Refractive Interstellar Scintillation for Flux Density Variations of Two Pulsars

Details Refractive Interstellar Scintillation for Flux Density Variations of Two Pulsars Refractive Interstellar Scintillation for Flux Density Variations of Two Pulsars

Aug 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003chphl..20.1405z&link_type=abstract

Chinese Physics Letters, Volume 20, Issue 8, pp. 1405-1408 (2003).

Physics

4

Scientific paper

The flux density structure functions of PSRs B0525+21 and B2111+46 are calculated with the refractive interstellar scintillation (RISS) theory. The theoretical curves are in good agreement with observations [Astrophys. J. 539 (2000) 300] (hereafter S2000). The spectra of the electron density fluctuations both are of Kolmogorov spectra. We suggest that the flux density variations observed for these two pulsars are attributed to refractive interstellar scintillation, not to intrinsic variability.

Affiliated with

Also associated with

No associations

Rating

Refractive Interstellar Scintillation for Flux Density Variations of Two Pulsars 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 Refractive Interstellar Scintillation for Flux Density Variations of Two Pulsars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Refractive Interstellar Scintillation for Flux Density Variations of Two Pulsars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1667490