Lecture CMOS - Center for Detectors

Download Report

Transcript Lecture CMOS - Center for Detectors

Detectors
RIT Course Number 1051-465
Lecture CMOS Detectors
1
Aims for this lecture
• To describe CMOS hybrid and monolithic detectors
– physical principles
– operation
– and performance of CMOS detectors
• Given modern examples of CMOS detectors
2
Lecture Outline
•
•
•
•
•
CMOS detector definition
CMOS detector principles of operation
Performance of modern CMOS detectors
Examples of CMOS detectors
Historical context of CMOS detectors
3
CMOS Detector Architectures
4
CMOS Detector Definition
• CMOS detectors are made of complimentary MOSFET
circuits connected to light-sensitive materials.
• The voltage change due to integrated photogenerated charge is
generally sensed directly through a source follower amplifier
in each pixel, instead of via a charge transfer process, i.e. in
CCDs.
• Charge is sensed as a voltage directly in the pixel and is not
reset every time it is sensed, unlike in a CCD.
• The readout circuit is often called a “multiplexer” because it
can sequentially direct signals from multiple pixels to an
individual output amplifier.
• Historically, they have been developed later than CCDs, and
first for infrared astronomy detectors.
5
CMOS vs. CCD Readout
• CMOS has “direct readout (DRO)” random access
architecture.
• (Note that the CMOS device in the figure has readout circuitry
that takes up some real estate – it is frontside illuminated,
producing non-ideal fill factor.)
6
CMOS Detector Types
• Monolithic (“one piece”)
– readout and photodiode integrated in same part, which means that light
sensitive layer is made of silicon (only sensitive to optical photons)
– frontside or backside illuminated
– can be made with mostly standardized CMOS processes that are
common to the commercial semiconductor industry
• Hybrid (“two pieces”)
–
–
–
–
readout circuit is separate from photodiode
readout is made of silicon
photodiode is made of semiconductor with suitable cutoff wavelength
requires many custom steps
7
Hybrid Architecture
8
Hybrid Array Benefits
• Hybrid arrays are used when one wants to detect light of
wavelengths that are not absorbed by silicon, i.e. wavelengths
beyond ~1um.
• Infrared arrays are “hybrids” – they use one material to detect
light and silicon for the readout circuit.
9
Hybrid Array Detection Flow
10
Hybrid Array Architecture
11
Hybrid Array Bonding
12
Hybrid Array Summary
13
Hybrid Array Key Technologies
14
CMOS Hybrid Detector Example: InSb Array
15
CMOS Hybrid Detector Example: NICMOS Array
16
Infrared Hybrid Array Substrate Removal
17
Readout Integrated Circuit (ROIC)
also known as the Multiplexer
18
Detector Unit Cell
19
Detector Multiplexer
20
Detector Operation
21
NICMOS MUX
22
Light-sensitive Materials
23
Periodic Table
• Semiconductors occupy column IV of the Periodic Table
• Outer shells have four empty valence states
• An outer shell electron can leave the shell if it absorbs enough
24
energy
Periodic Table Continued
• The column number gives the number of valence electrons per
atom. Primary semiconductors have 4.
• Compounds including elements from neighboring columns can
be formed. These alloys have semiconductor properties as well
(e.g. HgCdTe & InSb).
• Mercury-cadmium-telluride (HgCdTe; used in NICMOS) and
indium-antimonide (InSb; used in SIRTF) are the dominant
detector technologies in the near-IR.
25
The Band Gap Determines the Red Limit
E G  hc 
hc
c
.
(1)
26
Performance
27
Dark Current
• Dark current is the signal that is seen in the absence of any
light.
• The dominant components are diffusion across the pn junction,
thermal generation-recombination (G-R) of charges within the
bulk of the semiconductor, and leakage currents typically
through surfaces.
• Dark current adds an effective noise due to the shot noise of
the dark charge.
• Dark current can be reduced by cooling.
28
Dark Current Example
29
Dark Current vs. Temperature
30
Read Noise
• Read noise is the uncertainty in the signal measurement due to
electrical fluctuations produced by the detector.
• For CMOS devices, it is due to:
– Johnson noise of FETs
– random telegraph signal (a.k.a. popcorn noise) in the output FET
– interface states at material surfaces
• Typical read noise values for CMOS devices are around 10
electrons.
31
Read Noise Example
32
Sampling Schemes
• By being a bit clever about reading out the array, one can
minimize or eliminate some of these noise modes.
• During an exposure, typically each pixel is sampled several
times.
• The most common approaches are correlated double sampling
(CDS), multiple non-destructive reads (aka “Fowler
Sampling”), & fitting a line (aka “up the ramp”).
33
Fowler Sampling
1 N
1 N
V   Vi j   Vf j
N j 1
N j 1
34
“Up the Ramp”
•
•
•
•
Fit best line to multiple non-destructive samples.
Sample spacing does not need to be uniform.
Not clear whether this or Fowler sampling is best.
This is what is done in NICMOS MULTIACCUM mode.
35
Hybrid Array Optimization – Quantum Efficiency
36
Well Depth and Non-linearity
• Well capacity is defined as the maximum charge that can be
held in a pixel.
• “Saturation” is the term that describes when a pixel has
accumulated the maximum amount of charge that it can hold.
• The “full well” capacity in a CCD is typically a few hundred
thousand electrons per pixel for today’s technologies.
37
Well Depth and Non-linearity Example
38
Non-linearity Example
39
Persistence
• Persistence is the afterimage that a detector can produce if it
traps charge from a previous exposure and releases it during
the current exposure.
• It is produced by charge traps.
• Charge traps will decay with an exponential timescale.
40
Persistence Example
41
Persistence Movie
42
Pixel-to-pixel Crosstalk
• Crosstalk is the generic term that describes signal
contamination due to the presence of a signal in another pixel
or electrical channel.
• Charge diffusion from one pixel to a neighbor is an important
crosstalk mechanism in IR arrays and CCDs.
• Once charge carriers are created, their motion is governed by
charge diffusion.
43
IPC
• Interpixel capacitance (IPC) is a form of crosstalk.
• In this case, charge in a pixel induces a voltage change in a
neighbor, just like the behavior between parallel plates in a
capacitor.
• The effect is to blur the point spread function.
• The induced voltage does not have noise.
44
IPC
• In this example, IPC is very large for the H4RG SiPIN device
(10 um pixel size).
45
Arrays in Use Today
46
Teledyne H4RG Si PIN
• This is an image of the H4RG device in the Rochester
Imagingn Detector Laboratory (RIDL).
47
Raytheon Family Arrays
48
Hybrid Visible Silicon Imager - HyViSI
49
HyViSI
50
HyViSI
51
Modern Array Examples
52
History of Hybrid Infrared Arrays
53
History of Infrared Detection
•
•
•
•
•
•
•
•
Herschel’s detection of IR from Sun in 1800
Johnson’s IR photometry of stars (PbS) mid 60’s
Neugebauer & Leighton: 2mm Sky Survey (PbS), late 60’s
Development of bolometer (Low) late 60’s
Development of InSb (mainly military) early 70’s
IRAS 1983
CMOS Hybrid Arrays (InSb, HgCdTe, Si:As IBCs) mid-80’s
NICMOS, 2MASS, IRTF, UKIRT, KAO, common-user instruments,
Gemini, etc.
• JWST
54
Science Motivation
• Exploration & discovery
– Neugebauer, Leighton, Low, Fazio, Townes
• Technological opportunities
– Bolometer (Low), PbS (Neugebauer), balloons (Fazio), IR lasers &
interferometry (Townes)
• A few, key problems
– Bolometric luminosities (Herschel, Johnson)
– The Galactic Center (Becklin)
– Star formation
55