`
`Briefs
`
`CMOS Active Pixel Image Sensor
`
`Sunetra Mendis, Sabrina E. Kemeny, and Eric R. Fossum
`
`Abstract-A new CMOS active pixel image sensor is reported. The
`sensor uses a 2.0 p n double-poly, double-metal foundry CMOS process
`and is realized as a 128 x 128 array of 40 p n x 40 pm pixels. The sensor
`features TTL compatible voltages, low noise and large dynamic range,
`and will be useful in machine vision and smart sensor applications.
`
`I. INTRODUCTION
`Charge-coupled devices (CCD’s) are typically employed for image
`acquisition. While offering high performance, CCD area arrays are
`difficult to integrate with CMOS due to their high capacitances,
`complicating the integration of on-chip drive and signal processing
`electronics. CCD’s are also highly susceptible to image smear. Some
`achievement in on-chip signal processing with CCD’s has been
`reported [ 11-[4] but a fully CMOS-compatible sensor technology
`enabling a higher level of integration would greatly benefit many
`applications [5]. These include machine vision, vehicle navigation,
`video phones, computer input devices, surveillance systems, auto
`focus, and star trackers. Simple p-// junction photodiode arrays have
`been fabricated using CMOS processes but typically have high read
`noise and suffer from image lag [GI. Both bipolar [7] and charge
`modulation device [SI image sensors are compatible with CMOS
`integration, but require specialized fabrication processes. In this
`paper, a new, 100%) CMOS-compatible image sensor with good
`performance is reported.
`
`11. ACTIVE PIXEL SENSOR DESIGN AND OPERATION
`The CMOS active pixel sensor (APS) is shown schematically in
`Fig. 1. In essence, a small single-stage CCD has been fabricated
`in each pixel. For discussing the operation of the image sensor,
`it is assumed that the sensor is operated with voltage rails of 0
`and +.5 V, though higher and lower voltage operation is possible
`and has been demonstrated. Operation of the sensor is as follows.
`During signal integration, the pixel photogate (PG) is biased at +5
`V, the transfer gate TX and reset transistor R are biased at +2.5
`V, and the selection transistor S is biased off (0 V). Following
`signal integration, all pixels in the row to be read are read out
`simultaneously onto column lines by the following process. First,
`the pixels are addressed by the row selection transistor S biased
`at +5 V. This activates the source-follower output transistor in
`each pixel (the load transistor is located at the bottom of the pixel
`column and is biased at $2.5 V). The reset gate R is then briefly
`
`Manuscript received June 14, 1993; revised October 11, 1993. The review
`of this brief was arranged by Associate Editor W. F. Kosonocky. This work
`was supported in part by the Defense Advanced Research Projects Agency
`and in part by the National Aeronautics and Space Administration.
`S . Mendis is a student in the Dept. of Electrical Engineering, Columbia
`University, New York, NY 10027.
`S . E. Kemeny and E. R. Fossum are with the Center for Space Mi-
`croelectronics Technology, Jet Propulsion Laboratory, Califomia Institute of
`Technology, Pasadena, CA 91 109.
`IEEE Log Number 92 14896.
`
`IEEE TRANSAnIONS ON ELECTRON DEVICES. VOL. 41, NO. 3, MARCH 1994
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`Fig. 1. Schematic illustration of image sensor circuit. Dotted line shows
`boundary of in-pixel circuits. The remainder of circuit is at bottom of column.
`
`pulsed to +5 V to reset the floating diffusion output node FD to
`amroximatelv Jr3.5 V. The outDut of the source follower is then
`sampled onto a holding capacitor at the bottom of the column. The
`photogate PG is then pulsed low to 0 V (with TX held at +2.5
`V) to transfer the integrated signal charge under the photogate to
`the floating diffusion output node FD. The new source follower
`output voltage is sampled onto a second holding capacitor at the
`bottom of the column. Storing the reset level and the signal level on
`separate capacitors permits correlated double sampling of the pixel
`[9], eliminating kTC noise from the pixel, and suppressing I/f noise
`and fixed pattern noise from the output transistor. In this circuit, the
`major source of readout noise is the kTC noise introduced by the
`sample/hold capacitors, since kTC noise from the pixel is suppressed
`by the differential output technique. The rms noise on these 1 pF
`capacitors is estimated to be 64 p V per capacitor, or 91 p V in
`differential mode.
`All transistors were sized for readout at the rate of 30pHz cor-
`responding to a row readout time of 260 ps/row. The total time to
`capture the row signal, in parallel, to the bank of capacitors at the
`bottom of each column was designed to be 0.7 p s . The capacitors
`are sequentially scanned for serial readout.
`The APS was designed using highly conservative 2 pm p-well
`CMOS design rules and practices. The array was sized at 128 x 128
`elements for a total die size of 6.8 x 6.8 mm. The fill factor of the
`40 pm x 40 mm pixel, as measured by the ratio of active area (by
`design) to the total pixel area, is 26%.
`The row and column selection 7-10-32 decoders were implemented
`using a 7-input NAND gate designed to fit in the 40 p m pixel pitch.
`The PG and R pulses were gated with the row selection. The reset
`and signal channels for each column were laid out to be as symmetric
`as possible to ensure good common-mode rejection and differential
`output. The digital decoder was designed to be highly isolated from
`the column-wise analog circuitry. A light shield surrounding the
`imaging area was made using second level metal. A photograph of
`the completed sensor is shown in Fig. 2.
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`IEEE TRANSACTIONS ON ELECTRON DEVICES, VOL. 41, NO. 3, MARCH 1994
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`CMOS has encouraged us to continue to pursue a more highly
`integrated CMOS APS in the near future. A reduction in noise of
`more than a factor of 2, an increase in fill-factor to 35% and reduction
`in FPN to below 0.5% p-p is believed to be readily feasible in later
`generations. The use of 0.8 Lim design rules could yield a 15 jrm x
`15 pm pixel size. Coupled with a microlens technology, the effective
`aperture could reach 65% or more. This initial work paves the way
`for more complex pixel structures and on-chip electronics for robot
`vision, guidance and navigation, and other smart sensor applications.
`
`ACKNOWLEDGMENT
`
`The authors appreciate useful conversations and encouragement
`from their colleagues at JPL, especially B. Pain and R. Gee. The
`support of V. Sarohia of JPL and G. Johnston of NASA HQ is
`gratefully acknowledged. The research described in this paper was
`carried out by the Jet Propulsion Laboratory, California Institute of
`Technology.
`
`REFERENCES
`
`E. R. Fossum, “Architectures for focal-plane image processing,” Optical
`Engineering, vol. 28, no. 8, pp. 865-871, 1989.
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`signal processors,” Proc. I990 IEEE Int. Solid-State Circuits Conf., pp.
`218-219, 1990.
`S. E. Kemeny, E.-S. Eid, S. Mendis, and E. R. Fossum, “Update on
`focal-plane image processing research,” in Charge-Coupled Devices and
`Solid-State Optical Sensors II, Proc. SPIE, vol. 1447, pp. 243-250, 1991.
`S. E. Kemeny, H. Torbey, H. Meadows, R. Bredthauer, M. LaShell, and
`E. R. Fossum, “CCD focal-plane image reorganization processors for
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`3, pp. 398-405, 1992.
`E. R. Fossum, “Active pixel sensors: are CCD’s dinosaurs?,” in Charge-
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`M. White. D. Lampe, F. Blaha, and I. Mack, “Characterization of surface
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`
`Fig. 2. Photograph of fabricated 128 x 128 CMOS APS array.
`
`Fig. 3. Unprocessed output of 128 x 128 CMOS active pixel sensor.
`
`111. EXPERIMENTAL RESULTS
`The image sensors were driven in accordance to the timing and
`voltage levels described above. A sample image is shown in Fig. 3.
`Using an electrical test circuit on a separate IC, output conversion
`was determined to be 4.0 jrV/electron. Saturation was measured to be
`600 mV, or 150 000 electrons. The saturation level was determined
`by the output amplifier rather than well capacity since the 2.5 V well
`capacity was estimated to be approximately 6 x IO6 electrons for this
`surface-channel device. No lag or smear was observed. The design
`of the CMOS APS reset transistor results in a lateral anti-blooming
`drain so that blooming is suppressed. The fixed pattern noise (FPN)
`was approximately 3.3%’ 11-11 of the saturation level. Dark current was
`found to be well behaved and measured to be 62 e-/ms/pixel or under
`InA/cm2 at ambient temperature. Dark current shot noise determines
`the noise floor of 42 e-rms at a 30 Hz frame rate at room temperature,
`corresponding to a dynamic range of 71 dB.
`
`IV. CONCLUSION
`loo’/: CMOS active pixel
`image sensor has been
`A new,
`demonstrated. The high performance obtained using standard foundry