10 papers analyzed
These studies suggest that solar five-minute oscillations impact various solar and geophysical phenomena, including sky condition estimation, ion-cyclotron waves, geoelectromagnetic waves, and the solar atmosphere's temperature and density structure.
The topic of solar five-minute oscillations encompasses various aspects of solar physics, including their detection, impact on solar and terrestrial phenomena, and underlying mechanisms. These oscillations, typically observed in the photosphere and corona, are a key feature in helioseismology and provide insights into the Sun's internal structure and dynamics.
Detection and Characteristics of Five-Minute Oscillations:
Impact on Solar Wind and Geomagnetic Phenomena:
Mechanisms of Excitation:
Nonlinear Interactions and Atmospheric Response:
Solar five-minute oscillations are a fundamental aspect of solar dynamics, detectable in various layers of the solar atmosphere and influencing both solar wind and terrestrial phenomena. Their excitation is a complex interplay of convection coupling and stochastic processes, with significant nonlinear interactions affecting the solar atmosphere. Understanding these oscillations provides valuable insights into the Sun's internal processes and their broader impact on the heliosphere.
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