Collaborative Research: Frameworks: A Software Ecosystem for Plasma Science and Space Weather Applications

合作研究:框架:等离子体科学和空间天气应用的软件生态系统

基本信息

  • 批准号:
    2209471
  • 负责人:
  • 金额:
    $ 200.44万
  • 依托单位:
  • 依托单位国家:
    美国
  • 项目类别:
    Standard Grant
  • 财政年份:
    2022
  • 资助国家:
    美国
  • 起止时间:
    2022-07-15 至 2027-06-30
  • 项目状态:
    未结题

项目摘要

This project advances the frontiers of global simulations of space and laboratory plasma systems, and makes these advances accessible to a broad community of users. The plasma states in such systems are often in weakly collisional regimes where traditional fluid models break down. To describe such systems, the project team is developing Gkeyll, a multi-fluid, multi-moment model that incorporates important kinetic effects. The model can be used for high-fidelity and accurate predictions for space weather events, and for the design and study of laboratory experiments engaged in discovery plasma science. The project will develop comprehensive cyberinfrastructure (CI) to support professional scientists in the execution of space weather and basic plasma physics simulations over a wide variety of computing platforms from local clusters to high-performance computing facilities. Gkeyll CI to be developed includes (1) providing web-based user interfaces for defining, executing, and managing simulations, (2) workflows consisting of of pre-defined sequences of tasks, and (3) user-friendly tools that implement the workflow tasks. Gkeyll science will be facilitated by algorithmic advances. Gkeyll is open-source and provides the space and laboratory plasma science communities with a modern and versatile software ecosystem. The project team is strongly interdisciplinary, including space and laboratory plasma scientists, applied mathematicians, computer scientists and software engineers, and the project will promote diversity in professional training and education.The CI to be built in the project is centered on the Gkeyll framework that consists of advanced plasma simulation models, tools, and automated continuous integration of new software. The project will provide a uniform and complete open-source solution with workflow control to model plasma systems from terrestrial magnetospheres to laboratory experiments in collisionless or weakly collisional plasma regimes, which are essential for space weather and laboratory plasma experiments. The project will extend and enhance the core algorithms in Gkeyll and integrate the software with the NSF Science Gateway Platform as a Service (SciGaP). Gkeyll science is facilitated by core modeling and PDE discretization advances, including automated and adaptive gridding for relevant sets of parameterized geometries that are properly matched to the equation discretization methods. The project will employ modern software engineering practices to produce scalable, secure, and high-fidelity physics-based software.This award by the Office of Advanced Cyberinfrastructure is jointly supported by the Division of Physics within the NSF Directorate for Mathematical and Physical Sciences, and the Division of Atmospheric and Geospace Sciences and the Division of Research, Innovation, Synergies, and Education within the NSF Directorate for Geosciences.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.
该项目推动了全球对太空和实验室等离子体系统的模拟的前沿,并使广泛的用户社区可以实现这些进步。这种系统中的等离子体状态通常处于传统流体模型破裂的微弱碰撞状态。为了描述这样的系统,项目团队正在开发Gkeyll,这是一种多流体,多功能模型,结合了重要的动力学效果。该模型可用于对太空天气事件的高保真和准确的预测,以及从事发现等离子体科学的实验室实验的设计和研究。该项目将开发全面的网络基础设施(CI),以支持专业科学家在太空天气和基本等离子体物理模拟的执行,从本地群集到高性能计算设施的各种计算平台。要开发的Gkeyll CI包括(1)提供基于Web的用户接口,用于定义,执行和管理模拟,(2)由预定义的任务序列组成的工作流以及(3)实现工作流任务的用户友好工具。 Gkeyll科学将通过算法进步来促进。 Gkeyll是开源的,并为空间和实验室等离子科学社区提供了现代和多功能的软件生态系统。该项目团队是强烈的跨学科,包括太空和实验室等离子体科学家,应用数学家,计算机科学家和软件工程师,该项目将促进专业培训和教育方面的多样性。该项目中构建的CI集中在Gkeyll框架上,该框架由高级等离子体模拟模型,工具,工具,工具,持续整合的新软件组成。该项目将通过工作流控制提供统一而完整的开源解决方案,以模拟从地面磁层到实验室实验的等离子体系统,这对于空间天气和实验室血浆实验至关重要。该项目将扩展和增强Gkeyll中的核心算法,并将软件与NSF Science Gateway平台作为服务(SCIGAP)集成在一起。 Gkeyll科学通过核心建模和PDE离散化进步来促进,包括与方程离散方法正确匹配的相关几何形状集的自动和自适应网格。 The project will employ modern software engineering practices to produce scalable, secure, and high-fidelity physics-based software.This award by the Office of Advanced Cyber​​infrastructure is jointly supported by the Division of Physics within the NSF Directorate for Mathematical and Physical Sciences, and the Division of Atmospheric and Geospace Sciences and the Division of Research, Innovation, Synergies, and Education within the NSF Directorate for Geosciences.This award反映了NSF的法定任务,并使用基金会的知识分子优点和更广泛的影响审查标准来评估值得支持。

项目成果

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Amitava Bhattacharjee其他文献

Statistical simulation of the magnetorotational dynamo.
磁旋转发电机的统计模拟。
  • DOI:
    10.1103/physrevlett.114.085002
  • 发表时间:
    2014
  • 期刊:
  • 影响因子:
    8.6
  • 作者:
    Jonathan Squire;Amitava Bhattacharjee
  • 通讯作者:
    Amitava Bhattacharjee
Plasmoid-mediated reconnection during nonlinear peeling–ballooning edge-localized modes
非线性剥离-气球边缘局部模式期间等离子体介导的重连接
  • DOI:
    10.1088/1741-4326/ad0062
  • 发表时间:
    2021
  • 期刊:
  • 影响因子:
    3.3
  • 作者:
    F. Ebrahimi;Amitava Bhattacharjee
  • 通讯作者:
    Amitava Bhattacharjee
Kolmogorov versus Iroshnikov-Kraichnan spectra: Consequences for ion heating in the solar wind
柯尔莫哥洛夫光谱与 Iroshnikov-Kraichnan 光谱:太阳风中离子加热的后果
  • DOI:
    10.1029/2009ja014377
  • 发表时间:
    2007
  • 期刊:
  • 影响因子:
    0
  • 作者:
    C. Ng;Amitava Bhattacharjee;D. Munsi;P. Isenberg;Charles W. Smith
  • 通讯作者:
    Charles W. Smith
Overview of NSTX Upgrade initial results and modelling highlights
NSTX Upgrade 初步结果和建模亮点概述
  • DOI:
  • 发表时间:
    2017
  • 期刊:
  • 影响因子:
    0
  • 作者:
    J. Menard;Jean P. Allain;D. Battaglia;F. Bedoya;R. Bell;Elena Belova;J. Berkery;M. Boyer;N. Crocker;A. Diallo;F. Ebrahimi;Nathaniel Ferraro;E. Fredrickson;H. Frerichs;S. Gerhardt;N. Gorelenkov;W. Guttenfelder;W. Heidbrink;R. Kaita;S. Kaye;D. Kriete;S. Kubota;B. LeBlanc;D. Liu;R. Lunsford;D. Mueller;Clayton E. Myers;M. Ono;Jinseop Park;Mario Podesta;R. Raman;Matthew Reinke;Y. Ren;S. Sabbagh;O. Schmitz;F. Scotti;Y. Sechrest;C. H. Skinner;D. R. Smith;V. Soukhanovskii;T. Stoltzfus;H. Yuh;Zhirui Wang;I. Waters;J. Ahn;R. Andre;R. Barchfeld;P. Beiersdorfer;N. Bertelli;Amitava Bhattacharjee;D. Brennan;R. Buttery;A. Capece;G. Canal;John Canik;C. S. Chang;D. Darrow;L. Delgado;C. Domier;S. Ethier;T. Evans;J. Ferron;M. Finkenthal;R. Fonck;K. Gan;D. Gates;I. Goumiri;T. Gray;J. Hosea;D. Humphreys;T. Jarboe;S. Jardin;Michael Jaworski;B. Koel;E. Kolemen;S. Ku;R. L. Haye;F. Levinton;N. C. Luhmann;R. Maingi;R. Maqueda;G. Mckee;E. Meier;J. Myra;R. Perkins;F. Poli;T. Rhodes;J. Riquezes;C. Rowley;D. Russell;Eugenio Schuster;B. Stratton;D. Stutman;Gary Taylor;K. Tritz;W. Wang;B. Wirth;S. Zweben
  • 通讯作者:
    S. Zweben
Helicity-flux-driven α effect in laboratory and astrophysical plasmas.
实验室和天体物理等离子体中螺旋通量驱动的 α 效应。
  • DOI:
  • 发表时间:
    2014
  • 期刊:
  • 影响因子:
    8.6
  • 作者:
    F. Ebrahimi;Amitava Bhattacharjee
  • 通讯作者:
    Amitava Bhattacharjee

Amitava Bhattacharjee的其他文献

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{{ truncateString('Amitava Bhattacharjee', 18)}}的其他基金

WoU-MMA: Role of the Dynamo Effect in Neutron Star Mergers
WoU-MMA:发电机效应在中子星合并中的作用
  • 批准号:
    2206756
  • 财政年份:
    2022
  • 资助金额:
    $ 200.44万
  • 项目类别:
    Standard Grant
Collaborative Research: Integration of Extended Magnetohydrodynamic (MHD) and Kinetic Effects in Global Magnetosphere Models
合作研究:全球磁层模型中扩展磁流体动力学 (MHD) 和动力学效应的集成
  • 批准号:
    1552142
  • 财政年份:
    2014
  • 资助金额:
    $ 200.44万
  • 项目类别:
    Continuing Grant
Collaborative Research: Integration of Extended Magnetohydrodynamic (MHD) and Kinetic Effects in Global Magnetosphere Models
合作研究:全球磁层模型中扩展磁流体动力学 (MHD) 和动力学效应的集成
  • 批准号:
    1338944
  • 财政年份:
    2013
  • 资助金额:
    $ 200.44万
  • 项目类别:
    Continuing Grant
SHINE: Instability of Large-Scale Current Sheets, Plasmoid Formation, and Particle Acceleration in Coronal Plasmas
SHINE:大尺度电流片的不稳定性、等离子体团的形成以及日冕等离子体中的粒子加速
  • 批准号:
    1331784
  • 财政年份:
    2013
  • 资助金额:
    $ 200.44万
  • 项目类别:
    Continuing Grant
Collaborative Research: Integration of Extended Magnetohydrodynamic (MHD) and Kinetic Effects in Global Magnetosphere Models
合作研究:全球磁层模型中扩展磁流体动力学 (MHD) 和动力学效应的集成
  • 批准号:
    1338863
  • 财政年份:
    2013
  • 资助金额:
    $ 200.44万
  • 项目类别:
    Continuing Grant
SHINE: Instability of Large-Scale Current Sheets, Plasmoid Formation, and Particle Acceleration in Coronal Plasmas
SHINE:大尺度电流片的不稳定性、等离子体团的形成以及日冕等离子体中的粒子加速
  • 批准号:
    0962698
  • 财政年份:
    2010
  • 资助金额:
    $ 200.44万
  • 项目类别:
    Continuing Grant
Stability of Thin Current Sheet in the Magnetotail: Theory, Simulations, and Observations
磁尾中薄电流片的稳定性:理论、模拟和观察
  • 批准号:
    0903915
  • 财政年份:
    2009
  • 资助金额:
    $ 200.44万
  • 项目类别:
    Standard Grant
GEM: Can Global Magnetohydrodynamics (MHD) Codes Model Magnetic Reconnection in the High Lundquist Number Limit?
GEM:全球磁流体动力学 (MHD) 代码能否模拟高伦德奎斯特数限制下的磁重联?
  • 批准号:
    0802727
  • 财政年份:
    2008
  • 资助金额:
    $ 200.44万
  • 项目类别:
    Continuing Grant
Collaborative Research: Global Simulations of Substorm Trigger with GGCM: Synergistic Coupling of Magnetic Reconnection and Ballooning-Interchange Instabilities in the Magnetotail
合作研究:使用 GGCM 对亚暴触发进行全局模拟:磁尾磁重联和气球交换不稳定性的协同耦合
  • 批准号:
    0543202
  • 财政年份:
    2006
  • 资助金额:
    $ 200.44万
  • 项目类别:
    Continuing Grant
Stability of Thin Current Sheets in the Earth's Magnetotail: Theory, Simulations, and Observations
地球磁尾中薄电流片的稳定性:理论、模拟和观测
  • 批准号:
    0425806
  • 财政年份:
    2004
  • 资助金额:
    $ 200.44万
  • 项目类别:
    Continuing Grant

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Collaborative Research: Frameworks: MobilityNet: A Trustworthy CI Emulation Tool for Cross-Domain Mobility Data Generation and Sharing towards Multidisciplinary Innovations
协作研究:框架:MobilityNet:用于跨域移动数据生成和共享以实现多学科创新的值得信赖的 CI 仿真工具
  • 批准号:
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合作研究:用于分离应用的大面积金属有机框架薄膜的可扩展制造
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