Decadal to monthly timescales of magma transfer and reservoir growth at a caldera volcano

被引:299
作者
Druitt, T. H. [1 ,2 ,3 ]
Costa, F. [4 ]
Deloule, E. [5 ]
Dungan, M. [6 ]
Scaillet, B. [7 ]
机构
[1] Univ Blaise Pascal, Clermont Univ, Lab Magmas & Volcans, F-63000 Clermont Ferrand, France
[2] CNRS, UMR 6524, LMV, F-63038 Clermont Ferrand, France
[3] IRD, LMV, F-63038 Clermont Ferrand, France
[4] Nanyang Technol Univ, Earth Observ Singapore, Singapore 639798, Singapore
[5] CRPG CNRS, F-54501 Vandoeuvre Les Nancy, France
[6] Univ Geneva, Dept Mineral, CH-1205 Geneva, Switzerland
[7] Univ Tours, Univ Orleans, CNRS, ISTO UMR 6113, F-45071 Orleans, France
关键词
RESIDENCE TIMES; ION MICROPROBE; PLAGIOCLASE; DIFFUSION; SANTORINI; EVOLUTION; RECHARGE; TRACE; SR; EMPLACEMENT;
D O I
10.1038/nature10706
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Caldera-forming volcanic eruptions are low-frequency, high-impact events capable of discharging tens to thousands of cubic kilometres of magma explosively on timescales of hours to days, with devastating effects on local and global scales(1). Because no such eruption has been monitored during its long build-up phase, the precursor phenomena are not well understood. Geophysical signals obtained during recent episodes of unrest at calderas such as Yellowstone, USA, and Campi Flegrei, Italy, are difficult to interpret, and the conditions necessary for large eruptions are poorly constrained(2,3). Here we present a study of pre-eruptive magmatic processes and their timescales using chemically zoned crystals from the 'Minoan' caldera-forming eruption of Santorini volcano, Greece(4), which occurred in the late 1600s BC. The results provide insights into how rapidly large silicic systems may pass from a quiescent state to one on the edge of eruption(5,6). Despite the large volume of erupted magma(4) (40-60 cubic kilometres), and the 18,000-year gestation period between the Minoan eruption and the previous major eruption, most crystals in the Minoan magma record processes that occurred less than about 100 years before the eruption. Recharge of the magma reservoir by large volumes of silicic magma (and some mafic magma) occurred during the century before eruption, and mixing between different silicic magma batches was still taking place during the final months. Final assembly of large silicic magma reservoirs may occur on timescales that are geologically very short by comparison with the preceding repose period, with major growth phases immediately before eruption. These observations have implications for the monitoring of long-dormant, but potentially active, caldera systems.
引用
收藏
页码:77 / U97
页数:6
相关论文
共 44 条
[1]  
Aizawa K, 2006, GEOL SOC SPEC PUBL, V269, P65, DOI 10.1144/GSL.SP.2006.269.01.05
[2]  
Andersen DJ., 1985, EOS Trans Am Geophys Union, V66, P416
[3]  
[Anonymous], EUROPEAN LAB VOLCANO
[4]   On the origin of crystal-poor rhyolites: Extracted from batholithic crystal mushes [J].
Bachmann, O ;
Bergantz, GW .
JOURNAL OF PETROLOGY, 2004, 45 (08) :1565-1582
[5]   Ion microprobe study of plagioclase-basalt partition experiments at natural concentration levels of trace elements [J].
Bindeman, IN ;
Davis, AM ;
Drake, MJ .
GEOCHIMICA ET COSMOCHIMICA ACTA, 1998, 62 (07) :1175-1193
[6]   CRYSTAL-CHEMICAL CONTROLS ON THE PARTITIONING OF SR AND BA BETWEEN PLAGIOCLASE FELDSPAR, SILICATE MELTS, AND HYDROTHERMAL SOLUTIONS [J].
BLUNDY, JD ;
WOOD, BJ .
GEOCHIMICA ET COSMOCHIMICA ACTA, 1991, 55 (01) :193-209
[7]   A rapid mechanism to remobilize and homogenize highly crystalline magma bodies [J].
Burgisser, Alain ;
Bergantz, George W. .
NATURE, 2011, 471 (7337) :212-U97
[8]   Cation Diffusion in Feldspars [J].
Cherniak, D. J. .
DIFFUSION IN MINERALS AND MELTS, 2010, 72 :691-733
[9]   Diffusion coupling between trace and major elements and a model for calculation of magma residence times using plagioclase [J].
Costa, F ;
Chakraborty, S ;
Dohmen, R .
GEOCHIMICA ET COSMOCHIMICA ACTA, 2003, 67 (12) :2189-2200
[10]  
Costa F., 2010, Timescales of Magmatic Processes: From Core to Atmosphere, DOI DOI 10.1002/9781444328509.CH7