Frequency Selective Surfaces for Radio Astronomy

Details Frequency Selective Surfaces for Radio Astronomy Frequency Selective Surfaces for Radio Astronomy

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991exa.....2..123i&link_type=abstract

Experimental Astronomy, Volume 2, Issue 2, pp.123-136

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Frequency selective surfaces (FSSs) with the Jerusalem-cross array configuration have been developed for simultaneous observations of radio astronomical sources at the 40GHz and 80GHz bands. For supporting material, PET(polyethylene terephthalate: 200×220mm large, 12μm thick, permittivity 3.0) was used, and copper was used for the conducting array. The measured characteristics were in good agreement with the calculated ones. The fabricated FSS has low insertion losses of less than 0.2dB and little distortion of polarization for each band. The characteristics of the developed FSS satisfy radio astronomical requirements.

Affiliated with

Also associated with

No associations

Rating

Frequency Selective Surfaces for Radio Astronomy 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 Frequency Selective Surfaces for Radio Astronomy, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Frequency Selective Surfaces for Radio Astronomy will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1604972