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Find link is a tool written by Edward Betts.searching for Dipole anisotropy 14 found (17 total)
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Cosmic microwave background
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mean square variations are just over 100 μK, after subtracting a dipole anisotropy from the Doppler shift of the background radiation. The latter isList of unsolved problems in physics (11,344 words) [view diff] exact match in snippet view article find links to article
cosmological principle an invalid assumption? The number count and intensity dipole anisotropy in radio, NRAO VLA Sky Survey (NVSS) catalogue is inconsistent withSolar apex (907 words) [view diff] case mismatch in snippet view article find links to article
4.1023. See also Table 3 on page 13 of Kogut, A.; et al. (1993). "Dipole Anisotropy in the COBE Differential Microwave Radiometers First-Year Sky Maps"Galactic coordinate system (1,380 words) [view diff] case mismatch in snippet view article find links to article
30–31. ISBN 0-691-02565-7. For example in Kogut, A.; et al. (1993). "Dipole Anisotropy in the COBE Differential Microwave Radiometers First-Year Sky Maps"Motion (3,793 words) [view diff] case mismatch in snippet view article find links to article
; Tenorio, L.; Weiss, R.; Wilkinson, D.T.; Wright, E.L. (1993). "Dipole Anisotropy in the COBE Differential Microwave Radiometers First-Year Sky Maps"Cosmological principle (3,744 words) [view diff] exact match in snippet view article find links to article
homogeneous universe. The largest scale feature of the CMB is the dipole anisotropy; it is typically subtracted from maps due to its large amplitude.Steady-state model (3,543 words) [view diff] exact match in snippet view article find links to article
Already in 1967, Dennis Sciama predicted that the CMB has a significant dipole anisotropy. In recent years the CMB dipole has been tested and current resultsCMB cold spot (2,717 words) [view diff] exact match in snippet view article find links to article
Wall Void (astronomy) Wilkinson Microwave Anisotropy Probe After the dipole anisotropy, which is due to the Doppler shift of the microwave background radiationExtragalactic cosmic ray (4,016 words) [view diff] exact match in snippet view article find links to article
Pierre Auger Observatory's most notable results is the detection of a dipole anisotropy in the arrival directions of cosmic rays with energy greater thanDark energy (9,657 words) [view diff] case mismatch in snippet view article find links to article
the Universe Accelerating? All Signs Still Point to Yes: A Local Dipole Anisotropy Cannot Explain Dark Energy". The Astrophysical Journal. 894 (1): 68Black-body radiation (8,651 words) [view diff] exact match in snippet view article find links to article
found in the cosmic microwave background radiation, which exhibits a dipole anisotropy from the Earth's motion relative to this blackbody radiation fieldMilky Way (21,677 words) [view diff] exact match in snippet view article find links to article
1088/1674-4527/20/10/159. S2CID 229005996. Kogut, Alan; et al. (December 10, 1993). "Dipole anisotropy in the COBE differential microwave radiometers first-year sky maps"Sun (18,120 words) [view diff] case mismatch in snippet view article find links to article
Touchstone. ISBN 9780671766061. Table 3 of Kogut, A.; et al. (1993). "Dipole Anisotropy in the COBE Differential Microwave Radiometers First-Year Sky Maps"Lambda-CDM model (11,049 words) [view diff] exact match in snippet view article find links to article
predicted that the cosmic microwave background has a significant dipole anisotropy. In recent years, the CMB dipole has been tested, and the results