日本地球惑星科学連合2016年大会

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セッション記号 S (固体地球科学) » S-VC 火山学

[S-VC48] 火山・火成活動と長期予測

2016年5月22日(日) 15:30 〜 17:00 コンベンションホールA (2F)

コンビーナ:*及川 輝樹(国研)産業技術総合研究所 活断層・火山研究部門)、長谷川 健(茨城大学理学部地球環境科学コース)、三浦 大助(一般財団法人 電力中央研究所 地球工学研究所 地圏科学領域)、石塚 吉浩(産業技術総合研究所活断層・火山研究部門)、下司 信夫(産業技術総合研究所 活断層・火山研究部門)、座長:宇野 康司(岡山大学大学院教育学研究科)、前野 深(東京大学地震研究所)

16:15 〜 16:30

[SVC48-18] 桜島火山歴史時代溶岩の斜長石斑晶サイズ分布解析 ーマグマ移動・蓄積過程の時間発展と噴火様式・頻度の関係ー

*山下 俊介1寅丸 敦志2 (1.九州大学大学院理学府地球惑星科学専攻、2.九州大学大学院理学研究院地球惑星科学部門)

キーワード:結晶サイズ分布、斜長石斑晶、マグマ供給系

In order to obtain insights into roles played by magma plumbing system in the long-term behavior of eruptive activity, we conducted crystal size distribution (CSD) analysis of plagioclase phenocrysts in four historical lavas of Sakurajima volcano, located in southern Kyushu, Japan: Bunmei eruption (1471-76), An-ei eruption (1779-82), Taisho eruption (1914-15), and Showa eruption (1946). Bunmei, An-ei, and Taisho eruptions firstly fell pumice by Plinian eruptions from newly formed flank vents, and subsequently flowed lavas. Showa eruption firstly had fell ash frequently for about three months, and subsequently flow lava from the Showa crater. After Showa eruption, Vulcanian eruptions occurred frequently, indicating the temporal change of eruptive style from large volume Plinian eruptions with lava flows (c.a. 1 km3 DRE) to small volume frequent eruptions (one event less than 10-3 km3).
In four historical lavas, plagioclase phenocrysts are classified into 3 types. Type-A is represented by the clear texture and lower An content (around An60) in core and rim. Type-B shows the clear texture and higher An content (around An80) in core and lower An content (around An60) in rim, and the sharp compositional contrast between the core and the rim. In addition, the length of rim varies by a wide range as 10-200μm in all lavas. Type-C has the sieve texture and heterogeneous compositions in core. From above chemical analysis, the magma plumbing system consist of two magma reservoirs (felsic magma chamber and mafic magma chamber) where the crystallization proceeds to form phenocrysts. Type-A crystallizes in the felsic magma chamber in which the compositions gradually changes from felsic to mafic during hundreds years by repeated injections of mafic magmas. Type-B crystalizes in the mafic magma chamber, and the mafic magma continuously injects to the felsic magma chamber.
The CSD plots of both type-A and type-B can be approximated by log-linear CSDs. Slopes of type-A are constant regardless of eruptive ages, and those of type-B become steeper with time, that is, Showa has the steepest slope. From the CSD analysis, the residence time in the felsic magma chamber is nearly constant with time, whereas the residence time in the mafic magma chamber becomes shorter with time, indicating that both mantle-derived mafic magma supply rate and extraction-rate to the felsic magma chamber increase with time. The magmatic behavior such as crystallization and accumulation rates in the felsic magma chamber keeps a constant pace and has no influence on eruptive phenomena. On the other hand, the mafic magma chamber located at deeper level controls the surficial behavior in eruptive phenomena, such as frequency of eruptive events and dominant eruption styles of Vulcanian type, through increasing rates of mantle-derived mafic magma supply.