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This critical design review details the K-Band Focal Plane Array (KFPA) developed for the Green Bank Telescope (GBT), focusing on its performance across 18-26.5 GHz. Key metrics such as feed frequency, horn taper, and element configurations are explored, with results presented on aperture efficiency, beam patterns, and cross-polarization measurements. The findings also include optimal element orientation and spacing, alongside insertion and return loss data for the orthomode junction. This review serves as a foundational document for further developments in radio astronomy technology.
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EM COMPONENTSUPDATE & PERFORMANCE RESULTS S. Srikanth Critical Design Review GBT K-Band Focal Plane Array January 30-31, 2009
KFPA Feed Frequency 18-26.5 GHz Feed taper -13 dB Compact/Profile taper horn Ring-loaded corrugations Aperture ID = 2.93” (5.5λ22) OD = 3.4” Length = 6.658” Pitch = 0.082” (λ18/8) Vane = 0.026” Depth = 0.13” (0.28λ26.5) 69 corrugations Θi = 8º ; Θmax = 17º
Layout of Elements (61 feeds) Element spacing 3.45” 1+6+12+18+24
22 GHz; Telescope beams in Azimuth (asym.) planeHPBW = 34” Beam throw 27.4”/inch; 0.43HPBW/λ
22 GHz; Telescope beams in Elevation (symm.) planeHPBW = 34” Beam throw 27.4”/inch; 0.43HPBW/λ
Feed Offset & Aperture Efficiency Circle #1 (3.4”rad): 7 feeds 62.9% min. Circle#2 (6.9”rad): 19 feeds 62.9% min. Circle#3 (10.4”rad): 37 feeds, 61.7% min. Circle#4 (13.8”rad): 61 feeds, 58.9% (az); 61.6% (el) Circle 18.0” : 91 feeds, 54.7% (az); 60.2% (el)
Beam width & Beam spacing Element spacing 3.45”; Beam spacing 94arcsec Beam throw 27.4 arcsec/”
KFPA (Profile Horn) Feed Vs. 20 GHz (Linear Taper) Feed Measured feed patterns
KFPA (Profile Horn) Feed Vs. 20 GHz (Linear Taper) Feed Telescope beam patterns, Efficiency
KFPA (Profile Horn) Feed Vs. 24 GHz (Linear Taper) Feed Measured feed patterns
KFPA (Profile Horn) Feed Vs. 24 GHz (Linear Taper) Feed Telescope beam patterns, Efficiency
18-26.5 GHz Phase Shifter 0.474 x 0.452; Length 4.84” S. Srikanth, “A Wide-Band Corrugated Rectangular Waveguide Phase Shifter for Cryogenically Cooled Receivers”, IEEE Microwave and Guided Wave Letters, Volume 7, pp. 150-152, June 1997.
ORTHO MODE JUNCTION 6061T6 Aluminum 353 Leaded brass WR42 waveguide; 4.5” x 2.8” Septum 0.010” (Beryl. Cu) Pin 0.040” dia. (Beryl. Cu) E. Wollack, “A Full Waveguide Band Orthomode Junction”, EDIR No. 303, NRAO, May 16, 1996
Measured of S-parameters- Al. OMJ Side arm Main arm