LEADER 04112nam 22005055 450 001 9910257410003321 005 20200630083512.0 010 $a3-540-48328-4 024 7 $a10.1007/3-540-57755-6 035 $a(CKB)1000000000234082 035 $a(DE-He213)978-3-540-48328-1 035 $a(PPN)155210920 035 $a(EXLCZ)991000000000234082 100 $a20121227d1994 u| 0 101 0 $aeng 135 $aurnn|008mamaa 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 10$aPresent and Future of the Cosmic Microwave Background$b[electronic resource] $eProceedings of the Workshop Held in Santander, Spain, 28 June ? 1 July 1993 /$fedited by Jose L. Sanz, Enrique Martinez-Gonzalez, Laura Cayon 205 $a1st ed. 1994. 210 1$aBerlin, Heidelberg :$cSpringer Berlin Heidelberg :$cImprint: Springer,$d1994. 215 $a1 online resource (VIII, 236 p. 9 illus.) 225 1 $aLecture Notes in Physics,$x0075-8450 ;$v429 311 $a3-540-57755-6 327 $aThe CMB spectrum at centimeter wavelengths -- Recent measurements of the Sunyaev-Zel'dovich effect -- Clusters and the cosmic microwave background -- Theoretical aspects of the CMB spectrum -- Medium scale CBR anisotropy measurements: UCSB South Pole HEMT (1990?91) and MAX 3 (1991) -- Results from the cosmic background explorer -- The MSAM/TopHat program for measuring the CMBR anisotropy -- The current status of the tenerife experiments and prospects for the future. -- Making maps with the tenerife data -- Anisotropy of the relic radiation in relict-1 experiment and parameters of grand unification -- RELIKT1 and COBS-DMR results: A comparison -- Comments on the COBE 1 DMR quadrupole estimation -- Pip analysis of the Tenerife and ULISSE data -- Telling adiabatic perturbations from gravitational waves and the CMB polarization -- Imprints of galaxy clustering evolution on the CMB -- Analysis of texture on cosmic background maps -- Sakharov modulation of the spectrum of initial perturbations and its manifestation in the anisotropy of cosmic microwave background and galaxy correlation function -- Constraints on models from POTENT and CMB anisotropies -- Reionization and the cosmic microwave background -- Possible reionization and first structures in CDM -- CMB anisotropies in the reionized universe -- Microwave background anisotropies: Future plans -- New constraints on reionization from the Compton y-parameter -- Future projects on the Cosmic Microwave Background -- The COBRAS mission. 330 $aThese review articles by outstanding specialists cover the present status ofthe observations of the spectrum and of the anisotropies of the cosmic microwave background radiation. Experimental developments, data analysis and related theoretical aspects are also treated. The idea is to review and discuss at a level accessible to non-specialised astronomers and graduate students the most recent developments in this field as well as the future perspectives for astrophysics and cosmology in particular. 410 0$aLecture Notes in Physics,$x0075-8450 ;$v429 606 $aSpace sciences 606 $aGeophysics 606 $aSpace Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics)$3https://scigraph.springernature.com/ontologies/product-market-codes/P22030 606 $aGeophysics/Geodesy$3https://scigraph.springernature.com/ontologies/product-market-codes/G18009 615 0$aSpace sciences. 615 0$aGeophysics. 615 14$aSpace Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics). 615 24$aGeophysics/Geodesy. 676 $a520 676 $a500.5 702 $aSanz$b Jose L$4edt$4http://id.loc.gov/vocabulary/relators/edt 702 $aMartinez-Gonzalez$b Enrique$4edt$4http://id.loc.gov/vocabulary/relators/edt 702 $aCayon$b Laura$4edt$4http://id.loc.gov/vocabulary/relators/edt 906 $aBOOK 912 $a9910257410003321 996 $aPresent and Future of the Cosmic Microwave Background$92498492 997 $aUNINA