Interferometer for solar observations at a frequency of 127 MHz

Details Interferometer for solar observations at a frequency of 127 MHz Interferometer for solar observations at a frequency of 127 MHz

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975poast..23..141b&link_type=abstract

Postepy Astronomii, vol. 23, Apr.-June 1975, p. 141-151. In Polish.

Computer Science

Performance

1

Dipole Antennas, Radio Astronomy, Radio Interferometers, Solar Instruments, Circuit Diagrams, Performance Tests, Radio Astronomy, Signal Reception, Time Response

Scientific paper

The interferometer described is intended for routine solar observations. The antenna system consists of two identical antennas arranged along the East-West line. Each antenna is composed of two half-wave dipoles and a plane-quadratic reflector. The antenna gain is 7.7 dB. The radioastronomic receiver which records and measures the signals from the antenna is discussed, and some test results are presented.

Affiliated with

Also associated with

No associations

Rating

Interferometer for solar observations at a frequency of 127 MHz 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 Interferometer for solar observations at a frequency of 127 MHz, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Interferometer for solar observations at a frequency of 127 MHz will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-751299