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交换过器:用于广场EUV太阳能图像的简单的亚齐木斯变量辐射过器
Daniel B Seaton1, David Berghmans2, D Shaun Bloomfield3
1Southwest Research Institute, Boulder, CO USA.
概括
我们开发了SWAP过器,以增强太阳冠状的极端紫外线 (EUV) 图像. 这种新的过器可以更好地分析来自广泛视野太阳观测的低信号噪声数据.
科学领域:
- 太阳物理 太阳物理
- 太空天气 太空天气
- 天文学 天文学
背景情况:
- 极端紫外线 (EUV) 成像对于研究太阳冠状的研究至关重要.
- 在中部冠状病毒中分析低信号对噪声数据存在重大挑战.
- 带有主动像素和图像处理 (SWAP) 仪器的太阳观测器提供了广泛的视野EUV观测.
研究的目的:
- 介绍和描述SWAP过器,一种新的图像处理技术.
- 详细介绍过器的开发,实现和可配置参数.
- 为了证明过器在增强EUV太阳冠状图像方面的有效性.
主要方法:
- 研发了一种异方向变化的,辐射正常化过器.
- 将SWAP过器应用于PROBA2.2上的SWAP仪器对EUV图像的应用.
- 用户可配置的参数,用于定制的数据处理.
主要成果:
- SWAP过器有效地增强了EUV太阳冠状图像中的特征.
- 在数据质量方面取得了明显的改善,特别是在信号对噪声效应较低的地区.
- 这些例子说明了波器对科学数据分析的影响.
结论:
- SWAP过器是处理EUV太阳冠状图像的宝贵工具.
- 它解决了对先进分析技术与新的观测数据日益增长的需求.
- 这种过器预计将在未来的太阳物理研究中变得越来越重要.
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