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Extra resources for Advanced Far Infrared Detectors
Contour levels are in percent of peak intensity. , Ref. 59) Fig. 12 The SCUBA 91 pixel and 37 pixel NTD Ge bolometer arrays development for the James Clerk Maxwell submillimeter telescope. Cunningham and Gear, Ref. 61) 31 under (Courtesy ! u') i ! i D_ I I i q_ 0 _ ----- r_ IV , lr III I III Fig. 32 Z. 1 Fig. 33 2 03 | I::: NA- 1012 l0 8 04 P lO , 0 oO I 0 I I I ' POSITION u. _... 1,1 935-592 Fig. 34 3 Fig. 35 4 Fig. Lm) uJ Z 0 Q- 100 50 I I , 40, I 30 25, I I 20, stressed uJ 13:: Ge:Ga Ge:Ga Ge:Be Si:B " i-0 Z 0 0 0 p.
I I 0 _ 0_ IlJllll I IlUlll 0 _ I llUlll 011--I lUUlII CD _ _ I INUlII I T C_. C_I 41 Fig. I0 Z rv ::::) I I I, -b 42 r_.
Neutral (A°). photons can ionize neutral acceptors forming a free hole (_) charged acceptor (A-). Incoming and a negatively The free hole drifts an average distance 1 before it recombines with an A-. Fig. 2 The near-contact band diagram showing the Fermi level position relative to the valence band edge. (Courtesy Haegel and White, Ref. 6) Fig. 3 illuminated. mV) p+-p-p+ and Ge:Ga (Courtesy Haegel and White, Ref. 6) Fig. 4 Mesh plot of the relative free hole increase as a function of position and time in a homogeneously illuminated p+-p-p+ Ga:Ge photoconductor.
Advanced Far Infrared Detectors