The evolution of the orbit of a small particle affected by regular and irregular components of the solar wind is examined. If the irregularity is taken into account, the pattern of motion may qualitatively change on large time scales, because the general integrals of motion are not conserved. ...
We review evidence for the FIP-related fractionation of SEPs and compare it with FIP fractionation effects in the solar wind at 1 AU. On the basis of several significant differences between the solar wind and SEP compositions, we suggest that most solar energetic particles are not simply an ...
Wave-particle interactions in the solar wind and solar flares. Resonant interactions between particles and plasma waves play an important role in both the solar wind and solar flares. The dynamics of plasma turbulence in these settings controls the strength of the interactions, by determining the am...
The wind conditions affect the performance of a solid particle solar receiver (SPSR) by convection heat transfer through the existing open aperture. Aerowindows have the potential of increasing the efficiency of an SPSR. In the present paper, the wind effect on the performance of an SPSR is inv...
The Earth’s magnetosphere is the outermost layer of the geospace system deflecting energetic charged particles from the Sun and solar wind. The solar wind has major impacts on the Earth’s magnetosphere, but it is unclear whether the same holds for sola
Real-time on-line overview of geomagnetic disturbances caused by solar wind particles, deteriorating HF propagation on Earth.
We review particle input models currently used to study the effects of particle energy input on the thermosphere-ionosphere system. We describe the objective of the climatology development, the optimal low-altitude database to be used, and the selection of indices to be incorporated into the model...
Thus, the term energetic solar particles (ESP) or solar energetic particles (SEP), i.e., energetic with respect to solar wind particles. In the following we will use the first term. Not all solar flare events produce particle fluxes that are observable on Earth. Whether or not a solar ...
Some of the accelerated particles travel to the near-Earth interplanetary medium where they can be detected by spacecraft. The most energetic of these particles produce effects at the surface of the Earth. 展开 关键词: Sun Solar wind 出版时间: 1997/12/30 ...
effects on the terrestrial space environment. At great distances from the sun it is likely that the heliosphere, with the embedded sun and planets, forms a kind of magnetosphere itself in the localinterstellar medium. A boundary will be established between the outward flowing solar wind and the...