Specific detectivity, or ''D*'', for a
photodetector
Photodetectors, also called photosensors, are sensors of light or other electromagnetic radiation. There is a wide variety of photodetectors which may be classified by mechanism of detection, such as photoelectric or photochemical effects, or by ...
is a
figure of merit used to characterize performance, equal to the reciprocal of
noise-equivalent power (NEP), normalized per square root of the sensor's area and frequency bandwidth (reciprocal of twice the integration time).
Specific detectivity is given by
, where
is the area of the photosensitive region of the detector,
is the bandwidth, and NEP the noise equivalent power in units
It is commonly expressed in ''Jones'' units (
) in honor of
Robert Clark Jones who originally defined it.
[R. C. Jones, "Proposal of the detectivity D** for detectors limited by radiation noise," ''J. Opt. Soc. Am.'' 50, 1058 (1960), )]
Given that noise-equivalent power can be expressed as a function of the
responsivity (in units of
or
) and the
noise spectral density (in units of
or
) as
, it is common to see the specific detectivity expressed as
.
It is often useful to express the specific detectivity in terms of relative noise levels present in the device. A common expression is given below.
:
With ''q'' as the electronic charge,
is the wavelength of interest, ''h'' is Planck's constant, ''c'' is the speed of light, ''k'' is Boltzmann's constant, ''T'' is the temperature of the detector,
is the zero-bias dynamic resistance area product (often measured experimentally, but also expressible in noise level assumptions),
is the quantum efficiency of the device, and
is the total flux of the source (often a blackbody) in photons/sec/cm².
Detectivity measurement
Detectivity can be measured from a suitable optical setup using known parameters.
You will need a known light source with known irradiance at a given standoff distance. The incoming light source will be chopped at a certain frequency, and then each wavelength will be integrated over a given time constant over a given number of frames.
In detail, we compute the bandwidth
directly from the integration time constant
.
:
Next, an average signal and
rms noise needs to be measured from a set of
frames. This is done either directly by the instrument, or done as post-processing.
:
:
Now, the computation of the radiance
in W/sr/cm² must be computed where cm² is the emitting area. Next, emitting area must be converted into a projected area and the
solid angle
In geometry, a solid angle (symbol: ) is a measure of the amount of the field of view from some particular point that a given object covers. That is, it is a measure of how large the object appears to an observer looking from that point.
The po ...
; this product is often called the
etendue. This step can be obviated by the use of a calibrated source, where the exact number of photons/s/cm² is known at the detector. If this is unknown, it can be estimated using the
black-body radiation
Black-body radiation is the thermal electromagnetic radiation within, or surrounding, a body in thermodynamic equilibrium with its environment, emitted by a black body (an idealized opaque, non-reflective body). It has a specific, continuous sp ...
equation, detector active area
and the etendue. This ultimately converts the outgoing radiance of the black body in W/sr/cm² of emitting area into one of W observed on the detector.
The broad-band responsivity, is then just the signal weighted by this wattage.
:
Where,
*
is the responsivity in units of Signal / W, (or sometimes V/W or A/W)
*
is the outgoing radiance from the black body (or light source) in W/sr/cm² of emitting area
*
is the total integrated etendue between the emitting source and detector surface
*
is the detector area
*
is the solid angle of the source projected along the line connecting it to the detector surface.
From this metric noise-equivalent power can be computed by taking the noise level over the responsivity.
:
Similarly, noise-equivalent irradiance can be computed using the responsivity in units of photons/s/W instead of in units of the signal.
Now, the detectivity is simply the noise-equivalent power normalized to the bandwidth and detector area.
:
References
{{FS1037C
Physical quantities
Infrared imaging