A MODEL FOR THE ORIGIN OF LARGE SILICIC MAGMA CHAMBERS: PRECURSORS OF CALDERA-FORMING ERUPTIONS
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dc.contributor.author | Jellinek A.M. | |
dc.contributor.author | DePaolo D.J. | |
dc.date.accessioned | 2021-11-23T00:58:48Z | |
dc.date.available | 2021-11-23T00:58:48Z | |
dc.date.issued | 2003 | |
dc.identifier | https://www.elibrary.ru/item.asp?id=13678859 | |
dc.identifier.citation | Bulletin of Volcanology, 2003, 65, 5, 363-381 | |
dc.identifier.issn | 0258-8900 | |
dc.identifier.uri | https://repository.geologyscience.ru/handle/123456789/32421 | |
dc.description.abstract | The relatively low rates of magma production in island arcs and continental extensional settings require that the volume of silicic magma involved in large catastrophic caldera-forming (CCF) eruptions must accumulate over periods of 10^5 to 10^6 years. We address the question of why buoyant and otherwise eruptible high-silica magma should accumulate for long times in shallow chambers rather than erupt more continuously as magma is supplied from greater depths. Our hypothesis is that the viscoelastic behavior of magma chamber wall rocks may prevent an accumulation of overpressure sufficient to generate rhyolite dikes that can propagate to the surface and cause an eruption. The critical overpressure required for eruption is based on the model of Rubin (1995a). An approximate analytical model is used to evaluate the controls on magma overpressure for a continuously or episodically replenished spherical magma chamber contained in wall rocks with a Maxwell viscoelastic rheology. The governing parameters are | |
dc.subject | Dike Formation | |
dc.subject | Viscoelastic Rocks | |
dc.subject | Rhyolitic Volcanism | |
dc.subject | Granitic Plutons | |
dc.subject | Silicic Magma | |
dc.subject | Chumber Evolution | |
dc.title | A MODEL FOR THE ORIGIN OF LARGE SILICIC MAGMA CHAMBERS: PRECURSORS OF CALDERA-FORMING ERUPTIONS | |
dc.type | Статья |
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