Structures and Fluctuations of Solar Wind
A special issue of Atmosphere (ISSN 2073-4433). This special issue belongs to the section "Upper Atmosphere".
Deadline for manuscript submissions: closed (28 June 2024) | Viewed by 268
Special Issue Editors
Interests: solar wind observations; interplanetary coronal mass ejections; space weather
Special Issue Information
Dear Colleagues,
Multi-scale structures and fluctuations have been measured in solar wind. The scales range from days to electron gyro periods. The origin and evolution of these structures and fluctuations are key questions of heliophysics. As one type of day-scale structure, the Interplanetary Coronal Mass Ejection (ICME) is the largest eruption in the solar system, which is the main driver of geoeffectiveness. However, the components, evolution and propagation of ICMEs are still unclear due to their strong variability. On the other hand, waves under the ion-gyro-scale are important for energy transmission and dissipation. To reveal the mechanisms of generation and the evolution of these multi-scale structures and fluctuations in solar corona or in interplanetary space, both simulations and observations focus on the heating and accelerating processes and interplanetary magnetic field variation. This Special Issue aims to collect recent important work on the origin and evolution of the multi-scale structures and fluctuation of solar wind from different aspects. It may help us to understand one structure or fluctuation deeper in an interactive view.
Dr. Shuo Yao
Dr. Zhifang Guo
Guest Editors
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Keywords
- solar wind turbulence
- interplanetary magnetic field structures and reconnections
- interplanetary coronal mass ejections
- interplanetary shocks and energetic particles
- MHD waves and kinetic waves
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