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Noise poissonian

Owing to the constraints, no direct solution exists and we must use iterative methods to obtain the solution. It is possible to use bound constrained version of optimization algorithms such as conjugate gradients or limited memory variable metric methods (Schwartz and Polak, 1997 Thiebaut, 2002) but multiplicative methods have also been derived to enforce non-negativity and deserve particular mention because they are widely used RLA (Richardson, 1972 Lucy, 1974) for Poissonian noise and ISRA (Daube-Witherspoon and Muehllehner, 1986) for Gaussian noise. [Pg.405]

If the exact statistics of the noise is unknown, assuming stationary Gaussian noise is however more robust than Poissonian (Lane, 1996). [Pg.408]

For better comparison of theoretical predictions for different-order processes, we have plotted the quantum Fano factors for both interacting modes in the no-energy-transfer regime with N = 2 — 5 and r = 5 in Fig. 7. One can see that all curves start from F w(0) = 1 for the input coherent fields and become quasistationary after some relaxations. The quantum and semiclassical Fano factors coincide for high-intensity fields and longer times, specifically for t > 50/(Og), where il will be defined later by Eq. (54). In Fig. 17, we observe that all fundamental modes remain super-Poissonian [F (t) >1], whereas the iVth harmonics become sub-Poissonian (F (t) < 1). The most suppressed noise is observed for the third harmonic with the Fano factor 0.81. In Fig. 7, we have included the predictions of the classical trajectory method (plotted by dotted lines) to show that they properly fit the exact quantum results (full curves) for the evolution times t > 50/(Og). The small residual differences result from the fact that the amplitude r was chosen to be relatively small (r = 5). This value does not precisely fulfill the condition r> 1. We have taken r = 5 as a compromise between the asymptotic value r oo and computational complexity to manipulate the matrices of dimensions 1000 x 1000. Unfortunately, we cannot increase amplitude r arbitrary due to computational limitations. [Pg.508]

We have proved that in the no-energy-transfer regime, the fundamental mode evolves into a quasistationary state with the super-Poissonian (Ff >1) photocount statistics, whereas the Mh harmonic goes over into a sub-Poissonian (Fx < 1) quasistationary state. We have found that the most suppressed photocount noise is obtained for the third harmonic as described by the quantum Fano... [Pg.515]

If we assume a constant fluorescence rate, the noise is determined by Poissonian counting statistics. Then, the highest S/N level that can be achieved [32] is... [Pg.8]

The secondary emission coefficient at a particular dynode depends on the dynode material and energy of the primary electrons. For typical interdynode voltages used in PMTs, the secondary emission coefficient, n, is between 4 and 10. Because the secondary emission is a random process the number of the generated secondary electrons varies from electron to electron. The width of the distribution can be expected at least of the size of the standard deviation, n, of a poissonian distribution of the secondary emission coefficient, n. Therefore the single-photon pulses obtained from a PMT have a considerable amplitude jitter. For TCSPC applications it is important that the pulse amplitudes of the majority of the pulses are well above the unavoidable noise background. [Pg.226]

Since white noise is qualified by a single parameter, namely by its intensity, the characterisation of real noise requires at least another parameter, its correlation time. The theoretical treatment of nonlinear systems subject to real, i.e. coloured , external noise has two newer difficulties. First, only the white noise idealisation leads to a Markov process. Second, from the practical point of view the Gaussian and Poissonian distributions are relevant only to describe white noise, and real noise can have a richer description. The disadvantage due to the loss of Markov property is partially compensated by the fact that non-Markovian processes have smoother realisations than Markov processes. Therefore no particular (Ito or Strato-... [Pg.151]

H. Ritsch, M. A. M. Marte. Quantum noise in Raman lasers Effects of pump bandwidth and super- and sub-Poissonian pumping. Physical Revew A 1993 Mar 47(6) 2354 - 2365... [Pg.96]

Another way to analyze the prepitting noise is to calculate the power spectral density (PSD) associated with the anodic current fluctuations. Let us consider a Poissonian series of birth and death events (birth frequency X, death frequency p), with a parabolic growth law between birth and death. This situation can be modeled as follows ... [Pg.440]


See other pages where Noise poissonian is mentioned: [Pg.227]    [Pg.125]    [Pg.127]    [Pg.74]    [Pg.14]    [Pg.495]    [Pg.495]    [Pg.508]    [Pg.514]    [Pg.515]    [Pg.563]    [Pg.565]    [Pg.151]    [Pg.165]    [Pg.296]    [Pg.20]    [Pg.67]    [Pg.84]    [Pg.84]    [Pg.93]    [Pg.130]    [Pg.124]    [Pg.230]   
See also in sourсe #XX -- [ Pg.307 ]




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