【摘 要】
：
Observations from multiple spacecraft show that there are energy spectral "breaks" at 1–10 Me V in some large CME-driven shocks. However, numerical models can hardly simulate this property due to high
【出 处】
：
Research in Astronomy and Astrophysics
论文部分内容阅读
Observations from multiple spacecraft show that there are energy spectral "breaks" at 1–10 Me V in some large CME-driven shocks. However, numerical models can hardly simulate this property due to high computational expense. The present paper focuses on
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