From: Dr. H. Paul Shuch (n6tx_at_setileague.org)
Date: Fri Feb 28 2003 - 06:57:25 PST
At 09:27 AM 2/28/03 -0500, Bill St. Arnaud wrote:
>But I am suggesting that we use the CBR spectrume profile as the
>de-spreading function?
>Alternatively is there a psuedo noise code that will generate a CBR like
>spectrum around a given
>carrier frequency ?
I could be mistaken, but I thought the CBR was thermal blackbody
radiation. If so, it should be distributed as a Poisson around the 3
kelvin mean. This gives us the distribution, but not the sequence (and for
direct sequence spread spectrum, we need both).
-----------------------------------------------------------------
H. Paul Shuch, Ph.D. Executive Director, The SETI League, Inc.
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