在太阳黑子半阴中检测对流下流
G B Scharmer1, V M J Henriques, D Kiselman
1Institute for Solar Physics of the Royal Swedish Academy of Sciences, and Department of Astronomy at Stockholm University, AlbaNova University Center, SE-10691 Stockholm, Sweden. scharmer@astro.su.se
天文学家观察到太阳黑点半影中的黑暗,向下流动,揭示了对流模式. 这一发现解释了Evershed流作为这个新发现的太阳对流的水平部分.
科学领域:
- 太阳物理 太阳物理
- 等离子体天体物理学
- 恒星动力学 恒星动力学
背景情况:
- 太阳黑子及其外半影长期以来一直困扰着天文学家关于它们的结构和动态.
- 之前的理论模型和模拟建议翻转对流作为半阴光纤和能量输出的解释.
研究的目的:
- 为了研究太阳黑点半阴影的精细结构和动态.
- 为了检测和描述半暗中向下流的情况.
- 了解这些流和Evershed流之间的关系.
主要方法:
- 利用来自瑞典1米太阳能望远镜的成像光谱测极数据.
- 分析数据以检测和测量太阳半影中的流速.
主要成果:
- 检测到无处不在的,相对黑暗的向下流动高达1公里/秒的内部半阴.
- 这些下流不同于形流管中的流量,并且无处不在.
- 观察到与向下流动相关的强烈的辐射外流 (3至3.5公里/秒).
结论:
- 检测到的向下流是半阴形对流流动模式的一部分.
- 埃弗舍德流被确定为这个半阴形对流的水平组成部分.
- 这一发现为太阳黑子内的能量传输和动态提供了新的理解.
更多相关视频
09:00Indoor Experimental Assessment of the Efficiency and Irradiance Spot of the Achromatic Doublet on Glass (ADG) Fresnel Lens for Concentrating Photovoltaics
Published on: October 27, 2017
11:26Integrating a Triplet-triplet Annihilation Up-conversion System to Enhance Dye-sensitized Solar Cell Response to Sub-bandgap Light
Published on: September 12, 2014
相关概念视频
Detection of Black Holes
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...
Precipitation Processes
Precipitation Titration: Endpoint Detection Methods
In the Volhard method, a standard excess of AgNO3 is first added to the...
Magnetic Field Lines
Magnetic field lines follow several hard-and-fast rules:
Precipitation Gravimetry
In determining nickel by gravimetric analysis, a precipitant of ethanolic dimethylglyoxime is added to a hot nickel salt solution. This is quickly followed by the dropwise addition of dilute ammonia solution until precipitation occurs. A...
Precipitation and Co-precipitation
