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Astronomy Colloquium (2017 Fall Semester)

* Date
Oct 19
* Speaker
Nai-Hwa Chen (KASI)
* Title
Energetic particles at the Sun
* Abstract
 

 

Our sun is an effective accelerator, producing highly energetic particles at all scales and driving space weather in whole solar system. Understanding the origin of those energetic particles is now a major issue in unveiling the fundamental physic processes which are also common seen in other astronomical systems. In the extended atmosphere of the Sun, known as the heliosphere, numerous eruptions take place at outer corona of the Sun in different scales in which escaping energetic particles can provide precious information of the energization processes. Additionally, those energization processes can also be investigated by multi-wavelengths observations (from radio emission to hard X-ray). In this talk, I will briefly introduce the current understandings of those fundamental questions (such as the dominant acceleration process in solar transient eruptions, how do those energetic particles propagate and fill the heliosphere?) and also address some following issues to be answered.
 
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