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zonde
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This article http://www.physorg.com/news/2011-06-big-edge-solar.html" tells about discovery of magnetic bubbles at the edge of solar system.
As I understand they are around 100AU from Sun and around the size of 1AU. That makes them roughly 3.6° angular size.
Shouldn't these bubbles cause some effect in CMB?
If they do then the effect should be discernible as it would undergo rather detectable paralax.
As I understand they are around 100AU from Sun and around the size of 1AU. That makes them roughly 3.6° angular size.
Shouldn't these bubbles cause some effect in CMB?
If they do then the effect should be discernible as it would undergo rather detectable paralax.
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