日本地球惑星科学連合2022年大会

講演情報

[J] 口頭発表

セッション記号 S (固体地球科学) » S-VC 火山学

[S-VC32] 火山噴火のダイナミクスと素過程

2022年5月26日(木) 15:30 〜 17:00 国際会議室 (IC) (幕張メッセ国際会議場)

コンビーナ:大橋 正俊(東京大学地震研究所)、コンビーナ:並木 敦子(名古屋大学 大学院環境学研究科 地球環境科学専攻)、鈴木 雄治郎(東京大学地震研究所)、コンビーナ:新谷 直己(東北大学大学院理学研究科地学専攻地球惑星物質科学講座)、座長:新谷 直己(東北大学大学院理学研究科地学専攻地球惑星物質科学講座)、並木 敦子(名古屋大学 大学院環境学研究科 地球環境科学専攻)

16:30 〜 16:45

[SVC32-10] 浮力に駆動される合体による気泡サイズ分布の時間発展

*丸石 崇史1寅丸 敦志1 (1.九州大学)


キーワード:気泡合体、玄武岩質マグマ、流体力学

The coalescence of ascending bubbles driven by buoyancy leads to the spatial heterogeneity of volatile in basaltic magma, to control the style and dynamics of basaltic eruptions. It is essential to quantitatively know what factors and how they control bubble size distribution (BSD), because the BSD controls the coalescence process through approaching velocity between two bubbles, and in turn, the coalescence process entirely changes the BSD. First, we derive the effective cross-section for bubble coalescence, including hydrodynamic interaction between bubbles. As a result, it is found that our newly-derived effective cross-section is proportional to the product of the radii, although the geometrical cross-section is proportional to the square of the sum of the radii. Next, using both cross-sections, we numerically calculate the evolution of BSD for the initial distribution with a narrow size range. For the geometrical cross-section, the BSD shows power-law with exponent -1.3 for larger bubbles. For our effective cross-section, the BSD shows power-law with exponent -2.2 for smaller bubbles. The exponent of -2.2 is close to the exponent of -2.0 for basaltic lava (Gaonach et al., 1996). Our calculation of BSD allows us to estimate the timescale of formation of power-law, as sometimes recorded in natural samples. For both cross-sections, the power-law region extends with time and covers all the sizes at a finite time, which can be interpreted as a rapid formation of large bubbles. This result may explain the formation of large bubbles observed in lava lakes and Strombolian eruptions.