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Effects of the crater on eruption column dynamics
https://nied-repo.bosai.go.jp/records/4526
https://nied-repo.bosai.go.jp/records/4526f508d304-d20f-4076-9226-f398072a3101
Item type | researchmap(1) | |||||||||||||||||
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公開日 | 2023-04-27 | |||||||||||||||||
タイトル | ||||||||||||||||||
言語 | ja | |||||||||||||||||
タイトル | Effects of the crater on eruption column dynamics | |||||||||||||||||
タイトル | ||||||||||||||||||
言語 | en | |||||||||||||||||
タイトル | Effects of the crater on eruption column dynamics | |||||||||||||||||
言語 | ||||||||||||||||||
言語 | eng | |||||||||||||||||
著者 |
T. Koyaguchi
× T. Koyaguchi
× Y. J. Suzuki
× T. Kozono
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抄録 | ||||||||||||||||||
内容記述タイプ | Other | |||||||||||||||||
内容記述 | During explosive eruptions, a mixture of pyroclasts and volcanic gas forms a buoyant eruption column or a pyroclastic flow. We systematically investigate how the condition that separates these two eruption styles (column collapse condition) depends on crater shape and magma chamber conditions by integrating the theoretical models for conduit flow, flow inside a crater, and eruption column dynamics. The results show that previous model predictions of column collapse condition based on the relationship between magma discharge rate ((m)over dot) and water content (n(f)) strongly depend on crater shape (depth D and opening angle theta). When a crater is present, the decompression and/or compression of gas-pyroclast mixture inside and just above the crater result in two distinct types of column collapse: collapse with increasing (m)over dot (HM-side collapse) and that with decreasing (m)over dot (LM-side collapse). HM-side collapse is caused by an increase in conduit radius during the waxing stage of an eruption. LM-side collapse is associated with a decrease in magma chamber pressure during the waning stage. The value of (m)over dot for HM-side collapse varies by two orders of magnitude depending on crater shape for fixed nf. This estimate also depends on assumed models for decompression into the atmosphere. The value of (m)over dot for LM-side collapse is < 10(6) kg s(-1) for a shallow crater with a small opening angle, whereas it can be > 10(8) kg s(-1) when D tan theta > 10(2) m. These results are consistent with the field observations from the St. Helens 1980 and Pinatubo 1991 eruptions. | |||||||||||||||||
言語 | en | |||||||||||||||||
書誌情報 |
en : Journal of Geophysical Research: Solid Earth 巻 115, p. B07205, 発行日 2010-07 |
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出版者 | ||||||||||||||||||
言語 | en | |||||||||||||||||
出版者 | AMER GEOPHYSICAL UNION | |||||||||||||||||
ISSN | ||||||||||||||||||
収録物識別子タイプ | ISSN | |||||||||||||||||
収録物識別子 | 0148-0227 | |||||||||||||||||
DOI | ||||||||||||||||||
関連識別子 | 10.1029/2009JB007146 |