"Greg Neill" wrote in message
...
"Hagar" wrote in message
...


COBE determined that the background radiation is indeed NOT uniform, but
rather blotchy. Even though that difference is measured in fractions of
a
degree K, nonetheless it matches the "clumpiness" of galaxy cluster
distribution throughout the observable universe.

Maybe you should revisit the figures. What's the magnitude
of the "blotchiness"? I think you'll find that the background
is remarkably uniform, and that the deviations are very, very
tiny in temperature.

"Blotchy" picture link attached:
http://aether.lbl.gov/www/projects/cobe/