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Titlebook: Non-linear Data Analysis on the Sphere; The Quest for Anomal Gregor Rossmanith Book 2013 Springer International Publishing Switzerland 2013

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11#
發(fā)表于 2025-3-23 09:55:11 | 只看該作者
12#
發(fā)表于 2025-3-23 16:32:07 | 只看該作者
13#
發(fā)表于 2025-3-23 22:00:52 | 只看該作者
Observations of the CMB with the WMAP Satellite,tion of its temperature was done by Ralph Alpher and Robert Herman in 1950. The discovery of the radiation by Arno Penzias and Robert Wilson in 1965 represents a milestone in the history of Cosmology. The first measurement with a full-sky coverage was realised with the satellite . (COBE) that was la
14#
發(fā)表于 2025-3-24 00:28:25 | 只看該作者
Scaling Indices Applied to the WMAP 5-Year Data,method on the single Q-, V-, W-bands and the co-added VW-band of the 5-year data of the .. We compare each of the results with 1000 Monte Carlo simulations mimicking the Gaussian properties of the best fit .-model. Based on the scaling indices, scale-dependent empirical probability distributions, mo
15#
發(fā)表于 2025-3-24 06:15:49 | 只看該作者
Surrogates and Scaling Indices Applied to the WMAP 7-Year Data, surrogate data sets are generated, in which the power spectrum of the original data is preserved, while the higher order correlations are partly randomised by applying a scale-dependent shuffling procedure to the Fourier phases. We apply this method to the WMAP data of the cosmic microwave backgrou
16#
發(fā)表于 2025-3-24 08:52:31 | 只看該作者
17#
發(fā)表于 2025-3-24 12:50:02 | 只看該作者
18#
發(fā)表于 2025-3-24 17:46:39 | 只看該作者
19#
發(fā)表于 2025-3-24 19:11:27 | 只看該作者
Methods for Testing the Non-Gaussianity of the CMB,ons. Besides, any analysis resulting in a non-detection of anomalous behaviour does not prove the CMB to be Gaussian, but just rules out a single type of non-Gaussianity corresponding to the characteristics of the analysis.
20#
發(fā)表于 2025-3-25 00:10:35 | 只看該作者
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