LEADER 02731nam 2200625Ia 450 001 9910145704703321 005 20170809164429.0 010 $a1-281-32298-9 010 $a9786611322984 010 $a0-470-70050-5 010 $a0-470-75467-2 010 $a0-470-75459-1 035 $a(CKB)1000000000414264 035 $a(EBL)351595 035 $a(OCoLC)437218818 035 $a(SSID)ssj0000234664 035 $a(PQKBManifestationID)11195087 035 $a(PQKBTitleCode)TC0000234664 035 $a(PQKBWorkID)10241346 035 $a(PQKB)11492756 035 $a(MiAaPQ)EBC351595 035 $a(MiAaPQ)EBC7076276 035 $a(Au-PeEL)EBL7076276 035 $a(EXLCZ)991000000000414264 100 $a20010605d2002 uy 0 101 0 $aeng 135 $aur|n|---||||| 181 $ctxt 182 $cc 183 $acr 200 14$aThe Reformation in Germany$b[electronic resource] /$fC. Scott Dixon 210 $aOxford ;$aMalden, Mass. $cBlackwell Publishers$d2002 215 $a1 online resource (241 p.) 225 1 $aHistorical Association studies 300 $aDescription based upon print version of record. 311 $a0-631-20253-6 311 $a0-631-20252-8 320 $aIncludes bibliographical references (p. [191]-205) and index. 327 $aThe Reformation in Germany; Contents; Preface; Chronologies; Political Chronology of the Reformation in the Holy Roman Empire (1521-1555); The Indulgences Dispute, 1514-1518; The Broadening Lutheran Confiict, 1518-1519; Luther's Excommunication, 1520-1521; 1 Germany on the Eve of Reformation; 2 Religious Culture and the Reformation; The Luther Affair; The German Church; Reformation Thought; 3 The Reformation in the Parishes; Spreading the Word; The Rural Reformation and the Peasants' War; The Theology of Revolution; 4 Political Culture and the German Reformation; The Urban Reformation 327 $aThe Princely ReformationThe Politics of Religious Change; 5 The Reformation Legacy; The Growth of Confessions; The Protestant State; Protestant Culture; 6 Reformation Histories; Bibliography; Index 330 $aThe Reformation Movement in Germany provides readers with a strong narrative overview of the most recent work on the Reformation in the German lands. 410 0$aHistorical Association studies. 606 $aReformation$zGermany 607 $aGermany$xChurch history$y16th century 608 $aElectronic books. 615 0$aReformation 676 $a274.306 700 $aDixon$b C. Scott$0918227 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910145704703321 996 $aThe Reformation in Germany$92058862 997 $aUNINA LEADER 02898nam 2200493 450 001 9910830874003321 005 20240124103428.0 010 $a1-119-81560-6 010 $a1-119-81547-9 010 $a1-119-81548-7 035 $a(PPN)275119939 035 $a(CKB)4940000000599451 035 $a(MiAaPQ)EBC6561798 035 $a(Au-PeEL)EBL6561798 035 $a(OCoLC)1247664424 035 $a(EXLCZ)994940000000599451 100 $a20211120d2021 uy 0 101 0 $aeng 135 $aurcnu|||||||| 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 00$aSolar physics and solar wind /$fNour E. Raouafi [and three others], editors 210 1$aHoboken, NJ :$cWiley,$d2021. 215 $a1 online resource (323 pages) 225 1 $aGeophysical monograph ;$v258 225 1 $aSpace physics and aeronomy collection ;$vVolume 1 300 $aIncludes index. 311 $a1-119-50753-7 330 $a"One of the current mysteries in Heliophysics is the heating of the solar atmosphere to temperatures that are orders of macagnitude hotter than the solar surface. As a result of this heating, the Sun cannot contain its atmosphere and a continual outflow of plasma streams out from the solar corona to interplanetary space and beyond. For the debate surrounding the exact physical mechanisms of the heating of the corona, we direct the reader to Chapter 6. We here discuss physical mechanisms behind the formation and propagation of the solar wind. The whole volume of space influenced by the solar wind is called the 'Heliosphere' and its size is in part modulated by the solar wind ram pressure. The solar wind extends from the corona to well beyond a hundred astronomical units (AU) to a termination shock. Beyond that shock, the solar wind slows down abruptly in response to the pressure of the interstellar medium, the plasma becomes compressed and more turbulent until it reaches a zone where it can no longer push back the interstellar plasma. In-situ measurements of these outer regions are sparse and our exploration of this boundary layer has only just begun with the Voyager spacecraft. In particular the global shape of the Heliosphere is still not known because the Voyager spacecraft have only measured a very small region of the heliospheric boundary. We direct the reader to Chapter 9 for more detailed information on fascinating region of the Heliosphere"--$cProvided by publisher. 410 0$aGeophysical monograph ;$v258. 410 0$aSpace physics and aeronomy collection ;$vVolume 1. 606 $aSolar wind 607 $aSun 615 0$aSolar wind. 676 $a523.58 702 $aRaouafi$b Nour E. 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910830874003321 996 $aSolar physics and solar wind$94063843 997 $aUNINA