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"Hagar" wrote in message
... "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/ The pictures there are lacking a legible measurement scale that would allow their interpretation as to actual variation magnitude. Take a look here instead: http://aether.lbl.gov/www/COBEimp.html Here's a brief quote: "There were variations in signal from the early Universe at a level of one part in 100,000." That's pretty small. |
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