KIZIMEN VOLCANO, KAMCHATKA — A FUTURE MOUNT ST. HELENS?

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dc.contributor.author Melekestsev I.V. en
dc.contributor.author Ponomareva V.V. en
dc.contributor.author Volynets O.N. en
dc.date.accessioned 2019-03-04T03:58:41Z
dc.date.available 2019-03-04T03:58:41Z
dc.date.issued 1995
dc.identifier.citation Journal of Volcanology and Geothermal Research 65 (1995) 205-226 en
dc.identifier.uri https://repository.geologyscience.ru/handle/123456789/446
dc.description.abstract We studied the tectonic setting, morphology, geologic structure, history of eruptive activity and evolution of the composition of the erupted material of Kizimen volcano, Kamchatka, from the moment of its origination 11–12 thousand years ago to the present time. Four cycles, each 2–3.5 thousand years long, were distinguished that characterize the activity of the volcano. All of the largest eruptions were dated, and their parameters determined. We also estimated the volume and the mass of the erupted products, the volcanic intensity of eruption of material during periods of high activity, and the amount of material the volcano ejected at different stages of its formation. It has been shown that the evolution of the composition of the rocks erupted (from dacite to basaltic andesite) takes place as a result of mixing of dacitic and basaltic magma. It is suggested that future eruptions that may take place at Kizimen may be similar to those at Bandai (1888) and Mount St. Helens (1980) volcanoes. ru_RU
dc.language Английский ru_RU
dc.relation.ispartof JOURNAL OF VOLCANOLOGY AND GEOTHERMAL RESEARCH ru_RU
dc.subject 38.37.25 Вулканология ru_RU
dc.subject Кизимен ru_RU
dc.title KIZIMEN VOLCANO, KAMCHATKA — A FUTURE MOUNT ST. HELENS? en
dc.type Статья, тезисы доклада ru_RU


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