Radio brightness distribution within cosmic background fluctuations

Details Radio brightness distribution within cosmic background fluctuations Radio brightness distribution within cosmic background fluctuations

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pazh...11..569s&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 11, Aug. 1985, p. 569-574) Soviet Astronomy Letters (ISSN 0360-0327), vol. 11, July-Aug

Astronomy and Astrophysics

Astronomy

Brightness Distribution, Fluctuation Theory, Radio Astronomy, Relic Radiation, Flux Density, Random Processes, Temperature Distribution

Scientific paper

The angular fluctuations delta T in the microwave background temperature constitute a random process. Calculations are performed for the number of 'pips' above a base level that might be produced by primordial scalar density perturbations or gravitational waves. The flux density expected for typical pips is determined, as well as the mean solid angle subtended by a pip that would exceed a level three times the dispersion in delta T.

Affiliated with

Also associated with

No associations

Rating

Radio brightness distribution within cosmic background fluctuations 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 Radio brightness distribution within cosmic background fluctuations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radio brightness distribution within cosmic background fluctuations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-760675