The cosmic microwave background radiation is an emission of uniform, black body thermal energy coming from all parts of the sky. The root mean square variations are only 18 μk, after subtracting out a dipole anisotropy from the doppler shift of the background radiation. The latter is caused by the peculiar velocity of the … The radiation is isotropic to roughly one part in 100,000:
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The cosmic microwave background radiation is an emission of uniform, black body thermal energy coming from all parts of the sky.
The cosmic microwave background radiation is an emission of uniform, black body thermal energy coming from all parts of the sky. The radiation is isotropic to roughly one part in 100,000: The root mean square variations are only 18 μk, after subtracting out a dipole anisotropy from the doppler shift of the background radiation. The latter is caused by the peculiar velocity of the …
The latter is caused by the peculiar velocity of the … The cosmic microwave background radiation is an emission of uniform, black body thermal energy coming from all parts of the sky. The root mean square variations are only 18 μk, after subtracting out a dipole anisotropy from the doppler shift of the background radiation. The radiation is isotropic to roughly one part in 100,000:
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The latter is caused by the peculiar velocity of the …
The cosmic microwave background radiation is an emission of uniform, black body thermal energy coming from all parts of the sky. The latter is caused by the peculiar velocity of the … The root mean square variations are only 18 μk, after subtracting out a dipole anisotropy from the doppler shift of the background radiation. The radiation is isotropic to roughly one part in 100,000:
The latter is caused by the peculiar velocity of the … The radiation is isotropic to roughly one part in 100,000: The root mean square variations are only 18 μk, after subtracting out a dipole anisotropy from the doppler shift of the background radiation. The cosmic microwave background radiation is an emission of uniform, black body thermal energy coming from all parts of the sky.
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The cosmic microwave background radiation is an emission of uniform, black body thermal energy coming from all parts of the sky.
The latter is caused by the peculiar velocity of the … The cosmic microwave background radiation is an emission of uniform, black body thermal energy coming from all parts of the sky. The root mean square variations are only 18 μk, after subtracting out a dipole anisotropy from the doppler shift of the background radiation. The radiation is isotropic to roughly one part in 100,000:
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