Solar Heliospheric and INterplanetary Environment (SHINE) Workshop, 2023-2027
太阳日光层和行星际环境 (SHINE) 研讨会,2023-2027
基本信息
- 批准号:2313220
- 负责人:
- 金额:$ 162.9万
- 依托单位:
- 依托单位国家:美国
- 项目类别:Continuing Grant
- 财政年份:2023
- 资助国家:美国
- 起止时间:2023-05-01 至 2028-04-30
- 项目状态:未结题
- 来源:
- 关键词:
项目摘要
Solar Heliospheric and INterplanetary Environment (SHINE) is an affiliation of researchers within the solar, interplanetary, and heliospheric communities, dedicated to promoting an enhanced understanding of the processes by which energy in the form of magnetic fields and particles are produced by the Sun and/or accelerated in interplanetary space, and on the mechanisms by which these fields and particles are transported to the Earth and elsewhere in the heliosphere. This project continues the highly successful series of SHINE workshops for the next five years; SHINE workshops have been held annually since 1995 and annually as stand-alone meetings since 1999. The SHINE workshop has a strong participation by students and post-doctoral researchers, representing about 30% of the whole participant population. SHINE students supported by NSF funding have been organizing a student-only student day on the Sunday preceding the workshop, which will continue with this award. Overall, SHINE provides a unique opportunity for students to participate and organize a workshop in the solar, interplanetary and heliospheric communities. SHINE research focuses in particular upon: (i) the connection between events and phenomena on the Sun and their relation to solar wind structures in the heliosphere; (ii) the origin and evolution of the solar wind; (iii) the nature of turbulence in the interplanetary medium; and (iv) the production and transport of solar energetic particles from the Sun through the heliosphere. The goal of SHINE activities is to enrich and strengthen both the physical understanding and predictive capabilities for these phenomena. Further details about SHINE can be found at http://www.helioshine.org/. The goals of SHINE are parallel to those of NSF’s GEM and CEDAR programs. This project will contribute in creating collaborations between researchers to move towards more advanced studies of the solar-terrestrial system. These collaborations made possible by the workshop are expected to improve our present understanding of the basic physical processes underlying the Sun-Earth system.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.
太阳日光层和行星际环境(SHINE)是太阳,行星际和日光层社区内研究人员的一个附属机构,致力于促进对太阳产生和/或在行星际空间加速的磁场和粒子形式的能量过程的深入了解,以及这些场和粒子被输送到地球和日光层其他地方的机制。该项目在今后五年里继续举办一系列非常成功的“特别行动倡议”讲习班;自1995年以来,“特别行动倡议”讲习班每年举行一次,自1999年以来,每年单独举行一次。SHINE研讨会有学生和博士后研究人员的强烈参与,约占整个参与者人口的30%。由NSF资助的SHINE学生在研讨会之前的星期天组织了一个学生专用的学生日,该研讨会将继续颁发该奖项。总的来说,SHINE为学生提供了一个独特的机会,让他们参与并组织太阳能,行星际和日光层社区的研讨会。太阳能研究所的研究特别侧重于:㈠太阳上的事件和现象之间的联系及其与日光层中太阳风结构的关系; ㈡太阳风的起源和演变; ㈢行星际介质中湍流的性质; ㈣太阳高能粒子的产生和从太阳通过日光层的传输。SHINE活动的目标是丰富和加强对这些现象的物理理解和预测能力。有关SHINE的更多详细信息,请访问http://www.helioshine.org/。SHINE的目标与NSF的GEM和CEDAR计划的目标是平行的。该项目将有助于在研究人员之间建立合作关系,以便对日地系统进行更深入的研究。通过研讨会,这些合作成为可能,预计将提高我们目前对太阳-地球系统的基本物理过程的理解。这个奖项反映了NSF的法定使命,并已被认为是值得通过使用基金会的智力价值和更广泛的影响审查标准进行评估的支持。
项目成果
期刊论文数量(0)
专著数量(0)
科研奖励数量(0)
会议论文数量(0)
专利数量(0)
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Nada Al-Haddad其他文献
The Magnetic Field Structure of Coronal Mass Ejections: A More Realistic Representation
日冕物质抛射的磁场结构:一种更现实的表示
- DOI:
10.1007/s11214-025-01138-w - 发表时间:
2025-02-01 - 期刊:
- 影响因子:7.400
- 作者:
Nada Al-Haddad;Noé Lugaz - 通讯作者:
Noé Lugaz
The Need for Near-Earth Multi-Spacecraft Heliospheric Measurements and an Explorer Mission to Investigate Interplanetary Structures and Transients in the Near-Earth Heliosphere
- DOI:
10.1007/s11214-024-01108-8 - 发表时间:
2024-09-20 - 期刊:
- 影响因子:7.400
- 作者:
Noé Lugaz;Christina O. Lee;Nada Al-Haddad;Robert J. Lillis;Lan K. Jian;David W. Curtis;Antoinette B. Galvin;Phyllis L. Whittlesey;Ali Rahmati;Eftyhia Zesta;Mark Moldwin;Errol J. Summerlin;Davin E. Larson;Sasha Courtade;Richard French;Richard Hunter;Federico Covitti;Daniel Cosgrove;J. D. Prall;Robert C. Allen;Bin Zhuang;Réka M. Winslow;Camilla Scolini;Benjamin J. Lynch;Rachael J. Filwett;Erika Palmerio;Charles J. Farrugia;Charles W. Smith;Christian Möstl;Eva Weiler;Miho Janvier;Florian Regnault;Roberto Livi;Teresa Nieves-Chinchilla - 通讯作者:
Teresa Nieves-Chinchilla
Nada Al-Haddad的其他文献
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{{ truncateString('Nada Al-Haddad', 18)}}的其他基金
Improving Models to Better Represent the Complex Structure of Coronal Mass Ejections
改进模型以更好地表示日冕物质抛射的复杂结构
- 批准号:
1954983 - 财政年份:2021
- 资助金额:
$ 162.9万 - 项目类别:
Standard Grant
EAGER: Developing an Ab initio Model of Coronal Mass Ejections (CMEs) Incorporating All Forms of Helicity
EAGER:开发包含所有形式螺旋度的日冕物质抛射 (CME) 从头算模型
- 批准号:
2027322 - 财政年份:2020
- 资助金额:
$ 162.9万 - 项目类别:
Standard Grant
相似海外基金
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职业:理解无碰撞磁重联作为基本的日光层过程
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2338131 - 财政年份:2024
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Heliospheric and Planetary Research 2023-2026
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职业:使用多航天器数据和机器学习的基于端对端活动区域的日光层预报系统
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2240022 - 财政年份:2023
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中央兰开夏大学综合太阳和日光层物理研究
- 批准号:
ST/V000934/1 - 财政年份:2021
- 资助金额:
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- 批准号:
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REU Site: Solar and Heliospheric Physics at University of Alabama in Huntsville (UAH) and Marshall Space Flight Center (MSFC)
REU 站点:亨茨维尔阿拉巴马大学 (UAH) 和马歇尔太空飞行中心 (MSFC) 的太阳和日光层物理中心
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- 批准号:
2019828 - 财政年份:2020
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Fellowship Award
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- 资助金额:
$ 162.9万 - 项目类别:
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日光层边界区域多组分等离子体的能量分配机制
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17K05666 - 财政年份:2017
- 资助金额:
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