Collaborative Research: SHINE: Observational and Theoretical Studies of the Parametric Decay Instability in the Lower Solar Atmosphere

合作研究：SHINE：太阳低层大气参数衰变不稳定性的观测和理论研究

• 批准号: 2229100
• 负责人: Michael Hahn
• 金额: $ 58.87万
• 依托单位: Columbia University
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2023
• 资助国家: 美国
• 起止时间: 2023-01-01 至 2025-12-31
• 项目状态: 未结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=2229100&HistoricalAwards=false
• 关键词: Collaborative; Research; SHINE; Observational; Theoretical

It is unclear how the outer layer of the Sun, the corona, is heated to millions of degrees. One potential mechanism is through the parametric decay instability (PDI). This project addresses the Solar, Heliospheric, and Interplanetary Environment (SHINE) goal of understanding the solar corona through numerical simulations and analysis of space-based and NSF-funded ground based solar observations. The project also supports outreach activities in New York City and New Mexico. Two post-doctoral researchers will be supported, along with undergraduate students at Columbia University.The project will determine whether PDI is an important process in the solar atmosphere. The team will analyze observations from the Coronal Multichannel Polarimeter, the Extreme Ultraviolet Imaging Spectrometer, the Interface Region Imaging Spectrometer, and the NSF-funded Daniel K. Inouye Solar Telescope. Numerical modeling will be used to better understand the behavior of PDI in the presence of gradients in the plasma properties of the transition region and the corona. Magnetohydrodynamic simulations will be carried out to study Alfven waves and PDI growth in the lower solar atmosphere, where the scale length of gradients is smaller than the wavelength. This is critical to understand how density fluctuations are generated very close to the Sun. Moreover, ion heating associated with acoustic waves produced by PDI will be investigated using hybrid simulations, to estimate what fraction of the Alfven wave power can be dissipated in the lower atmosphere.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.

目前还不清楚太阳的外层日冕是如何被加热到数百万度的。一个潜在的机制是通过参数衰减不稳定性（PDI）。该项目涉及太阳、日光层和行星际环境（SHINE）的目标，即通过数值模拟和分析天基和NSF资助的地面太阳观测来了解日冕。该项目还支持在纽约市和新墨西哥州开展外联活动。哥伦比亚大学的两名博士后研究人员将得到沿着本科生的支持。该项目将确定PDI是否是太阳大气中的一个重要过程。该团队将分析日冕多通道偏振仪、极紫外成像光谱仪、界面区成像光谱仪和NSF资助的丹尼尔K。Inouye太阳望远镜。数值模拟将被用来更好地理解的行为的PDI在过渡区和电晕的等离子体特性的梯度的存在。将进行磁流体动力学模拟，以研究阿尔芬波和PDI增长在较低的太阳大气中，梯度的尺度长度小于波长。这对于理解密度波动是如何在非常靠近太阳的地方产生的至关重要。此外，还将使用混合模拟研究与PDI产生的声波相关的离子加热，以估计阿尔芬波功率中有多少部分可以在低层大气中消散。该奖项反映了NSF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。