TY - JOUR
T1 - High Accuracy Pointing for Quasi-optical THz Mixer Arrays
AU - Gasparsilva, Jose Rui
AU - Finkel, Matvey
AU - Laauwen, Wouter
AU - Westerweld, Menno
AU - More, Nikhil
AU - Young, Abram
AU - Kulesa, Craig
AU - Walker, Christopher
AU - Van der Tak, Floris
AU - Gao, Jian Rong
N1 - Publisher Copyright:
© 2011-2012 IEEE.
PY - 2022/1/1
Y1 - 2022/1/1
N2 - We report a high accuracy pointing technique for quasi-optical hot electron bolometer (HEB) mixers in focal-plane arrays designed to operate at 1.4, 1.9, and 4.7 THz. The high accuracy pointing is achieved by prealignment of a HEB chip to a lens, measuring the angular error of each mixer in an array assembly, and then realignment of the chip to the same lens to correct the error. The realigned mixers, using 5 mm diameter Si elliptical lenses designed for operation at 4.7 THz, show a final pointing error distribution with an average (μ) = 0.13° and standard deviation (σ) = 0.06°, with respect to the normal direction of the respective array plane. Those using 10 mm diameter lenses designed for operation either at 1.4 or 1.9 THz, show μ = 0.08° and σ = 0.03°. We demonstrated our pointing technique in five 4×2 HEB focal plane arrays developed for NASA's balloon borne GUSTO THz observatory. Our results corroborate the simulated beam steering factors used to calculate the realignment corrections. With the unprecedented pointing accuracy at the high frequencies, our technique can significantly facilitate the use of lens-antenna, quasi-optical mixers for future focal-plane arrays, which is able to compete with traditional feedhorn-waveguide mixer arrays, operated typically below 1 THz, for astronomical instrumentation.
AB - We report a high accuracy pointing technique for quasi-optical hot electron bolometer (HEB) mixers in focal-plane arrays designed to operate at 1.4, 1.9, and 4.7 THz. The high accuracy pointing is achieved by prealignment of a HEB chip to a lens, measuring the angular error of each mixer in an array assembly, and then realignment of the chip to the same lens to correct the error. The realigned mixers, using 5 mm diameter Si elliptical lenses designed for operation at 4.7 THz, show a final pointing error distribution with an average (μ) = 0.13° and standard deviation (σ) = 0.06°, with respect to the normal direction of the respective array plane. Those using 10 mm diameter lenses designed for operation either at 1.4 or 1.9 THz, show μ = 0.08° and σ = 0.03°. We demonstrated our pointing technique in five 4×2 HEB focal plane arrays developed for NASA's balloon borne GUSTO THz observatory. Our results corroborate the simulated beam steering factors used to calculate the realignment corrections. With the unprecedented pointing accuracy at the high frequencies, our technique can significantly facilitate the use of lens-antenna, quasi-optical mixers for future focal-plane arrays, which is able to compete with traditional feedhorn-waveguide mixer arrays, operated typically below 1 THz, for astronomical instrumentation.
KW - antenna arrays
KW - Antenna measurements
KW - Antenna radiation pattern
KW - beam steering
KW - cryogenic
KW - Lenses
KW - lenses
KW - Mixers
KW - Quantum cascade lasers
KW - Receivers
KW - Semiconductor device measurement
KW - Silicon
KW - terahertz radiation
UR - http://www.scopus.com/inward/record.url?scp=85117075183&partnerID=8YFLogxK
U2 - 10.1109/TTHZ.2021.3118607
DO - 10.1109/TTHZ.2021.3118607
M3 - Article
AN - SCOPUS:85117075183
SN - 2156-342X
VL - 12
SP - 53
EP - 62
JO - Ieee transactions on terahertz science and technology
JF - Ieee transactions on terahertz science and technology
IS - 1
ER -