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为阿塔卡马大孔径亚毫米望远镜 (AtLAST) 进行科学发展研究:太阳和恒星观测
Sven Wedemeyer1,2, Miroslav Barta3, Roman Brajša4
1Rosseland Centre for Solar Physics, University of Oslo, Oslo, Oslo, N-0315, Norway.
Open research Europe
|August 14, 2024
概括
拟议的阿塔卡马大孔径亚毫米望远镜 (AtLAST) 将为观测太阳和恒星提供新的能力. 这将增强我们对恒星大气层,耀斑和太阳周期的理解.
科学领域:
- 太阳物理学和天体物理学
- 恒星大气的研究研究恒星大气.
- 太阳系外行星研究研究
背景情况:
- 亚毫米观测提供了对恒星染色球的独特见解.
- 目前的天文台缺乏用于详细研究太阳大气的诊断能力.
- 太阳是理解活跃恒星的关键参考.
研究的目的:
- 概述阿塔卡马大孔径亚毫米望远镜 (AtLAST) 的科学案例.
- 定义AtLAST的技术要求,以解决关键的太阳和恒星科学问题.
- 突出AtLAST在研究恒星活动及其对系外行星的影响方面的潜力.
主要方法:
- 在一个扩展的频率范围内同时观察辐射连续.
- 大型太阳区域和整个太阳盘的高时间节奏映射.
- 用于研究太阳活动周期的长期光学观测.
主要成果:
- AtLAST将能够详细地绘制不同的太阳大气层,揭示3D结构.
- 它将有助于检测和跟踪高时间分辨率的耀斑和突出点.
- 综光观测将提供一个前所未有的视图的太阳循环在亚毫米的制度.
结论:
- 亚特拉斯特的拟议能力将大大推进太阳和恒星物理学.
- 它将使我们能够更深入地了解恒星染色体,活动以及它们对系外行星的影响.
- 该望远镜准备好解决当前观测天文学中的关键差距.
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