太阳耀斑在一个大的冠状体内加速了几乎所有的电子
Gregory D Fleishman1, Gelu M Nita2, Bin Chen2
1Center for Solar-Terrestrial Research, New Jersey Institute of Technology, Newark, NJ, USA. gfleishm@njit.edu.
Nature
|June 8, 2022
概括
太阳耀斑加速电子, 但硬X射线观测错过了一些. 微波数据显示了电子加速的全部体积,
科学领域:
- 太阳物理
- 等离子天体物理学
- 高能天体物理学
背景情况:
- 太阳耀斑释放磁能,加速电子.
- 硬X射线观测仅限于密集的区域,可能缺少加速电子.
- 之前的研究无法完全解决电子加速体积.
研究的目的:
- 在太阳耀斑期间确定电子加速的真实空间范围.
- 调查火焰体积中的热和非热电子的分布.
- 了解磁能释放与粒子加速之间的关系.
主要方法:
- 使用微波观测进行空间分辨率分析.
- 导出热和非热电子的分布.
- 将观察到的电子分布与火焰等离子体属性进行比较.
主要成果:
- 发现一个与众不同的体积, 主要充满非热电子.
- 观察到这个加速体积已经耗尽了热等离子体.
- 发现这个体积与周围的更典型的耀斑等离子体隔离.
结论:
- 微波观测揭示了太阳耀斑中的电子加速区域.
- 有效的电子加速发生在释放的磁能中,没有热等离子体.
- 这一发现挑战了以有限的观测量为基础的先前假设.
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