太阳耀斑1/f 波动来自振幅调制的五分钟振荡
Masahiro Morikawa1, Akika Nakamichi2
1Department of Physics, Ochanomizu University, 2-1-1 Otsuka, Bunkyo, Tokyo 112-8610, Japan.
Entropy (Basel, Switzerland)
|December 23, 2023
概括
太阳耀斑表现出1/f波动,或粉红色噪声,与低能量事件相关. 这种粉红色的噪音可能源于太阳五分钟振荡,由磁再连接调节,类似于地震和黑洞活动.
科学领域:
- 太阳物理 太阳物理
- 天体物理学 天体物理学
- 地质物理学 地质物理学
背景情况:
- 太阳耀斑表现出复杂的时间动态.
- 1/f波动或粉红色噪声在自然现象中很常见.
- 以前的研究还没有完全描述太阳耀斑时间序列的光谱特性.
研究的目的:
- 分析太阳耀斑时间序列的功率光谱密度.
- 为了研究太阳耀斑中观察到的1/f波动的起源.
- 探索太阳耀斑和其他表现出1/f波动的自然现象之间的潜在并行.
主要方法:
- 对GOES16太阳耀斑数据的分析.
- 计算发火时间序列的功率光谱密度.
- 研究太阳五分钟振荡 (SFO) 和磁重新连接过程.
主要成果:
- 太阳耀斑表现出1/f波动,特别是低能量的事件.
- 高能火焰显示平面光谱,与低能火焰不同.
- 提出了一个假设,将1/f波动与SFO的幅度调制和磁重新连接的调制联系起来,并得到了部分支持.
结论:
- 太阳耀斑1/f波动与低能量现象有关,并可能与SFO和磁再连接有关.
- 1/f波动分析框架可以扩展到地震和黑洞/磁盘系统.
- 这项研究为太阳耀斑的基础物理及其与其他复杂系统的联系提供了新的视角.
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