FDSS: Solar and Space Physics Development at the Institute for Astronomy

FDSS：天文学研究所的太阳和空间物理发展

• 批准号: 1936393
• 负责人: Shadia Habbal
• 金额: $ 150万
• 依托单位: University of Hawaii
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2020
• 资助国家: 美国
• 起止时间: 2020-01-01 至 2024-12-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1936393&HistoricalAwards=false
• 关键词: FDSS; Solar; Space; Physics; Development

The goal of this Faculty Development in Space Science (FDSS) project is to enable a new faculty hire in solar-heliospheric physics at the Institute for Astronomy (IfA) of the University of Hawaii (UH). The IfA is heavily involved in experimental, observational, data analysis, and modeling investigations of the magnetized solar atmosphere of the Sun, starting from the solar surface and expanding outwards to form the solar corona and the solar wind. The solar program at the IfA, which focuses on a critical-mass faculty and a recently growing number of graduate and undergraduate students engaged in solar research, is designed to have a broad educational impact as we develop a premier center for solar and space physics education in the U.S. The UH is a minority serving higher education institution. This 5-year FDSS program will have a significant impact on UH's undergraduate as well as graduate programs. The engagement of solar faculty in the undergraduate program gives them direct access to a highly diverse group of students, with significant representation from minorities and under-represented groups. Direct involvement with the IfA's graduate program, together with plans for a new graduate course in solar and heliospheric physics, solar faculty can engage graduates in the different aspects of solar research, ranging from instrumentation, to DKIST, data analysis and modeling. In the past, the IfA's solar research programs in Manoa and Haleakala have demonstrated major breakthroughs for advancing our understanding of the structure and dynamics of the solar corona and solar wind. By capitalizing on their unique expertise, members of the solar group at the IfA are engaged in exploring the different facets of solar magnetism, and its role in the dynamics of the Sun's atmosphere. With the advent of the Daniel K. Inouye Solar Telescope (DKIST) first light in 2020, and with the two first light instruments being designed and built by two members of the group, the IfA's solar group is in an enviable position to achieve excellence. It is within this environment that this group is receiving NSF's support to expand its diversity and synergy by complementing their strength with a junior faculty appointment with expertise in modeling and/or theory. This opportunity comes at an ideal time not only for individual success, but also for the IfA's solar physics graduate education program, which has been expanding markedly over the past two years. Hawaii scientists are also in an enviable position of having 12.5% guaranteed observing time on DKIST, a priceless commodity for propelling the success of the new faculty. The research and EPO agenda of this 5-year FDSS project supports the Strategic Goals of the AGS Division in discovery, learning, diversity, and interdisciplinary research.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.

这项空间科学教师发展（FDSS）项目的目的是在夏威夷大学（UH）的天文学研究所（IFA）的太阳能物理学中获得新的教师雇用。 IFA大量参与了实验，观察性，数据分析以及对太阳磁化太阳大气的建模研究，从太阳能表面开始，然后向外扩展，形成太阳能电晕和太阳风。 IFA的太阳能计划侧重于关键质量的教师以及最近不断增长的太阳能研究的研究生和本科生，旨在在美国开发一个高级太阳能和太空物理教育中心，在美国，UH是UH，UH是少数为高等教育机构服务的。 这个为期5年的FDSS计划将对UH的本科和研究生课程产生重大影响。 太阳能教师参与本科课程，使他们可以直接访问一群高度多样化的学生，并从少数群体和代表性不足的群体中获得了重大代表。 直接参与IFA的研究生课程，以及在太阳能和地球物理学的新研究生课程的计划中，太阳能教师可以使毕业生参与太阳能研究的不同方面，从仪器到DKIST，数据分析和建模。 过去，IFA在MANOA和HAEAKALA的太阳能研究计划展示了我们对太阳电晕和太阳风的结构和动态的理解的重大突破。 通过利用其独特的专业知识，IFA太阳能集团的成员参与了探索太阳能磁性的不同方面及其在太阳气氛的动态中的作用。 随着丹尼尔·伊诺耶（Daniel K. Inouye）太阳能望远镜（DKIST）在2020年的出现，并由该集团的两个成员设计和建造两种第一灯仪器，IFA的太阳能集团处于令人羡慕的位置，可以取得卓越的成就。 正是在这种环境中，该小组通过通过在建模和/或理论方面具有专业知识的初级教师任命来补充其实力，从而获得NSF的支持，以扩大其多样性和协同作用。 这个机会不仅是个人成功的理想时间，而且是IFA太阳能物理学教育计划的理想时间，在过去的两年中，该计划一直在显着扩展。 夏威夷的科学家们也处于令人羡慕的地位，拥有12.5％的保证在DKIST上观察时间，DKIST是一种无价的商品，用于推动新教师的成功。 这个为期5年的FDSS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。该奖项反映了NSF的法定任务，并被认为是值得通过基金会的知识分子优点和更广泛影响的审查标准来通过评估来获得支持的。

项目成果

Ion Acceleration Efficiency at the Earth’s Bow Shock: Observations and Simulation Results

地球弓形激波的离子加速效率：观测和模拟结果

• DOI: 10.3847/1538-4357/abfafc
• 发表时间: 2021
• 期刊: The Astrophysical Journal
• 作者: Johlander, A.;Battarbee, M.;Vaivads, A.;Turc, L.;Pfau-Kempf, Y.;Ganse, U.;Grandin, M.;Dubart, M.;Khotyaintsev, Yu. V.;Caprioli, D.
• 通讯作者: Caprioli, D.

Spatial evolution of magnetic reconnection diffusion region structures with distance from the X-line

磁重联扩散区结构随距 X 线距离的空间演化

• DOI: 10.1063/5.0072182
• 发表时间: 2021
• 期刊: Physics of Plasmas
• 影响因子: 2.2
• 作者: Øieroset, M.;Phan, T. D.;Ergun, R.;Ahmadi, N.;Genestreti, K.;Drake, J. F.;Liu, Y.-H.;Haggerty, C.;Eastwood, J. P.;Shay, M. A.
• 通讯作者: Shay, M. A.

The Theory of Efficient Particle Acceleration at Shocks

冲击时有效粒子加速理论

• DOI: 10.22323/1.395.0482
• 发表时间: 2021
• 期刊: 37th International Cosmic Ray Conference (ICRC2021
• 作者: Caprioli, Damiano;Haggerty, Colby;Blasi, Pasquale
• 通讯作者: Blasi, Pasquale

Cosmic-ray generated bubbles around their sources

宇宙射线在其源头周围产生气泡

• DOI: 10.1093/mnras/stac466
• 发表时间: 2022
• 期刊: Monthly Notices of the Royal Astronomical Society
• 影响因子: 4.8
• 作者: Schroer, B.;Pezzi, O.;Caprioli, D.;Haggerty, C. C.;Blasi, P.
• 通讯作者: Blasi, P.

Relativistic Asymmetric Magnetic Reconnection

相对论不对称磁重联

• DOI: 10.1103/physrevlett.128.145101
• 发表时间: 2022
• 期刊: Physical Review Letters
• 影响因子: 8.6
• 作者: Mbarek, Rostom;Haggerty, Colby;Sironi, Lorenzo;Shay, Michael;Caprioli, Damiano
• 通讯作者: Caprioli, Damiano