Dynamics of wind-affected volcanic plumes: The example of the 2011 Cordon Caulle eruption, Chile

被引:75
作者
Bonadonna, C. [1 ]
Pistolesi, M. [2 ]
Cioni, R. [2 ]
Degruyter, W. [3 ]
Elissondo, M. [4 ]
Baumann, V. [4 ]
机构
[1] Univ Geneva, Sect Sci Terre & Environm, Geneva, Switzerland
[2] Univ Florence, Dipartimento Sci Terra, I-50121 Florence, Italy
[3] Georgia Tech, Earth & Atmospher Sci, Atlanta, GA USA
[4] Serv Geol Minero Argentino, Buenos Aires, DF, Argentina
基金
瑞士国家科学基金会;
关键词
eruption classification; mass eruption rate; cloud spreading; turbulent diffusion; density-driven transport; plume dynamics; LABORATORY EXPERIMENTS; SOURCE PARAMETERS; TEPHRA DISPERSAL; PLINIAN ERUPTION; CHAITEN VOLCANO; BUOYANT PLUMES; ASH FORECAST; MODELS; SEDIMENTATION; MAGMA;
D O I
10.1002/2014JB011478
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The 2011 Cordon Caulle eruption represents an ideal case study for the characterization of long-lasting plumes that are strongly affected by wind. The climactic phase lasted for about 1day and was classified as subplinian with plumes between similar to 9 and 12km above the vent and mass flow rate (MFR) on the order of similar to 10(7)kgs(-1). Eruption intensity fluctuated during the first 11days with MFR values between 10(6) and 10(7)kgs(-1). This activity was followed by several months of low-intensity plumes with MFR<10(6)kgs(-1). Plume dynamics and rise were strongly affected by wind during the whole eruption with negligible upwind spreading and sedimentation. The plumes that developed on 4-6 and 20-22 June can be described as transitional, i.e., plumes showing transitional behavior between strong and weak dynamics, while the wind clearly dominated the rise height on all the other days resulting in the formation of weak plumes. Individual phases of the eruption range between Volcanic Explosivity Indices (VEIs) 3 and 4, while the cumulative deposit related to 4-7 June 2011 is associated with VEIs 4 and 5. Crosswind cloud and deposit dispersal of the first few days are best described by a linear combination of gravitational spreading and turbulent diffusion, with velocities between 1 and 10ms(-1). Downwind cloud velocity for the same days is best described by a linear combination of gravitational spreading and wind advection, with velocities between 17 and 45ms(-1). Results show how gravitational spreading can be significant even for subplinian and small-moderate eruptions strongly advected by wind and with low Richardson number and low MFR.
引用
收藏
页码:2242 / 2261
页数:20
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