Results 31 to 40 of about 6,760 (227)
Intense Whistler-mode Waves at Foreshock Transients: Characteristics and Regimes of Wave−Particle Resonant Interaction [PDF]
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
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
The paper describes the algorithm and the results of the seismic hazard estimate based on the data of the seismological catalog of the US Geological Survey (USGS).
Aleksandr Malyshev, Lidiia Malysheva
doaj +1 more source
A global view of Pc3 wave activity in near-Earth space: Results from hybrid-Vlasov simulations
Ultra-low frequency (ULF) waves in the Pc3 range, with periods between 10–45 s, are routinely observed in Earth’s dayside magnetosphere. They are thought to originate in the foreshock, which extends upstream of the quasi-parallel bow shock and is ...
Lucile Turc +18 more
doaj +1 more source
The preparation process of natural earthquakes is still difficult to quantify and remains a subject of debate even with modern observational techniques.
F. Yamashita +5 more
semanticscholar +1 more source
Cluster-based foreshock discrimination model with flexible time horizon and mainshock magnitudes
Foreshock detection before mainshock occurrence is an important challenge limiting the short-term forecasts of large earthquakes. Various models for predicting mainshocks based on discrimination of foreshocks activity have been proposed, but many of them
Shunichi Nomura, Yosihiko Ogata
doaj +1 more source
Ultra‐low Frequency Foreshock Waves and Ion Dynamics at Mars
We study the solar wind interaction with Mars in a global three‐dimensional hybrid model. A well‐developed, vast ion foreshock forms under a strongly flow‐aligned interplanetary magnetic field (IMF) configuration but otherwise nominal solar wind and ...
R. Jarvinen, E. Kallio, T. Pulkkinen
semanticscholar +1 more source
Magnetopause Reconnection and Indents Induced by Foreshock Turbulence [PDF]
Based on global hybrid simulation results, we predict that foreshock turbulence can reach the magnetopause and lead to reconnection as well as Earth‐sized indents. Both the interplanetary magnetic field (IMF) and solar wind are constant in our simulation,
Li-Jen Chen +3 more
semanticscholar +1 more source
Strain rate and temperature dependence of Omori law scaling constants of AE data: Implications for earthquake foreshock-aftershock sequences [PDF]
Little is known about the temperature and strain rate dependence of acoustic emission AE activity (AE). Hence, we carried out a preliminary series of flow-through triaxial compression tests on porous sandstones at different temperatures and strain rates.
Ira O. Ojala +3 more
core +1 more source

