Results 101 to 110 of about 6,760 (227)
The East Aegean Sea strong earthquake sequence of October–November 2005: lessons learned for earthquake prediction from foreshocks [PDF]
Natural Hazards and Earth System Sciences, 2006 The seismic sequence of October–November 2005 in the Samos area, East Aegean Sea, was studied with the aim to show how it is possible to establish criteria for (a) the rapid recognition of both the ongoing foreshock activity and the mainshock, and (
G. A. Papadopoulos +8 more
doaj
Observations and Simulations of a Double‐Core Hot Flow Anomaly
Geophysical Research LettersHot Flow anomalies (HFAs), one of the most well‐analyzed transient phenomena in the Earth's foreshock, are known as kinetic structures driven by tangential discontinuities (TDs).
Xi Lu +4 more
doaj +1 more source
Dizhen xuebao使用云南地震台网2009—2021年的地震目录和波形数据，采用双差定位方法、基于P波初动极性和S/P振幅比的HASH方法和最大似然法等，获取了维西—乔后断裂带及附近地区ML≥4.0震群和前震序列精确的震源位置、震源机制解、视应力和b值等地震活动参数，对比分析了维西—乔后断裂带及其周边震群及前震序列的活动特征。结果显示：除前震序列频次呈现出反大森定律外，前震序列与普通震群在空间分布、震源机制一致性、视应力和b值等单一参数方面并无明显的差异；但前震序列同时具备震中优势分布方向与区域主要构造展布方向一致 ...
Guangming Wang +4 more
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Simultaneous observations of MHD hot flow anomaly and kinetic foreshock bubble and their impacts
Frontiers in PhysicsHot flow anomalies (HFAs) and foreshock bubbles (FBs) are two types of transient phenomena characterized by flow deflected and hot cores bounded by one or two compressional boundaries in the foreshock.
Xi Lu +5 more
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Earthquake Research AdvancesEarthquakes are caused by the rapid slip along seismogenic faults. Whether large or small, there is inevitably a certain nucleation process involved before the dynamic rupture.
Zhigang Peng, Xinglin Lei
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An examination of prospective foreshock probabilities in New Zealand
, 2000 This thesis investigates aspects of prospective foreshock probabilities in New Zealand. An earthquake qualifies as a foreshock if it is followed by an event of at least the same magnitude within the next 5 days and an epicentral radius of 30 km.
Merrifield, Alistair
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The ULF wave foreshock boundary: Cluster observations [PDF]
, 2015 The interaction of backstreaming ions with the incoming solar wind in the upstream region of the bow shock gives rise to a number of plasma instabilities from which ultralow frequency (ULF) waves can grow.
Meziane, Karim +9 more
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Four Point Measurements of the Foreshock
, 2008 Hybrid code numerical simulations accurately predict the properties of the Earth's foreshock, a region populated by solar wind particles heated and reflected by their interaction with the bow shock.
Angelopoulos, V. +2 more
core
UniverseThis review examines ultra-low frequency (ULF) waves across different planetary environments, focusing on Earth, Mercury, and Saturn. Data from spacecraft missions (CHAMP, Swarm, and Oersted for Earth; MESSENGER for Mercury; and Cassini for Saturn ...
Zsofia Bebesi +4 more
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Structure and Properties of the Foreshock at Venus
, 2017 The interaction of the solar wind with Venus is dominated by the planet's ionosphere that acts as an obstacle to the flow resulting in an induced magnetosphere and bow shock much smaller than their terrestrial counterparts.
Collinson, G., Omidi, N., Sibeck, D.
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