Results 11 to 20 of about 129,945 (270)

Automatic Bayesian polarity determination [PDF]

open access: yes, 2016
The polarity of the first motion of a seismic signal from an earthquake is an important constraint in earthquake source inversion. Microseismic events often have low signal-to-noise ratios, which may lead to difficulties estimating the correct first ...
Christie, PAF, Pugh, DJ, White, RS
core   +3 more sources

CFM: a Convolutional network for First Motion polarity classification of earthquake waveforms.

open access: yes, 2023
The knowledge of the crustal stress field is essential in the evaluation of the seismic hazard of an area.To this aim, it is necessary to derive reliable focal mechanisms mainly when small earthquakes have to be included in the computation. The first motion focal mechanism solution techniques are still widely used in modern softwares. The determination
G. Messuti   +4 more
openaire   +4 more sources

Stick‐Slip Tremor Beneath an Alpine Glacier

open access: yesGeophysical Research Letters, 2021
Sliding of glacial ice over its base is typically described by a frictionless or slowly deforming bed. This view is challenged by recent seismic observations of stick‐slip motion at the ice‐bed interface.
J. Umlauft   +6 more
doaj   +1 more source

Reliability of Focal Mechanism Solutions for Small and Medium Earthquakes Based on Different Methods

open access: yesTaiyuan Ligong Daxue xuebao, 2022
Three representative small and medium earthquakes in Shanxi seismic belt in recent years were taken as examples. By using different methods, such as the first motion of P-wave, first motion of P-wave combining P/SV/SH amplitude ratio, CAP (Cut and Past),
Penghu GUAN   +4 more
doaj   +1 more source

An MCMC Bayesian full moment tensor inversion constrained by first-motion polarities and double couple percent [PDF]

open access: yes, 2020
Abstract. Monte Carlo Markov chain (MCMC) samplings can obtain a set of samples by directed random walk, mapping the posterior probability density of the model parameters in Bayesian framework. We perform earthquake waveform inversion to retrieve focal angles or the elements of moment tensor and source location using a Bayesian MCMC method with the ...
Mehrdad Pakzad   +2 more
openaire   +2 more sources

Coordinated Cluster/Double Star observations of dayside reconnection signatures [PDF]

open access: yesAnnales Geophysicae, 2005
The recent launch of the equatorial spacecraft of the Double Star mission, TC-1, has provided an unprecedented opportunity to monitor the southern hemisphere dayside magnetopause boundary layer in conjunction with northern hemisphere observations by ...
M. W. Dunlop   +21 more
doaj   +1 more source

The role of photospheric converging motion in initiation of solar eruptions

open access: yesFrontiers in Astronomy and Space Sciences, 2022
It is well-known that major solar eruptions are often produced by active regions with continual photospheric shearing and converging motions. Here, through high-accuracy magnetohydrodynamics simulation, we show how solar eruption is initiated in a single
Xinkai Bian   +2 more
doaj   +1 more source

Numerical Studies on the Motions of Magnetically Tagged Cells Driven by a Micromagnetic Matrix

open access: yesMicromachines, 2023
Precisely controlling magnetically tagged cells in a complex environment is crucial to constructing a magneto-microfluidic platform. We propose a two-dimensional model for capturing magnetic beads from non-magnetic fluids under a micromagnetic matrix.
Shanjia Tao   +3 more
doaj   +1 more source

Mechanism of High Frequency Shallow Earthquake Source in Mount Soputan, North Sulawesi

open access: yesIndonesian Journal on Geoscience, 2014
DOI: 10.17014/ijog.v6i3.122Moment tensor analysis had been conducted to understand the source mechanism of earthquakes in Soputan Volcano during October - November 2010 period. The record shows shallow earthquakes with frequency about 5 - 9 Hz.
Yasa Suparman   +2 more
doaj   +1 more source

Dynamic Coupling of Convective Flows and Magnetic Field during Flux Emergence [PDF]

open access: yes, 2011
We simulate the buoyant rise of a magnetic flux rope from the solar convection zone into the corona to better understand the energetic coupling of the solar interior to the corona. The magnetohydrodynamic model addresses the physics of radiative cooling,
Abbett   +35 more
core   +1 more source

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