A Pattern in the Large-scale Distribution of Galactic Polarized Radio Emission

Details A Pattern in the Large-scale Distribution of Galactic Polarized Radio Emission A Pattern in the Large-scale Distribution of Galactic Polarized Radio Emission

Sep 1964

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1964natur.203.1273m&link_type=abstract

Nature, Volume 203, Issue 4951, pp. 1273-1274 (1964).

Computer Science

8

Scientific paper

THE initial discovery by the Dutch1 and Cambridge2 groups of a linearly polarized component of galactic radio emission was followed by a large-scale survey3,4 of the polarization at 408 Mc/s using the Dwingeloo radio telescope (aerial beam-width 2°). In 1963, a polarization survey was made, using the 210-ft. steerable reflector at Parkes at 408 Mc/s (aerial beam-width 0.8°), of that part of the sky not covered by the Dutch survey; the detailed results of this will be published elsewhere. This communication concerns an outstanding feature of the large-scale distribution of the polarized radio emission which is seen when the results of both surveys are combined. It appears that more than 90 per cent of the polarized radio emission at this frequency comes from regions which lie inside a band about 50° wide that contains the great circle which passes through the galactic poles and cuts the plane at lII = 340° and 160°.

Affiliated with

Also associated with

No associations

Rating

A Pattern in the Large-scale Distribution of Galactic Polarized Radio Emission 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 A Pattern in the Large-scale Distribution of Galactic Polarized Radio Emission, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Pattern in the Large-scale Distribution of Galactic Polarized Radio Emission will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1031779