相关实验视频
Updated: Jul 22, 2025

11:47
A 100 KW Class Applied-field Magnetoplasmadynamic Thruster
Published on: December 22, 2018
9.1K
一个强磁化太阳黑子中的横振荡和能量源
概括
科学家在太阳斑纤维中检测到强烈的横向波. 这些波带有相当大的能量,可能解释太阳冠冕的高温,并有助于未来的太阳望远镜观测.
科学领域:
- 太阳物理 太阳物理
- 等离子体物理学的物理学
- 磁动力学 磁动力学
背景情况:
- 太阳冠状体比光球要热得多,因此需要大量的热流.
- 冠状体等离子体经历强烈的能量损失,需要持续的能量输入来维持其高温.
研究的目的:
- 检测和表征染色球阴纤维中的横向波.
- 为了估计这些波带来的能量流.
- 为了研究这些波在冠状热中的作用.
主要方法:
- 使用1.6米高德太阳望远镜进行高分辨率观测.
- 在阴影纤维中检测到无处不在和持久的横向波.
- 波浪能量流量的估计.
- 两流体磁动力学模拟以重现观测并分析波浪散射.
主要成果:
- 在膜纤维中检测到无处不在和持久的横向波.
- 这些波带来的估计能量流量为7.52 × 10^6 W m^-2,明显超过了等离子体能量损失率.
- 模拟证实,这些波浪散发大量的能量.
结论:
- 阴影纤维中的横波带有显著的能量流,对于冠状热至关重要.
- 这些振荡可能在各种磁化太阳区域中普遍存在.
- 这些发现突出了下一代太阳能望远镜的潜在目标.
关键词:
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