A Helioseismic Study of Active Region Flows and their Contribution to Global Dynamics

作为这个为期三年的项目的一部分，将进行的调查将大大增加我们对太阳内部地下流动物理学的了解，使其随着磁区特性和时间的变化得以确定。 该研究计划旨在了解这些流动如何影响较大的环流模式，特别是全球环流的纬向和纬向流动成分。 日冕流在导致太阳极场极性反转的过程中起着至关重要的作用，并且能够预测随后的太阳周期的性质。 目前尚不清楚活跃地区相关资金流入的贡献如何及时调节它。 由该研究项目提供的对这一贡献的定量评估将允许在预测模型中做出关键改进。 关于流动的物理学理论已经提出，并预测了它们随深度的变化。 作为本项目的一部分，这些预测将通过逆向建模工作进行测试。 研究活动还将利用从数值磁流体动力学模拟中获得的人工数据，旨在开发和验证可靠推断地下流动的方法，避免地表磁场对地震波的影响造成的人为现象。 这些方法对于改进和验证通过日震学推断的流动和结构的其他模型将是非常宝贵的，这个为期三年的项目的主要目的是对太阳磁区周围的地下流动进行全面的、高空间分辨率的日震调查，以改进太阳发电机模型。 该研究项目有四个主要目标。第一个目标是，利用应用于SDO使命机载日震成像仪多普勒图的日震全息照相术，确定在太阳活动区周围观测到的近地表气流的特征。 该表征将包括检查流动特性与磁通量的依赖性。 随着区域的发展，流动的时间依赖性也将被检查。 第二个目标是建立和量化的贡献，近地表流动周围的活跃地区的纬度和时间变化的全球纬向和纬向流模式。 这将通过比较活动区域相关流量的月时间和经度平均值与纬向和纬向流量测量值来实现。 第三个目标是通过日震逆模型确定活动区相关流动的深度依赖性，以便对流动有一个物理上的了解。 第四个目标是验证活动区域周围流量确定的可靠性。 这将通过使用现有的合成数据来实现，这些数据来自于对磁结构附近的波进行的最先进的数值MHD模拟，需要了解太阳内部与活动区相关的流动对大尺度动力学的贡献，以改进太阳发电机的表面通量输运模型。 预计该项目的成果将增进对太阳和恒星发电机以及磁场演变的一般了解。 预期的结果将有助于改进对太阳周期的预测。 作为该计划的一部分，项目小组将广泛传播数据产品，供其在这些类型的模型中使用。 该项目将促进该小组继续参与博尔德科罗拉多大学主办的太阳和空间物理学REU方案。 这项研究的相当一部分是由一名博士后研究科学家进行的，他将领导几项项目任务。 该项目的研究和EPO议程支持AGS部门在发现，学习，多样性和跨学科研究方面的战略目标。

The survey to be produced as part of this 3-year project will considerably increase our knowledge about the physics of subsurface flows inside the Sun, allowing their variation with magnetic region properties, and with time, to be ascertained. The research program seeks to understand how these flows affect larger circulation patterns, particularly the meridional and zonal flow components of global circulation. The meridional flow is involved critically in the process that leads to Sun's polar field polarity reversals and the ability to predict properties of subsequent solar cycles. It is not clear how it is modulated in time by the contribution of active-region related inflows. A quantitative assessment of this contribution, provided by this research project, will allow critical improvements to be made in predictive models. Theories regarding the physics of the flows have been put forward, with predictions about their variation with depth. These predictions will be tested by the inverse modeling efforts as part of this project. Using artificial data available from numerical MHD simulations, the research activities will also aim to develop and validate methods to infer subsurface flows reliably and which avoid artifacts caused by the influence of surface magnetic fields on the seismic waves. These methods will be invaluable for improving and validating other models of flows and structures inferred through helioseismology.The main purpose of this 3-year project is to perform a comprehensive, high-spatial-resolution helioseismic survey of subsurface flows around solar magnetic regions in order to improve models of solar dynamo. The research project has four main objectives. The first objective is to characterize, using helioseismic holography applied to Dopplergrams from the Helioseismic Imager onboard the SDO mission, the near-surface flows observed around solar active regions. This characterization will include examining the dependence of the flow properties with magnetic flux. The time dependence of the flows as regions evolve will also be examined. The second objective is to establish and quantify the contribution of the near-surface flows surrounding active regions to the latitudinal- and temporal-variation of the global meridional and zonal flow patterns. This will be achieved by comparing monthly time and longitude averages of active-region related flows with meridional and zonal flow measurements. The third objective is to determine, through helioseismic inverse modeling, the depth dependence of active-region related flows, in order to provide a physical understanding of the flows. The fourth objective is to validate the reliability of the flow determination around active regions. This will be achieved using existing synthetic data derived from state-of-the-art numerical MHD simulations of waves in the vicinity of magnetic structures.An understanding of the contribution of active-region-related flows in Sun's interior to the larger-scale dynamics is required for improving surface-flux-transport models of the solar dynamo. The outcome of this project is expected to improve general knowledge of solar and stellar dynamos and the evolution of magnetic fields. The expected results will allow improvements in predicting the solar-cycles of the Sun. The project team will broadly disseminate data products for their use in these types of models as part of this program. This project will facilitate continued involvement of the team in the REU Program in Solar and Space Physics hosted by the University of Colorado at Boulder. A considerable portion of this research is being carried out by a postdoctoral research scientist who will take the lead on several of the project tasks. The research and EPO agenda of this project supports the Strategic Goals of the AGS Division in discovery, learning, diversity, and interdisciplinary research.