velocity Distribution
Scientific paper
Slow frequency drifts revealed by multichannel spectrometer observations of pulsars provide a sensitive method of detecting irregularities of electron density which are too large to cause interstellar scintillation. Observations of four pulsars are used to compare the density variations in the large- and small-scale irregularities. The values obtained are compatible with a Kolmogorov spectrum for scales in the range 10 to the 10th - 10 to the 13th cm, but suggest that the power-law index may exceed 11/3. The large irregularities offer a simple explanation of apparent reversals in two-station measurements of drift velocity.
No associations
LandOfFree
Frequency-time structure of pulsar scintillation 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 Frequency-time structure of pulsar scintillation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Frequency-time structure of pulsar scintillation will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-908285