日本地球惑星科学連合2023年大会

講演情報

[J] オンラインポスター発表

セッション記号 S (固体地球科学) » S-CG 固体地球科学複合領域・一般

[S-CG57] 破局噴火:メカニズムと地球表層へのインパクト

2023年5月26日(金) 13:45 〜 15:15 オンラインポスターZoom会場 (6) (オンラインポスター)

コンビーナ:奥村 聡(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)、前野 深(東京大学地震研究所)、鈴木 雄治郎(東京大学地震研究所)

現地ポスター発表開催日時 (2023/5/25 17:15-18:45)

13:45 〜 15:15

[SCG57-P03] 火山噴煙中での火山灰・ガス反応に伴う硫酸塩生成の数値計算と噴煙からの硫黄除去への応用

*渡辺 詩文1奥村 聡1鈴木 雄治郎2 (1.東北大学、2.東京大学地震研究所)


キーワード:ガス–火山灰反応、元素拡散、火砕流、SO2除去、硫黄塩、ピナツボ火山1991年噴火

Explosive volcanic eruptions inject sulfur dioxide (SO2) gases into the stratosphere. The SO2 gas can be converted into H2SO4 aerosols through chemical reactions in the stratosphere, which scatter solar radiations and decrease the temperature of the Earth’s surface. Therefore, estimating amounts of SO2 injected into the stratosphere is important to evaluate the impacts of volcanic eruptions on the Earth’s climate. Fresh volcanic ashes adhere SO2 gases onto their surfaces in eruption plume and in the conduit after magma fragmentation, resulting in the formation of CaSO4 through the reaction between Ca in the ash and SO2 gas molecules at high temperatures. When the volcanic ashes settle, the sulfate salts are removed from the eruption plume, that is, the volcanic ashes scavenge SO2 gases from the eruption plume through the formation of CaSO4. The growth of CaSO4, i.e., the process of SO2 scavenging depends on Ca diffusion at high temperatures. Here, we estimated the amount and efficiency of SO2 scavenged by volcanic ash in the eruption plume and in the conduit, combining the 3D numerical simulation of the volcanic cloud and the diffusion model.
The 3D simulation combines a pseudo-model for fluid motion and Lagrangian model for particle motion. The diffusion model assumes that the rate-limited process of the CaSO4 formation is Ca diffusion in a silicate melt and its diffusivity depends on only temperature. We obtained the temperature history of particles from the 3D simulation of the cloud and the size distribution of particles in the eruption plume was estimated based on pyroclast deposits. This model is applied to the pyroclastic flow and eruption column observed during the Pinatubo 1991 eruption. We assume the initial concentration of Ci = 4.5 wt%, and the boundary condition of C = 0 for time t > 0. Magma discharge rate was set to be 1.0×109 kg s-1 and the magma temperature was set to be 780°C.
Our calculation results showed that the amount of SO2 scavenging in the eruption plume is comparable to or slightly larger than that in the conduit. This result is quite different from the previous prediction that the amount of SO2 scavenging in the eruption plume must be low. The amount of SO2 scavenging in pyroclastic flow is larger than that in the eruption column in the case of Pinatubo. This is because pyroclastic flow forms a larger hot region just above the vent and thermal energy cannot be consumed easily by mixing volcanic gas and air compared to the eruption column. Our results also indicate that fine ash particles remove efficiently SO2 because of their high ratio of surface area to mass. An individual particle with a large size can uptake large amounts of SO2, but the contribution to the total amount of SO2scavenging is small compared to fine particles. These results are explained by considering that the large hot region formed in the eruption plume (especially in the pyroclastic flow) can trap fine particles for a long time while large particles are quickly removed from the eruption plume. Finally, we estimated the actual efficiency of SO2 scavenging during the Pinatubo 1991 eruption (9 h), using our calculation results and the satellite data of SO2 injected into the stratosphere (20 Mt), resulting in 62–81%. This estimate suggests that the large amounts of SO2 might have been scavenged in the case of the Pinatubo. However, it should be noted that our estimate includes large uncertainties.
We also found that the efficiency of the SO2 scavenging is low and high in the case of small-scale and large-scale eruptions, respectively, because the hot region in the eruption plume is more likely to be formed by large-scale eruptions. In the case of small-scale eruptions, scavenging at high temperatures can be dominant in the post-fragmentation conduit rather than in the eruption plume.