一个冠状活动区域的精细热结构
Fabio Reale1, Susanna Parenti, Kathy K Reeves
1Dipartimento di Scienze Fisiche ed Astronomiche, Sezione di Astronomia, Università di Palermo, Piazza del Parlamento 1, 90134 Palermo, Italy. reale@astropa.unipa.it
概括
研究太阳冠状的研究.
科学领域:
- 太阳物理 太阳物理
- 血物理学的等离子体物理学
- 天体物理学 天体物理学
背景情况:
- 了解太阳冠状热机制至关重要.
- 太阳王冠的热结构提供了关键的诊断信息.
研究的目的:
- 为了确定太阳冠状的细热结构.
- 使用先进的成像技术限制太阳冠状热机制.
主要方法:
- 利用HinodeX射线望远镜进行太阳冠状图像.
- 使用多个传输带和过器组合用于温度诊断.
- 从五种不同的过器中拍摄的图像中分析了能量比率.
主要成果:
- 揭示了一个高度热结构的太阳冠状在一个活跃的区域.
- 在核心和外围观测到非常细的热结构和更大的结构.
- 沿着冠状环和纠结构检测到连续的热分布.
- 在视线上发现热结构的变化.
结论:
- 观察到的细热结构对于理解冠状热是必不可少的.
- 多过器成像为太阳冠冕复杂的热特性提供了详细的见解.
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