When an intensity-modulated beam is used to illuminate diffusive media, the modulation amplitude and phase of the beam are attenuated and delayed, respectively, due to absorption and scattering inside the medium. The amplitude attenuation is caused by both scattering and absorption, whereas the phase delay is mainly related to scattering. Because the typical modulation frequency range in frequency-domain diffusive imaging is from tens of megahertz up to a gigahertz,12.–3 a very high bandwidth detector is required to correctly measure modulation amplitudes and phases. In additional to measuring the frequency-response information, it has been shown that obtaining large datasets using detector arrays also improves diffusive imaging performance.4,5 It is almost impossible to achieve the high bandwidths required in frequency-domain measurements with high-density detector arrays such as charge-coupled device (CCD) or complementary metal-oxide-semiconductor (CMOS) sensors. Heterodyne and/or homodyne (hetero/homodyne) methods extract the amplitude and phase information by converting the rapidly modulating output beam into a beat-frequency modulation mode using gain-modulated amplifiers, such as an image intensifier (IIN) and photo multiplier (PMT).6,7 When the gain modulation frequency is slightly different from that of a light source, the amplified output modulates at the frequency difference—a beat frequency, which is a heterodyne measurement. For a homodyne measurement, where a gain is modulated at the same frequency as a modulation source, the output is stable in time, but its irradiance is varied along the heterodyne output according to relative phases between source and gain modulations. Although time-domain measurements can also extract the frequency response of diffusive media, hetero/homodyne measurements are more widely used in diffusive imaging because of their relatively low cost and simplicity.1,6
In general, measuring intensity-modulated outputs improves the reconstruction algorithms and other algorithms designed to estimate tissue properties, when compared to measuring just diffused intensities (i.e., steady-state measurements).1 For example, diffuse optical tomography (DOT), which is considered a noninvasive and cost-effective medical imaging tool, can tomographically reconstruct images of scattering and absorption coefficients up to tens of millimeters in depth.2,3 DOT systems based on just a diffused intensity are simple and inexpensive but have significant disadvantages including the measurement variability caused by skin structure, hair, and surface roughness.1 Furthermore, the measured diffused intensity generally cannot reconstruct a unique solution, and the crosstalk between absorption and scattering coefficients cannot be effectively separated in reconstruction processes.8,9 A frequency-domain DOT can remedy these problems and thus improves detectability and reconstruction performance. Frequency-domain measurements are also required in fluorescent lifetime imaging (FLI), where the fluorophore lifetime is used as an important indicator of tissue characteristics.10 Since the typical fluorescent lifetimes are a few nanoseconds and cannot be measured directly, measuring attenuated amplitude and delayed phase of modulated fluorescent photons can be used effectively to estimate the lifetime.7,1112.–13 Measuring the frequency-domain information in large tissue areas using a CCD and a gain-modulated IIN can be used to generate a spatial fluorescent lifetime map of the tissue.14
Noise is inherent in all measurements. Even though averaging multiple measurements or increasing detector exposure time can reduce the amount of noise, these approaches are prohibited or limited in some dynamic-imaging applications and clinical situations.1 In medical imaging, data are acquired for specific purposes or tasks that include classification, such as detection of abnormalities like a tumor, and estimation of biological quantities, such as a fluorescent lifetime. Noise-contaminated data is a limiting factor in an observer’s ability to perform these classification and/or estimation tasks. The noise is especially significant in diffusive medical imaging, such as DOT and FLI, because of low photon counts.118.104.22.168.–17 The performance of noise-contaminated systems can be evaluated quantitatively by considering figures of merit (FOMs) that are chosen to reflect an observer’s ability to perform these medial-relevant tasks.15,18 Task-based assessment of image quality evaluates and/or optimizes diffusive imaging systems by employing FOMs that assess observer performance.1819.–20 Many task-based FOMs rely on the first and second moments of output data,18,21,22 so understanding the noise property of output data is important and necessary.
Because of the importance of noise analysis in diffusive imaging, the noise characteristics of a modulation amplitude and phase for frequency-domain diffusive imaging have been previously investigated. Toronov et al.23 mathematically derived variances of these quantities in frequency-domain DOT assuming a quantum shot noise model on the hetero/homodyne outputs. Conventional signal-to-noise ratios (SNRs) and a task-based FOM known as a Hotelling observer SNR were derived based on Toronov’s result, and an optimal modulation frequency was explored in DOT systems of a single point source and CCD-based phased array.16,2324.–25 In FLI, a FOM called -value is commonly used to evaluate system performance, where the -value is defined by first- and second-order statistics of a fluorescent lifetime.12,13 Many investigators have optimized FLI systems by maximizing the -value or minimally required fluorescent photon numbers for a meaningful -number.12,13,26 It is reasonable that the -value is strongly dependent on the noise characteristics of modulation amplitude and/or phase in frequency-domain FLI because the fluorescent lifetime is estimated from these quantities. For all previous studies including Toronov’s result, however, Gaussian or shot noise is simply considered for the statistics of modulation amplitude and phase or only shot noise is assumed for the hetero/homodyne outputs,9,23 which might not be valid in reality. For example, the irradiance of hetero/homodyne outputs is usually high due to the photon amplification process, which is enough to ignore the effect of shot noise in a detector. Furthermore, the beat-frequency modulated output might be temporally correlated, which is seriously harmful to the assumption of quantum shot noise.
The noise properties of amplified photons for the non-modulation case have already been investigated, where incident photons are assumed to be Poisson distributed. The photon amplification in IINs and intensified CCDs (ICCDs) should be considered a random process even for a constant gain, which generally induces non-Poisson outputs for Poisson inputs.18 Bell theoretically analyzed a noise figure for IINs with a constant gain,27 where the noise figure was defined as the ratio of SNRs of input and output photons. He considered photons incident on a micro channel plate (MCP) in IINs or ICCDs as governed by Poisson statistics, and each photoelectron collision on the wall of the MCP generates the photoelectron distribution called Furry distribution. Moran et al.28 theoretically derived a noise factor () of ICCDs, which is defined as the square of the noise figure. He showed that variations of a and an output SNR are not linearly related to MCP gain, which is partially observed in experiments elsewhere.17,29 Moran adapted a Polya distribution as a single photoelectron pulse in a MCP. Instead of photoelectron distributions in a MCP, Apanasovich and Novikov30 analyzed the amplification process considering electron multiplication events in a MCP as random point processes and compared the theoretical model with experiments. Frenkel et al.31 investigated variance and noise-equivalent irradiance of outputs in an ICCD using the approach of spatial point processes. Although these previous noise analyses for randomly amplified photons are mathematically sound, to the author’s knowledge, noise analysis has not been performed for heterodyne/homodyne measurements where both incident beam and amplification gain are modulating. Spring and Clegg32 briefly touch on the SNR of homodyne outputs, but gain modulation is simply substituted for the constant gain in the conventional SNR expression for PMTs.
In this paper, we theoretically derive mean and covariance properties of hetero/homodyne outputs, which are expressed with systematic parameters of hetero/homodyne measurements, such as dc and ac parts of incident primary modulation beams and modulation gain. The theoretical development includes both temporal and spatial analyses. Temporally, a hetero/homodyne measurement process is considered random amplification of a modulated temporal point process. Spatially, a multinomial selection rule is applied to model the spatial distribution of the amplified photons from MCPs to detector array pixels. Resulting from this, it is found that hetero/homodyne outputs are temporally uncorrelated and the variance oscillates like the mean in some specific conditions. We suggest experimental results of homodyne measurements that show similar characteristics with what is expected from the developed theory. Discussions for the influence of the derived noise property on frequency-domain diffusive imaging are also presented.
Theory for Temporal Noise Analysis
For hetero/homodyne detection processes in diffusive imaging, the diffused photons exiting an object (e.g., phantom) are captured by an imaging system, where the exit face is imaged onto a cathode of an IIN through the imaging system. The incident photons to the cathode generate photoelectrons that are injected into the MCP of the IIN, where the voltage difference between the cathode and the MCP determines the amount of injected photoelectrons. A MCP is typically composed of millions of small channels that are related to the overall resolution of an IIN. A single photoelectron collision that occurred on the wall of the MCP generates multiple photoelectrons, the number of which is proportional to the voltage applied to the MCP. The overall gain of the IIN is determined mainly by photoelectrons generated from the cathode and the MCP voltage that are independent of a cathode voltage. To achieve gain modulation in an IIN, a modulated voltage is applied to a cathode to generate modulated photoelectrons that are amplified in a MCP. The multiplied photoelectrons from the MCP are accelerated to an anode (phosphor) to generate intensified photons. The usual decay time of phosphors ranges from hundreds of nanoseconds to a few milliseconds.33 The photons discharged from the anode are transferred to a detector array, such as a CCD or CMOS, by an appropriate imaging system. Overall, a phantom exit face and a CCD detector surface are object and image planes, respectively, of the whole frequency-domain measurement system. Resulting from this view, each CCD detector pixel is conjugate to a detection area on the exit face, the size of which is determined by the CCD pixel size and the transverse magnification of the whole hetero/homodyne imaging system.
It is assumed that hetero/homodyne output photons are described by a temporal point process as1), and are numbers of primaries and secondaries, respectively; these are all random variables. The mean and covariance of the point process of Eq. (1) have been derived for the case of non-modulation input and IIN gain.18,34 Referring to this known procedure, we will develop the mean and covariance of for hetero/homodyne measurements. A mean photon arrival rate from a phantom to a cathode of the IIN is expressed as 2). If we assume that Poisson postulates are fulfilled for the diffused photons on the detection area, the probability density function (PDF) for the primary is18 2) is not random, which indicates that noise external to the hetero/homodyne system, such as random biological motions and respiration, will not be considered in this theoretical development.
The shift-variant temporal point spread function (PSF) of the IIN with gain modulation can be described as5) indicates a modulated photoelectron rate from the cathode for a single primary, which is equivalent to cathode gain modulation. The term is the same as or close to in hetero/homodyne measurements. Because the modulation voltage should be applied to around the cutoff voltage of a cathode, the modulated cathode gain is generally similar to a bottom-truncated sinusoidal function rather than a perfect sinusoidal curve.32 It is noted that for this case, the largest coefficient in the cathode modulation could be larger than 1 because is defined by averaging the modulated cathode gain. The periodic cathode gain is expanded to Fourier cosine terms,32 as shown in Eq. (5), where the amplitude and phase of each term is indicated as and , respectively. From the assumption that the gain is an even and periodic function, it can be easily shown that there is no phase difference between cosine terms (we set all as zeros for simplicity) and , where is an integer. The usual photocathode response time of a cathode is picoseconds to femtoseconds,35 so the photoelectron conversion time on a cathode is ignored in Eq. (5). The time for multiplying photoelectrons in the MCP is also negligible compared with the photoelectron-photon conversion time on an anode, which is usually a few milliseconds. The random variable for the secondary in Eq. (5) is not independent of each other because is correlated to . If in Eq. (5) is replaced by as in Eq. (1), can be considered statistically independent and Poisson postulates are satisfied for secondaries produced from each primary.18 With this replacement, the probability density function (PDF) for secondary photons can be written from Eq. (5) as 7), indicates the mean number of amplified photons for a single photoelectron injected into the MCP. The time dependence in indicates a long-term MCP and/or anode variation caused by, for example, thermal instability. We are interested in the noise property of a hetero/homodyne output that is stationary in time, thus assuming . Also, photon and photoelectron losses, such as cathode quantum efficiency and an open area ratio of the MCP,27 could be included in in Eq. (7).
Mean and covariance of Eq. (1) can be derived by statistically averaging the time for secondary , the number of secondaries , the time for primary , and the number of primaries . As a final step, averaging would be necessary if the primary is doubly stochastic, but this is not the case as we assumed before. As shown in the appendix, the mean and covariance are derived from Eqs. (2) to (7) as9) indicates variance of secondary photons produced by a single primary photon. Applying trigonometric identities to the integrand in Eq. (8) generates dc, , , , and other high-frequency terms. Except the dc and (i.e., the integer ) terms, all other modulation terms are averaged out because the decay time of in Eq. (5) is much larger than modulation periods of these terms. Also, the typical beat frequency for heterodyne measurements is much shorter than , so for the dc and terms. With these descriptions, Eq. (8) is simplified to 10) is physically reasonable and in agreement with conventionally experienced hetero/homodyne outputs. For the case of homodyne, where , the phase difference changes to measure the trajectory of the beat-frequency modulated output. The unit of Eq. (10) is the same as , a photon rate (i.e., units of and are photonelectron/primary and secondary/photoelectron, respectively), so multiplying a detector exposure time to Eq. (10) measures the mean output photons.
We define the Fano factor,18 , for secondaries per primary as11) makes the integrand of in Eq. (9) the same as Eq. (10) with the multiplication of . The remaining mean square term in Eq. (9) is further developed by substituting Eq. (7) to . Removing and higher modulation frequency terms, the integrand of results in 12), are survived because of the relatively long decay time of in Eq. (9). Therefore, the covariance of Eq. (9) becomes 9). Notice that this Dirac delta function approximation is valid only if the detector integration time for each measurement point is much longer than the decay time of . However, should be much shorter than of heterodyne outputs. Therefore, the range of validating the uncorrelation of the covariance depends on a phosphor of the IIN and a beat frequency of heterodyne outputs. If all are zero, which means non-modulated gain in the IIN, the variance of Eq. (13) becomes the well-known result of the Burgess Variance theorem18,36 for Poisson inputs. For gain modulation as in hetero/homodyne measurements, the covariance of Eq. (13) modulates at the beat frequency like the mean of Eq. (10), where dc () and ac () variances can be considered separately. Notice that in Eq. (13) is increased by the factor of , compared with the variance for a non-modulated input (), which is the effect of the gain modulation.. Both and are strongly dependent on and , which is an overall dc gain of the IIN, and affects only . Since we discuss mean and variance of output photons, is the photon number with the multiplication of , which is unitless, as the mean.
Theory for Spatial Noise Analysis
The mean and covariance of Eqs. (10) and (13) are derived based on the temporal PSF of an IIN, as shown in Eq. (5), where the effect of spatial distribution of the PSF is omitted. The temporal consideration would be valid for photoelectrons from a MCP output pore because photoelectrons incident into each MCP input pore are Poisson and MCP channels are physically separated from each other. As shown in Fig. 1(a), however, secondaries from a single MCP output pore are spatially distributed to multiple CCD pixels, which should be considered for the noise analysis of photons detected on a CCD. It is reasonable to assume that the event of detecting one photon among secondaries from a specific MCP output pore by a certain CCD pixel does not affect other secondary photons from the MCP output pore. With this assumption, the spatial distribution of secondaries is theoretically described by a multinomial selection rule.18
To simplify the mathematics, simplified terminologies are used for the spatial noise analysis. If the number of total photons detected by the ’th CCD pixel during some measurement time is ,14) is for all MCP output pores contributing to . Like the temporal noise analysis, is assumed to be much longer than an anode decay time in the IIN. The mean is derived as 15), averaging is done for two random variables and with a multinomial PDF and that is unknown, respectively. For convenience, these two averages are denoted as and to calculate the covariance . The second moment of is 18 photoelectrons incident into each MCP input pore are also Poisson, which indicates that in Eq. (16) can be approximated to . Then, from Eq. (16), the covariance is 16) to derive Eq. (17). The variance of photons detected on a single CCD pixel (i.e., ’th pixel) is given by in Eq. (17). of Eq. (17) shows that measured images on a CCD from an IIN are spatially correlated and the correlation length is mainly determined by . It is known that the efficiency of a photon transferring from an anode to a CCD in a typical IIN having a relay lens imaging system is . Therefore, the first term in Eq. (17) cannot be ignorable for the variance, unless is much higher than . We insist that the spatial noise property shown in Eq. (17) is general in IINs and should be considered even for a PMT. In a PMT, only two probabilities of detected and lost photons are considered, so might be much higher than that in IINs. Moran et al.28 analyzed a spatial noise property in ICCDs by introducing a spatiotemporal PSF, but their procedure is very complicated and their result is different from Eq. (17). Experimental results showing the covariance of Eq. (17) in IIN outputs are presented in the next section.
Complete noise expressions of hetero/homodyne measurements are given by combining the temporal and spatial analyses. Resulting from this, dc and ac means and variances on ’th CCD pixel in the frequency-domain measurement are18), we assumed that and of modulated output photons from a phantom slowly vary across the phantom exit surface or the cathode of the IIN, so these quantities are almost the same for each MCP channel contributing to the noise property of photons detected at ’th CCD pixel. This assumption is reasonable because the degree of diffusion (i.e., scattering) of tissues in medical imaging is usually large. It is important that both mean and variance modulate along with these dc and ac means and variances in Eq. (18). Equation (18) also shows that and are approximately different from and , respectively, by the factor of . When the gain of the IIN increases, both and are increased, which indicates that the second terms of in both dc and ac variances are significant. It is expected that although and are increased as increasing the gain, the relative difference between these two variances becomes larger because the multiplication factor in is typically less than 1. Furthermore, Eq. (18) implies that as the modulation gain of the IIN deviates from a perfect sinusoidal function more and more, the noise of the hetero/homodyne is increased more due to higher values for .
The CCD and the IIN used in the experiment are Point Grey F2-08S2M and Lambert Ins. II18MD, respectively. The source is the laser diode (LDH-M-C-650B) from PicoQuant with the modulated diode laser driver, MDL 300. This driver is run by external modulation signals from a Tektronix AFG3252 function generator that also generates modulation signals for the IIN cathode. The CCD is carefully adjusted onto the image plane of the relay lens of the IIN in Fig. 1(a) before the main experiment. Since the experiment of measuring variances usually takes a few hours, the experiment starts after about 2 h of warming-up to thermally stabilize all instruments. Especially, voltages directly measured from the cathode of the IIN show that the cathode is thermally unstable at the initial run, which might cause an unexpected long-term variation during the measurement. The laser diode (LD) beam incident into the IIN is almost spatially flat and speckle-free in intensity, which is achieved by lenses and ground glasses. Also, neutral density filters are used to decrease the power of the LD to avoid damage to the IIN cathode, because harmonic distortions of the modulated LD beam can be minimized by keeping the LD power high.
Figure 1(b) is the averaged variance-normalized spatial covariance calculated from images for non-modulated incident beams to the IIN with a non-modulated gain. The averaging is done with 49 variance-normalized spatial covariance matrices, where each of them is normalized by its own variance. The exposure time is 60 ms, and 2000 images are captured to calculate the spatial covariance. The transverse magnification of the relay lens in the IIN is 0.5 and the CCD pixel size is , so the pixel size on the anode surface in Fig. 1(b) is equivalent to . As shown in Fig. 1(b), the data are spatially correlated, which is caused by the secondary photon distribution from MCP output pores to CCD pixels. Figure 1(c) shows 1-D profiles of calculated spatial covariance matrices for different MCP voltages. The exposure time is adjusted for different MCP voltages so that measured means are almost the same, where Exp60 ms in the legend indicates 60 ms CCD exposure time and highest MCP voltage. As the MCP voltage gets higher (i.e., the IIN gain is higher), the variance becomes larger than the mean for a single MCP output pore, so the contribution of the second term of Eq. (17) to the variance for a CCD pixel is also increased. This is the reason that the width of variance-normalized correlation functions is decreased with decreasing MCP voltage, as shown in Fig. 1(c). It is noticed that the correlation length is almost the same for all three MCP voltages, which indicates that in Eq. (17) is almost independent of a MCP voltage. We observed that even modulating the cathode voltage does not have a large affect on these correlation functions. Figure 1(d) is a variance-normalized temporal auto covariance from data measured at a single CCD pixel for . Since 60 ms of is much longer than the decay time of the phosphor (1 ms to drop 1% of the peak output for P43 in II18MD), data are temporally uncorrelated as expected. The experimental results in Fig. 1 show that the approach of a multinomial PDF for the spatial distribution of secondaries is reasonable and that its effect can be independently considered from the temporal point process analysis.
A homodyne method is used to experimentally measure and of Eq. (18), because it is more appropriate for measuring multiple images than a heterodyne method. Applying a high modulation frequency to the cathode in the IIN for a long time could permanently damage the cathode, so the modulation frequency for this experiment is set to 100 kHz. Although 100 kHz is several hundred times lower than a typical modulation frequency used in frequency-domain diffusive imaging, the noise characteristics shown in Eq. (18) can still be observed. Also, CCD pixels are considered a single macro pixel, which increases the reliability of measuring variances without dramatically increasing the number of images, hence reducing the overall measurement time. As the first step, a homodyne profile is measured with 64 phase steps for of the phase difference () between modulation signals applied to the IIN and LD. Homodyne profiles measured at three observer points (ObPs) of a macro pixel are shown in Fig. 2(a), indicating that these profiles are slightly different for different macro pixels. The maximum detector output (bin) is . Each measurement point in these homodyne profiles is produced by averaging 50 homodyne images. Next, the averaged homodyne profile is calculated from 100 homodyne profiles measured at different macro pixels within an arbitrarily chosen local detector area. From this averaged homodyne profile, three ’s corresponding to maximum, dc, and minimum irradiances of the homodyne profile are sought. After these ’s are found, 1000 images are measured for each to calculate means (, , ) and variances (, , ) for all 100 macro pixels within the arbitrarily chosen local detector area. Finally, and are calculated from and , respectively. Macro pixels satisfying the ac mean ratio of and is almost 1 are selected for investigating noise characteristics of Eq. (18), the number of which is out of 100. Macro pixels showing ac mean ratios not close to 1 indicate that their homodyne profiles deviate much from the averaged homodyne profile.
Figure 2(b) shows measured , and their ratios to different MCP voltages that are indicated as numbers in the -axis. for these different MCP voltages are set to 60, 120, 240, and 480 ms. The MCP voltages for these ’s are chosen to make all measured the same, where 1 MCP voltage in Fig. 2 corresponds to . The primary photon number increases as is increased, but it can be considered that primary photons are still Poisson for even due to a very small output photon rate incident into the IIN. If and are assumed almost constant within each measurement macro pixel, from Eq. (18). Since the separately measured in this experimental setup is , and in Fig. 2(b), which indicates that of the cathode modulation is . We observed that measured values of are around for all conducted experiments as long as applied modulation voltages to the cathode of IIN and LD remain the same. The different values of indicate that the characteristics of gain modulation are slightly different, macro pixel by pixel. Measured , and to different MCP voltages are shown in Fig. 2(c), where and . The value indicates the validity of the experiment. Figure 2(c) shows that both and increase as the MCP voltage increases, although and are constant as in Fig. 2(b). This means that and in Eq. (18) dramatically increase as the MCP voltage (i.e., gain of the IIN) increases. From the other view, it is observed that the decreasing rates of both and are smaller for a lower MCP voltage, which indicates the mean terms contributing to variances in Eq. (18) are more dominant. It is also observed in Fig. 2(c) that the absolute difference between and is increased as the MCP voltage increases, which is caused by in of Eq. (18). Since the developed theory in Eq. (18) shows that affects not but , we measure the variation of variances with different peak-to-peak voltages () of the modulation signal applied to LD, which changes . As shown in Fig. 2(d), ’s are almost invariant to , but ’s are proportionally changed to . As shown in Fig. 2, experimental results show good agreement with the developed theory of Eq. (18).
Discussion and Conclusion
A noise factor, , is commonly used for the study of noise properties in photon amplifiers, such as ICCDs or IINs.28 Although the noise factor is defined for the case of non-modulation gain in photon amplifiers, it is worth making a relationship between and for applying to Eq. (18), which is19). Substituting Eq. (19) to Eq. (18) can express and , including . For example, becomes 20) is ignored assuming . It is reported that a for MCP outputs in an ICCD is inversely proportional to the MCP voltage.28 From the experimental results in Fig. 2 and Eq. (20), it can be conjectured that is dramatically increased as the MCP voltage increases even though a is decreased. A similar phenomenon is experimentally observed in other study, where is increased as a MCP voltage increases although is decreased.28 As another issue, characterizing the noise property of photon amplifiers by measuring a as a function of gain should be done carefully. As shown in Eq. (20), the for MCP output photons might be significantly different from the for amplifiers’ outputs depending on the amount of when is low.
The noise model of hetero/homodyne outputs is theoretically derived considering random amplification and multinomial selection. The noise characteristics determined from the developed theory are experimentally verified. Although this noise model is developed for hetero/homodyne measurements in this paper, it can be used for the case of non-modulation input beam and gain. Furthermore, it is reasonable to assume that the primary photons for most amplification processes are described by Poisson point process, as assumed in this paper. Therefore, the model in this paper can be applied to most photon-amplification processes including PMTs and Avalanche photodiodes (APDs) with or without gain modulation.
Some valuable properties are obtained from the developed noise model. The output is temporally uncorrelated, like shot noise, only if detector integration time for sampling is much longer than the decay time of phosphors in imaging intensifiers. For heterodyne measurements, the exposure time should be much less than the period of beat-frequency heterodyne output. Therefore, the heterodyne output is temporally uncorrelated for the specific range of the detector integration time. The amount of variance oscillates like the heterodyne and/or homodyne mean, so dc and ac variances can be considered separately. The dc variance indicates that the noise of the frequency-domain measurement output is amplified by the random amplification and gain modulation compared with the case of non-modulation gain. As the gain modulation deviates more from a perfect sinusoidal function, both dc and ac variances are increased. Another interesting point is that when both the gain of the image intensifier and the probability of detecting amplified photons from the image intensifier on a detector pixel are low, the variance approaches the mean—that is, the output photons are close to Poisson.
Hetero/homodyne measurements are widely used in frequency-domain diffusive imaging, so understanding the noise property of the frequency-domain outputs is beneficial in many ways. For example, it has recently been reported that estimated means of modulation amplitude and phase from noisy hetero/homodyne outputs are biased when the number of output photons is small.37 By adapting the expressions of mean and covariance developed in this paper, we have practically clarified the relationship between the bias and primary photon number. Furthermore, the developed noise model would be useful to precisely estimate modulation amplitude and phase using a maximum likelihood estimation method. As another example, the noise model in this paper could consolidate figures of merit for evaluating diffusive imaging performance, which is effective at optimizing frequency-domain diffusive imaging systems and helpful in developing new modalities of them. Finally, the performance of reconstruction algorithms can be enhanced with the appropriate noise model, so the theoretical results in this paper can be adapted to improve the quality of reconstructed images from frequency-domain tomographic diffusive imaging.
For the mean of Eq. (1), averaging for is21) is done by that is independent of . The averaging for the secondary simply replaces in Eq. (21) to , so 3), the averaging for secondary time produces 21) to (22), further averaging Eq. (23) with becomes 2) and (5) to Eq. (24) finalizes the calculation for the mean, as shown in Eq. (8).
The covariance can be calculated with the similar averaging procedure from Eqs. (21)(22)(23)(24)(25)–(26), but it should be considered in three separate cases. The autocorrelation of the point process of Eq. (1) is expressed as
Case 1: ,
The averaging over for the autocorrelation with the condition of case 1 is21). The superscript (1) indicates that averaging is performed for case 1. Further averaging Eq. (26) for , , and produces 2) and (5) to Eq. (27) derives 8)(9)–(10), only the dc and terms survive in Eq. (28). Therefore,
Case 2: ,
Considering a marginal probability law, averaging Eq. (25) over produces30) over . Further averaging for and becomes 2), (5), and (7), 6) is used for in Eq. (31).
Case 3: ,
Calculating the autocorrelation under this condition is so straightforward that the detailed mathematical procedure is not shown. Basically, after considering that there are terms for the summations for and , two point processes and can be independently calculated. Resulting from this consideration is the multiplication of two means of Eq. (24). Because the covariance , the result of for case 3 is canceled out with in . Therefore, is the same as Eq. (31), which is the same as Eq. (9).