How Nanoflares Produce Kinetic Waves, Nano-Type III Radio Bursts, and Non-Thermal Electrons in the Solar Wind

Observations of the solar corona and the solar wind discover that the solar wind is unsteady and originates from the impulsive events near the surface of the Sun's atmosphere. How solar coronal activities affect the properties of the solar wind is a fundamental issue in heliophysics. We report...

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Veröffentlicht in:	Journal of physics. Conference series 2018-10, Vol.1100 (1), p.12005
1. Verfasser:	Che, H.
Format:	Artikel
Sprache:	eng
Schlagworte:	Charged particles Distribution functions Electron beams Electron velocity distribution Radio emission Solar corona Solar radio bursts Solar surface Solar wind
Online-Zugang:	Volltext
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