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Updated: Jun 12, 2026

11:41
Magnetic Tweezers for the Measurement of Twist and Torque
Published on: May 19, 2014
在射手座A事件地平线附近的磁场结构和可变性
Michael D Johnson1, Vincent L Fish2, Sheperd S Doeleman3
1Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA. mjohnson@cfa.harvard.edu.
概括
在我们银河系中心的超大质量黑洞射手座A*附近观测到磁场. 这些场地在事件视界附近, 显示了部分秩序和可变性, 提供了对黑洞物理学的新见解.
科学领域:
- 天体物理学
- 黑洞物理
- 磁动力学
背景情况:
- 黑洞周围的收缩盘被认为是通过微分旋转来放大磁场.
- 这些增强的磁场对于同步发射和相对论喷气形成等现象至关重要.
- 对地平线尺度磁场结构的观测证据一直缺乏.
研究的目的:
- 在射手座A*事件地平线附近空间解析磁场结构.
- 调查超大质量黑洞附近磁场的存在和性质.
- 检测和描述这些磁场的变化.
主要方法:
- 使用1.3毫米波长的干扰测量观测.
- 来自射手座A*的空间分辨率线性极化辐射.
- 分析数据以推断事件地平线尺度上的磁场特性.
主要成果:
- 在 Sagittarius A* 的事件地平线附近发现了部分有序磁场的证据.
- 在大约6个施瓦茨希尔德半径的尺度上解析这些磁场.
- 与这些磁场相关的局部内小时变化.
结论:
- 这些发现支持黑洞附近的磁场生成和放大理论.
- 提供了对地平线尺度有序磁场的第一个观测证据.
- 表明这些磁场在积累和流出过程中起着重要作用.
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