Titlebook: Current Topics in Astrofundamental Physics; The Early Universe N. Sánchez,A. Zichichi Book 1995 Springer Science+Business Media Dordrecht 1

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Cosmic Microwave Background Anisotropy Large Angular Scales / Cobe DMR Resultssts of various ideas of large scale structure formation. CMB observations now let us test the role of gravity and General Relativity in cosmology including the geometry, topology, and dynamics of the Universe. Foreground galactic emissions, dust thermal emission and emission from energetic electrons

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Detections of Primary and Secondary Anisotropies in the CMBthe three CMB programmes currently underway at MRAO Cambridge. Results are presented from the Tenerife experiments observing on ~ 5° scales at frequencies of 10, 15 and 33 GHz. The best scan attains a sensitivity ~20μK and clear features are present with the properties expected for CMB anisotropy. O

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