'Nyquist criterion' presentation slideshows

Kazuhiro Yamamoto Institute for Cosmics Ray Reseach, the University of Tokyo

Thermal noise History from Brownian motion until interferometer. Kazuhiro Yamamoto Institute for Cosmics Ray Reseach, the University of Tokyo . Advanced Interferometer Configuration lecture 6 September 2011 @Institute for Cosmic Ray Research, Kashiwa, Japan. References. Peter R. Saulson,

1.28k views • 113 slides

Chapter 8 Frequency-Domain Analysis

Chapter 8 Frequency-Domain Analysis. Automatic Control Systems, 9 th Edition F. Golnaraghi & B. C. Kuo. 1, p. 409. 8-1 Introduction. For a LTI system: input -- ? steady-state output -- Sinusoidal steady-state analysis :. s = j ?. M ( s ). 1, p. 410. Frequency Response.

3.53k views • 80 slides

Stability from Nyquist plot

1.48k views • 37 slides

Communications Part II

4. Optimal Receiver for AGN Optimal AWGN Receiver Generalization for coloured noise Symbol / Bit Error Probability 5. Equalization Linear Equalization Decision Feedback Adaptive Equalization Optimal Receiver for ISI Conditions Forney-Receiver (MLSE) Viterbi-Algorithm.

507 views • 31 slides