TY - JOUR
T1 - Modelling the noise influence associated with the discrete linear canonical transform
AU - Bao, Yi Ping
AU - Li, Bing Zhao
N1 - Publisher Copyright:
© The Institution of Engineering and Technology 2018.
PY - 2018/8/1
Y1 - 2018/8/1
N2 - In this study, the properties of noise after a discrete linear canonical transform (DLCT) are analysed. First, the authors prove that the DLCT of noise can be modelled by a Gaussian distribution with very weak assumptions on the noise in the time domain. Then, the mean and covariance matrix of this Gaussian distribution is derived and the general trend of the noise after DLCT is described. In addition, they find that the properties of noise in the LCT domain are the generalisation of the properties of noise in the Fourier transform domain. What is more, the authors prove that the additive white Gaussian noise (AWGN) is still an AWGN after performing the DLCT. Finally, the simulations are performed to verify the effectiveness of the obtained results.
AB - In this study, the properties of noise after a discrete linear canonical transform (DLCT) are analysed. First, the authors prove that the DLCT of noise can be modelled by a Gaussian distribution with very weak assumptions on the noise in the time domain. Then, the mean and covariance matrix of this Gaussian distribution is derived and the general trend of the noise after DLCT is described. In addition, they find that the properties of noise in the LCT domain are the generalisation of the properties of noise in the Fourier transform domain. What is more, the authors prove that the additive white Gaussian noise (AWGN) is still an AWGN after performing the DLCT. Finally, the simulations are performed to verify the effectiveness of the obtained results.
UR - http://www.scopus.com/inward/record.url?scp=85051528750&partnerID=8YFLogxK
U2 - 10.1049/iet-spr.2017.0319
DO - 10.1049/iet-spr.2017.0319
M3 - Article
AN - SCOPUS:85051528750
SN - 1751-9675
VL - 12
SP - 756
EP - 760
JO - IET Signal Processing
JF - IET Signal Processing
IS - 6
ER -