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Studio delle prestazioni di un sistema a fosfori per mammografia ...

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where � � and � � are the image <strong>di</strong>mensions. The integration can be extended to the entire<br />

plane if we consider Ò �� � � outside the image. Due to the Parseval theorem [13], the<br />

same relation is valid in the spatial frequency domain for the Fourier components �Ò ����� of<br />

Ò �� � :<br />

� � Ð�Ñ<br />

��� �� � � � � �<br />

�<br />

�<br />

��Ò ����� � ������ (2.31)<br />

Starting from Eq. 2.31, the noise spectral density Ï ����� is defined as:<br />

Ï ����� � Ð�Ñ<br />

��� � � � � � � � ��Ò ����� � (2.32)<br />

Finally, in order to take into acco<strong>un</strong>t the fact that the process statistics can depend on multiple<br />

realizations, the average of the noise spectral density is computed over a large ensemble of<br />

realizations, thus obtaining the Noise Power Spectrum (NPS):<br />

ÆÈË ����� � Ð�Ñ<br />

��� � � �<br />

� �� � � ��Ò ����� � � (2.33)<br />

The NPS (or Wiener spectrum) describes the variance in amplitude of each frequency com-<br />

ponent of a system.<br />

2.4 DQE<br />

The Detective Quantum Efficiency DQE is a physical quantity that takes into acco<strong>un</strong>t the imag-<br />

ing system <strong>per</strong>formances both from the noise and from the spatial resolution point of view. In<br />

order to <strong>un</strong>derstand the <strong>un</strong>derlying reasons that lead to the definition of the o<strong>per</strong>ative DQE def-<br />

inition, let us consider the expected value �� ℄and the variance Î �℄of an image signal. Given<br />

the relation � between input and output we obtain the system characteristic curve in absence<br />

of noise:<br />

��ÇÍÌ ℄�� ��ÁÆ℄ (2.34)<br />

The noise can be added as a term Æ�, with a zero expectation value ��Æ�℄ � , such that the<br />

output is:<br />

ÇÍÌ � � ÁÆ Æ� (2.35)<br />

27

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