The Eleventh (11th) Coronal Loops Workshop; Tenerife, Spain; June 25-28, 2024

第十一（11）届日冕环研讨会；

• 批准号: 2417806
• 负责人: Craig Johnston
• 金额: $ 1.5万
• 依托单位: George Mason University
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2024
• 资助国家: 美国
• 起止时间: 2024-03-01 至 2025-02-28
• 项目状态: 未结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=2417806&HistoricalAwards=false
• 关键词: Eleventh; 11th; Coronal; Loops; Workshop

The 11th Coronal Loops Workshop will be held at the Instituto de Astrofisica de Canarias, La Laguna, Tenerife, Spain, from June 25th – June 28th, 2024. The Loops Workshop series originated in 2002 motivated by the fact that theory was not able to explain in simple terms the coronal loop observations from missions like TRACE and SoHO. Since then, the Coronal Loops Workshop series has become a common setting for researchers to discuss in detail the basic physical processes behind the formation, evolution, and disappearance of coronal loops in solar active regions. This is a crucial discussion because it addresses one of the fundamental questions in all of space science: how the solar corona is heated to million-degree temperatures. The objectives of the workshop are to discuss the past, present and future of coronal loop theories and observations, their interrelation, and to advance our overall understanding of the physical processes that determine loop properties and govern their behavior. The main topics that Loops XI will address are: high (spatial/temporal) resolution observations of coronal loops, observations and simulations of loop cooling, reconciling 0/1-D hydrodynamic and 3-D magnetohydrodynamic models and community-driven topics (e.g. plasma diagnostics, heating mechanisms and DKIST observations). The workshop has also been very supportive of the attendance and participation of students and early career post-docs. Previous awards have been used to support travel for students to present their research at the workshops. The 2024 workshop aims to broaden participation with travel support, and those recipients will have the unique experience of touring several of the solar telescopes at the Teide Observatory.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.

第11届日冕环研讨会将于2024年6月25日至6月28日在西班牙特内里费岛拉古纳的加那利斯天文研究所举行。环路研讨会系列始于2002年，当时的理论无法用简单的术语解释TRACE和SoHO等任务观测到的日冕环路。从那时起，日冕环研讨会系列已经成为研究人员详细讨论太阳活动区日冕环形成、演化和消失背后的基本物理过程的常见场所。这是一个至关重要的讨论，因为它解决了所有空间科学中的一个基本问题：太阳日冕是如何被加热到百万度的温度的。本次研讨会的目的是讨论日冕环理论和观测的过去、现在和未来，以及它们之间的相互关系，并促进我们对决定日冕环性质和控制其行为的物理过程的全面理解。环路XI将讨论的主要主题是：日冕环的高（空间/时间）分辨率观测，环路冷却的观测和模拟，调和0/1-D流体动力学和3-D磁流体动力学模型以及社区驱动的主题（例如等离子体诊断，加热机制和DKIST观测）。研讨会也非常支持学生和早期职业博士后的出席和参与。以前的奖金被用来支持学生在研讨会上展示他们的研究。2024年的研讨会旨在通过旅行支持扩大参与，这些接受者将有参观泰德天文台几个太阳望远镜的独特体验。该奖项反映了美国国家科学基金会的法定使命，并通过使用基金会的知识价值和更广泛的影响审查标准进行评估，被认为值得支持。