Air ionization at rock surfaces and pre-earthquake signals

被引:160
作者
Freund, Friedemann T. [1 ,2 ,3 ]
Kulahci, Ipek G. [3 ]
Cyr, Gary [4 ]
Ling, Julia [5 ,6 ]
Winnick, Matthew [7 ]
Tregloan-Reed, Jeremy [3 ,8 ]
Freund, Minoru M. [2 ]
机构
[1] San Jose State Univ, SETI Inst, Dept Phys, REU Summer 2008, San Jose, CA 95192 USA
[2] NASA, Ames Res Ctr, Code SGE, Moffett Field, CA 94035 USA
[3] SETI Inst, Carl Sagan Ctr, Mountain View, CA 94043 USA
[4] San Jose State Univ Fdn, San Jose, CA 95192 USA
[5] NASA, Ames Res Ctr, NASA Acad 2007, Moffett Field, CA 94025 USA
[6] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA
[7] Vassar Coll, Dept Phys & Astron, Poughkeepsie, NY 12604 USA
[8] Univ Lancaster, Dept Phys, Lancaster LA1 4YQ, England
关键词
Pre-earthquake phenomena; Ionosphere; Air ionization; Corona discharges; Thermal infrared anomalies; Earthquake lights; Animal behavior; KOBE EARTHQUAKE; IONOSPHERE; ANOMALIES; MECHANISM; LIGHTS; RADON; PREDICTION; IRAN;
D O I
10.1016/j.jastp.2009.07.013
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
Pre-earthquake signals have been widely reported, including perturbations in the ionosphere. These precursory signals, though highly diverse, may be caused by just one underlying physical process: activation of highly mobile electronic charge carriers in rocks that are subjected to ever increasing levels of stress. The charge carriers are defect electrons associated with O- in a matrix of O2-. Known as positive holes or pholes h(center dot), they flow out of the stressed rock into the unstressed rock volume, traveling meters in the laboratory, probably kilometers in the field. At the rock-air interface they cause: (i) positive surface potential, (ii) field-ionization of air molecules, (iii) corona discharges. The rate of formation of airborne ions can exceed 10(9) cm(-2) s(-1). Massive air ionization prior to major earthquakes increases the electrical conductivity in the air column and may cause ionospheric perturbations, earthquake lights, and unusual animal behavior as well as infrared emission. (C) 2009 Elsevier Ltd. All rights reserved.
引用
收藏
页码:1824 / 1834
页数:11
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