Dual-frequency correlation of pulsar micropulses

Details Dual-frequency correlation of pulsar micropulses Dual-frequency correlation of pulsar micropulses

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986azh....63...84s&link_type=abstract

(Astronomicheskii Zhurnal, vol. 63, Jan.-Feb. 1986, p. 84-93) Soviet Astronomy (ISSN 0038-5301), vol. 30, Jan.-Feb. 1986, p. 51-

Astronomy and Astrophysics

Astronomy

7

Cross Correlation, Pulsars, Radiant Flux Density, Radio Frequencies, Spectrum Analysis, Micropulsations, Stellar Models, Temporal Resolution

Scientific paper

The pulsars PSR 0809+74 and PSR 1133+16 were observed at the frequencies 102.5 and 101 MHz simultaneously with 10 μs time resolution. It is shown from a cross-correlation analysis that the microstructure with timescales exceeding 300 μs is highly correlated at both frequencies, but such a correlation is absent for microstructure with small timescale (<300 μs). This difference between short timescale and long timescale microstructure can be explained in the polar cap model, due to the complicated structure of the pulsar's emitting region. For PSR 0809+74 a new value of the dispersion measure is obtained from time delay between micropulses at the two frequencies, DM = 5.751±0.003 cm-3pc.

Affiliated with

Also associated with

No associations

Rating

Dual-frequency correlation of pulsar micropulses 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 Dual-frequency correlation of pulsar micropulses, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dual-frequency correlation of pulsar micropulses will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1675362