I've been rather active in following commissioning of the James Webb
Space telescope, in its optical near infrared and middle infrared
wavelenghts.
Why don't we do everything alike in audio? In particular, why don't we
do audio range coronagraphy, in order to separate the Loud from the
Feeble? Also, why don't we do physical, spatial modulation even on the
projection side, backwards? Because the huge constrast *does* go both
ways.
--
Sampo Syreeni, aka decoy - de...@iki.fi, http://decoy.iki.fi/front
+358-40-3751464, 025E D175 ABE5 027C 9494 EEB0 E090 8BA9 0509 85C2
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