SGER: Feasibility of Taking the MAS (Magnetohydrodynamic Algorithm outside a Sphere) Model to Petascale

该项目是一项探索性活动，旨在测试性能建模和优化的新专业知识和技术在日冕数值模拟中的应用。 它包括初步工作，以确定未来的努力，以开发一个千万亿次版本的磁流体动力学算法外的球体模型（MAS）的可行性。 如果MAS和类似的模型可以在大规模计算资源上运行良好，例如即将推出的千万亿次系统，那么研究人员将有可能扩展与日冕相关的多尺度物理问题的范围，例如日冕物质抛射，这些模型可以研究。 该项目是2006年春季“Petascale Computing and the Geosciences”研讨会所产生的一系列试点项目之一。 这些试点活动都与在地球科学的不同部分使用高性能计算建模有关，其目的是确定前沿地球科学研究中使用的模拟工具如何适用于未来几年将部署的超大规模计算系统。 这些分析的结果将在2006年秋季举行的关于“Petascale计算和地球科学”的第二次讲习班上讨论。 这个SGER项目涉及来自加州大学圣地亚哥分校（UCSD）的计算机科学家之间的合作，他们专门从事数值应用程序的详细分析和优化，和来自科学应用国际（SAIC）的空间物理学家参与了MAS的进一步发展，作为NSF活动的一部分，这项工作的更广泛影响来自于对一种工具的改进，这种工具可能对空间物理学研究和实用空间气象预报都有用。

This project is an exploratory activity intended to test the application of new expertise and techniques in performance modeling and optimization to the numerical simulation of the solar corona. It encompasses preliminary work to determine the feasibility of a future effort to develop a petascale version of the Magnetohydrodynamic Algorithm outside a Sphere model (MAS). If MAS and similar models can be adapted to run well on large-scale computational resources, such as forthcoming petascale systems, then it will be possible for researchers to extend the range of multi-scale physical problems associated with the solar corona, such as coronal mass ejections, that can be studied with these models. The project is one of a series of pilot projects spawned by a workshop on "Petascale Computing and the Geosciences" in Spring 2006. The purpose of these pilot activities, all related to the use of high-performance computational modeling in different parts of the geosciences, is to determine how the simulation tools used in leading-edge geoscience research can be adapted for the very large-scale computing systems that will be deployed in the next few years. The results of these analyses will be discussed at a second workshop on "Petascale Computing and the Geosciences" in Fall 2006. This SGER project involves a collaboration between computer scientists from University of California-San Diego (UCSD), who specialize in the detailed analysis and optimization of numerical applications, and space physicists from Science Application International (SAIC) involved in the further development of MAS as part of the activities of the NSF-funded Center for Integrated Space Weather Modeling.Broader impacts of this work stem from the improvement of a tool that is potentially useful for both space physics research and for operational space weather forecasting.