Problem of using lunar occultations of radio sources for investigating their angular structure. IV

Details Problem of using lunar occultations of radio sources for investigating their angular structure. IV Problem of using lunar occultations of radio sources for investigating their angular structure. IV

Oct 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977azh....54..967a&link_type=abstract

Astronomicheskii Zhurnal, vol. 54, Sept.-Oct. 1977, p. 967-972. In Russian.

Astronomy and Astrophysics

Astronomy

Lunar Occultation, Radio Sources (Astronomy), Stellar Luminosity, Angular Distribution, Angular Resolution, Brightness, Error Analysis, Signal To Noise Ratios, Wavelengths

Scientific paper

The dependence of angular resolution on wavelength band employed is determined for the problem of reconstructing the brightness distribution of radio sources from observations of lunar occultations performed at a high S/N ratio. Errors in the calculations are evaluated, and a case involving the observation of a lunar occultation of a compact radio source with a specified angular brightness distribution is considered as an example. Limitations of the outlined technique are discussed.

Affiliated with

Also associated with

No associations

Rating

Problem of using lunar occultations of radio sources for investigating their angular structure. IV 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 Problem of using lunar occultations of radio sources for investigating their angular structure. IV, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Problem of using lunar occultations of radio sources for investigating their angular structure. IV will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-745612