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Field electron emission characteristics of energetic silicon ion irradiated carbon nanotube arrays were investigated.
The results of this study indicated that the proposed thermal history method can be successfully used to quickly and effectively identify the autocatalysis characteristics of energetic materials.
Based on previous models of particle acceleration at CME-driven shocks, our simulation allows us to investigate various characteristics of energetic particles arriving at various distances from the sun.
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The size and morphology of the fuel and oxidizer and the pellet density are important factors influencing the burn characteristics of energetic-material (EM) pellets.
We discuss spatial and temporal characteristics of the energetic particle interaction with the foreshock plasma.
While it is now common to refer to a solar event as "impulsive" or "gradual," the classification of the event can be difficult in practice and does not completely clarify the characteristics of solar energetic particles.
The total output of the NM-BANGLE Model is a multi-dimensional GLE picture that gives an important contribution to revealing the characteristics of solar energetic particle events recorded at ground level.
In this work, we study the anisotropy characteristics of solar energetic electron (E > 53 keV) fluxes observed by the ULYSSES/HI-SCALE instrument during the passage of a well-identified Coronal Mass Ejection.
On board the Auroral satellite, SKA-3 (a set of particle detectors) and the magnetometer IMAP-3 provide in-situ characteristics of the energetic particles and the magnetic field, respectively.
Systematic local time and radial dependencies observed in the characteristics of the energetic ion and electron distributions, specifically the particle pitch angle distributions and particle flow pattern are discussed.
Further investigation of the characteristics and frequency of energetic swell waves are recommended to enhance prediction and the design of coastal defences, and hence reduce their consequences.
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