Sun: solar windMethods: analyticalPhysical data and processes: convectionThe amount of solar wind produced continuously by the sun is not constant due to changes in solar activity. This unsteady nature of the solar wind seems to be responsible for galactic cosmic ray flux...
Real-time on-line overview of geomagnetic disturbances caused by solar wind particles, deteriorating HF propagation on Earth.
They predict the most significant effects of solar wind variation on the global magnetospheric structure. On the dayside, the region 1 Birkeland currents cause major changes of the magnetic configuration as the IMF turns southward. The tail current intensity is controlled mainly by the pressure of ...
The development of a particle climatology for the purpose of studying solar particle fluxes and their effect on the terrestrial atmospheric system has been adopted as an activity of the International Solar Cycle Study, Working Group 1, Panel 2. The activity has been incorporated as a component of...
The supply of oxygen to the ocean interior is not homogeneous across the global ocean, but is largely concentrated in specific locations of water mass formation8,9. Ventilation is the result of a suite of interacting processes10, with the main atmospheric drivers being wind stress (i.e., the...
Green, A. A. (1988) Wind Speed Effects in Solar Collector Testing. Advances in Solar Energy, Vol. 1, Pergamon Press, Oxford, U. K., pp.768-772.Green, A. A., 1988, "Wind Speed Effects in Solar Collector Testing," Ad- vances in Solar Energy Technology, Vol. 1, (Proceedings of ...
Magnetic reconnection is a key plasma process that couples the solar wind to the Earth's magnetosphere, permitting the exchange of energy and mass between these two plasmas, and converting large amounts of energy stored in the magnetic fields into kinetic energy of the particles. The magnetospheric...
Transport and turbulence modeling of solar wind fluctuations Magnetohydrodynamic (MHD) activity, including waves and turbulence, has been a focus of attention in solar wind research for several decades, owing to the ... Y Zhou,WH Matthaeus - 《Journal of Geophysical Research Space Physics》 被引...
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 solar flares—a sudden eruption of electromagn...
In this dissertation, I analyze the drivers of wind power development in the United States as well as the relationship between renewable power plant location and transmission congestion and emissions levels. I first examine the role of government renewable energy incentives and access to the electricit...