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AWGN, Colored Noise, Modulation, Thermal Asperities, Disk Defects, etc.
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There’s more affecting your system than additive white gaussian noise. Does it matter if the signal into the Viterbi algorithm is clipped? What does a thermal asperity look like in the frequency-domain? The answers are easy to find with PRMLpro™'s noise and distortion screen.
Generate complex distortion profiles easily for studying the extreme performance bounds of your servo and data recovery systems. Experiment with off-track interference, disk defects, correlated noise and more.
Please contact us for a free initial consultation.
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For more information:
ChannelScience
7300 Cody Court
Plano, TX 75024-3837 US
Email: connect@channelscience.com
© Copyright 2009 ChannelScience. All Rights Reserved.
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