VLBI observations of the scattering disk of pulsar 1933 + 16

Details VLBI observations of the scattering disk of pulsar 1933 + 16 VLBI observations of the scattering disk of pulsar 1933 + 16

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988aipc..174..106g&link_type=abstract

IN: Radio wave scattering in the interstellar medium; Proceedings of the AIP Conference, San Diego, CA, Jan. 18, 19, 1988 (A89-2

Physics

7

Interstellar Matter, Plasma Density, Pulsars, Radio Scattering, Very Long Base Interferometry, Data Correlation, Kolmogoroff Theory, Spectrum Analysis

Scientific paper

A Kolmogorov spectrum of density fluctuations in the interstellar plasma is favored by VLBI observations of the scattering disk of pulsar 1933 + 16. The decline of visibility with baseline length and the scaling of size with frequency agree with those predicted on the basis of such a spectrum. The spectral index of density fluctuations is calculated as 3.52 + or - 0.13. An upper limit of 1:1.7 on the elongation of the scattered image is obtained.

Affiliated with

Also associated with

No associations

Rating

VLBI observations of the scattering disk of pulsar 1933 + 16 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 VLBI observations of the scattering disk of pulsar 1933 + 16, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and VLBI observations of the scattering disk of pulsar 1933 + 16 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1825255