. . . "978"^^ . "Part III: Effusive Volcanism"@cs . . "efuzivn\u00EDho vulkanismu"@cs . "efuziva"@cs . "v\u00FDlev"@cs . . . "efusiv"@cs . "Academic Press"@cs . . "v\u00FDlevn\u00FD vulkanismus"@cs . . "V\u00FDlevn\u00FD vulkanismus"@cs . "V\u00FDlevn\u00FD vulkanismus nebo efuzivn\u00ED vulkanismus je typ sope\u010Dn\u00E9 erupce, p\u0159i kter\u00E9 l\u00E1va pouze voln\u011B vyt\u00E9k\u00E1 z trhliny (na rozd\u00EDl od exploz\u00EDvn\u00ED erupce). L\u00E1va m\u00E1 n\u00EDzkou viskozitu a tedy velkou tekutost. P\u0159\u00EDkladem takov\u00E9to l\u00E1vy je l\u00E1va Pahoe-hoe s mal\u00FDm obsahem SiO2, kter\u00E1 m\u016F\u017Ee urazit n\u011Bkolik kilometr\u016F l\u00E1vov\u00FDmi kan\u00E1ly \u010Di po povrchu ne\u017E se ochlad\u00ED a ztuhne. Tento typ vulkanismu je charakteristick\u00FD pro \u0161t\u00EDtov\u00E9 sopky. N\u011Bkdy l\u00E1va nevyt\u00E9k\u00E1 z kr\u00E1teru sopky, ale z tektonick\u00E9ho zlomu a vytv\u00E1\u0159\u00ED l\u00E1vovou tabuli, kter\u00E1 m\u016F\u017Ee m\u00EDt tlou\u0161\u0165ku a\u017E n\u011Bkolik kilometr\u016F. Nebezpe\u010D\u00ED v\u00FDlevn\u00E9ho vulkanismu spo\u010D\u00EDv\u00E1 v tom, \u017Ee l\u00E1va b\u011Bhem v\u00FDlevu zas\u00E1hne velk\u00E9 oblasti, ve kter\u00FDch doch\u00E1z\u00ED ke vzniku l\u00E1vov\u00FDch jezer, \u010Di se m\u016F\u017Ee rychle p\u0159em\u00EDstit do oblasti pom\u011Brn\u011B vzd\u00E1len\u00FDch od m\u00EDsta erupce.L\u00E1vov\u00E9 tabule se nach\u00E1zej\u00ED na Zemi na Islandu, v oblast\u00ED Snake River Plain v Idahu, v Columbia River Plain ve st\u00E1t\u011B Washington a ve v\u00FDchodn\u00EDm Oregonu. K v\u00FDlevn\u00E9mu vulkanismu doch\u00E1z\u00ED nap\u0159. v oblasti Havajsk\u00FDch ostrov\u016F (sopky Kilauea, Mauna Loa). Mimo Zemi jsou zn\u00E1m\u00E9 \u0161t\u00EDtov\u00E9 sopky na Venu\u0161i (Sif Mons) \u010Di Marsu (Ascraeus Mons, Arsia Mons, Olympus Mons \u2013 nejv\u011Bt\u0161\u00ED \u0161t\u00EDtov\u00E1 sopka a hora v jednom v cel\u00E9 slune\u010Dn\u00ED soustav\u011B). V minulosti doch\u00E1zelo k v\u00FDlevn\u00E9mu vulkanismu tak\u00E9 na M\u011Bs\u00EDci a vznikla tak m\u011Bs\u00ED\u010Dn\u00ED mo\u0159e, \u010Di na povrchu Merkuru."@cs . . "523086"^^ . "26"^^ . "v\u00FDlevn\u00E1"@cs . . . . "283"^^ . "v\u00FDlevy"@cs . . "v\u00FDlevn\u00FDch"@cs . "v\u00FDlevn\u00E9"@cs . . "Haraldur a kolektiv"@cs . . . . . . . . "v\u00FDlevn\u00E9ho \u010Dedi\u010De"@cs . "13134123"^^ . "Sigurdsson"@cs . "Encyclopedia of Volcanoes"@cs . "l\u00E1vov\u00FDm v\u00FDlev\u016Fm"@cs . . . . "1999"^^ . . "V\u00FDlevn\u00FD vulkanismus nebo efuzivn\u00ED vulkanismus je typ sope\u010Dn\u00E9 erupce, p\u0159i kter\u00E9 l\u00E1va pouze voln\u011B vyt\u00E9k\u00E1 z trhliny (na rozd\u00EDl od exploz\u00EDvn\u00ED erupce). L\u00E1va m\u00E1 n\u00EDzkou viskozitu a tedy velkou tekutost. P\u0159\u00EDkladem takov\u00E9to l\u00E1vy je l\u00E1va Pahoe-hoe s mal\u00FDm obsahem SiO2, kter\u00E1 m\u016F\u017Ee urazit n\u011Bkolik kilometr\u016F l\u00E1vov\u00FDmi kan\u00E1ly \u010Di po povrchu ne\u017E se ochlad\u00ED a ztuhne. Tento typ vulkanismu je charakteristick\u00FD pro \u0161t\u00EDtov\u00E9 sopky."@cs . "v\u00FDlevu"@cs . "v\u00FDlevn\u00E9ho vulkanismu"@cs . . . "efuzivn\u00EDho"@cs . "anglicky"@cs . "2982"^^ . . . . "v\u00FDlevn\u00FD"@cs . . . . .