Results 21 to 30 of about 6,894 (231)

3-D global hybrid simulations of magnetospheric response to foreshock processes

open access: yesEarth, Planets and Space, 2021
It has been suggested that ion foreshock waves originating in the solar wind upstream of the quasi-parallel (Q-||) shock can impact the planetary magnetosphere leading to standing shear Alfvén waves, i.e., the field line resonances (FLRs). In this paper,
Feng Shi   +4 more
doaj   +2 more sources

From Foreshock 30-Second Waves to Magnetospheric Pc3 Waves. [PDF]

open access: yesSpace Sci Rev
Ultra-low frequency waves, with periods between 1-1000 s, are ubiquitous in the near-Earth plasma environment and play an important role in magnetospheric dynamics and in the transfer of electromagnetic energy from the solar wind to the magnetosphere.
Turc L   +9 more
europepmc   +2 more sources

Transmission of foreshock waves through Earth's bow shock. [PDF]

open access: yesNat Phys, 2023
The Earth’s bow shock results from the interaction of the solar wind with the terrestrial magnetic field. With global numerical simulations and spacecraft observations, the transmission of fast magnetosonic waves through the bow shock is revealed.
Turc L   +14 more
europepmc   +2 more sources

Seismic Sequence Vulnerability of Low-Rise Special Moment-Resisting Frame Buildings with Brick Infills

open access: yesApplied Sciences, 2022
When buildings are exposed to earthquake sequence, damage aggravation is expected to occur. Although several studies report seismic vulnerability of reinforced concrete (RC) buildings under the mainshock–aftershock sequence, indicating damage aggravation
Pushpa Mahat   +5 more
doaj   +1 more source

On the correlations between the largest foreshocks and mainshocks of earthquake sequences in Taiwan

open access: yesFrontiers in Earth Science, 2023
We collected a data set of mainshocks and their respective largest foreshocks of 38 earthquake sequences in Taiwan. The plot of local magnitude, ML, of a mainshock (denoted by MLm) versus ML of its largest foreshock (denoted by MLf) shows an increase in ...
Kou-Cheng Chen   +3 more
doaj   +1 more source

A laboratory perspective on accelerating preparatory processes before earthquakes and implications for foreshock detectability. [PDF]

open access: yesNat Commun
Dynamic failure in the laboratory is commonly preceded by many foreshocks which accompany premonitory aseismic slip. Aseismic slip is also thought to govern earthquake nucleation in nature, yet, foreshocks are rare. Here, we examine how heterogeneity due
Goebel THW   +4 more
europepmc   +2 more sources

Preacceleration in the Electron Foreshock. I. Electron Acoustic Waves [PDF]

open access: yesAstrophysical Journal, 2022
To undergo diffusive shock acceleration, electrons need to be preaccelerated to increase their energies by several orders of magnitude, else their gyroradii will be smaller than the finite width of the shock.
P. J. Morris   +3 more
semanticscholar   +1 more source

Foreshock properties illuminate nucleation processes of slow and fast laboratory earthquakes

open access: yesNature Communications, 2023
Understanding the connection between seismic activity and the earthquake nucleation process is a fundamental goal in earthquake seismology with important implications for earthquake early warning systems and forecasting.
D. C. Bolton   +3 more
semanticscholar   +1 more source

Intense Whistler-mode Waves at Foreshock Transients: Characteristics and Regimes of Wave−Particle Resonant Interaction [PDF]

open access: yesAstrophysical Journal, 2022
Thermalization and heating of plasma flows at shocks result in unstable charged-particle distributions that generate a wide range of electromagnetic waves. These waves, in turn, can further accelerate and scatter energetic particles. Thus, the properties
Xiao-Fei Shi   +5 more
semanticscholar   +1 more source

The Geoeffectiveness of Solar Wind Current Sheets and Its Modulation by Foreshock Ions

open access: yesGeophysical Research Letters, 2022
We examined the evolution of 34 solar wind bifurcated current sheets in the magnetosheath and their magnetospheric responses, using the in‐situ observations of the THEMIS probes and the GOES satellites.
Boyi Wang   +3 more
doaj   +1 more source

Home - About - Disclaimer - Privacy