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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. The illumination is turned on at 10-8 s.

Beeman, Lawrence Berkeley Laboratory) Fig. 11 Eeam pattern of the seven bolometer array obtained on Uranus with the IRAM 30 m telescope. 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.

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.

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Advanced Far Infrared Detectors


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