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.

这个空间科学教师发展项目的目标是使夏威夷大学天文学研究所（IfA）能够聘用一名太阳日光层物理学教师。 IfA积极参与太阳磁化太阳大气的实验、观测、数据分析和建模研究，从太阳表面开始，向外扩展，形成日冕和太阳风。 在IfA的太阳能计划，重点是临界质量的教师和最近越来越多的研究生和本科生从事太阳能研究，旨在有广泛的教育影响，因为我们开发了太阳能和空间物理教育的首要中心在美国UH是少数服务于高等教育机构。 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。 太阳能教师在本科课程的参与使他们能够直接接触到高度多样化的学生群体，其中少数民族和代表性不足的群体具有重要的代表性。 直接参与IfA的研究生课程，以及太阳和日光层物理学新研究生课程的计划，太阳能教师可以让毕业生参与太阳研究的不同方面，从仪器仪表到DKIST，数据分析和建模。 在过去，IfA在马诺阿和哈雷阿卡拉的太阳研究计划已经证明了重大突破，促进了我们对日冕和太阳风的结构和动力学的理解。 通过利用他们独特的专业知识，IfA太阳能小组的成员正在探索太阳磁场的不同方面，以及它在太阳大气动力学中的作用。 随着丹尼尔K. Inouye太阳望远镜（DKIST）将于2020年首次亮相，随着该集团两名成员设计和建造的两台首批照明仪器，IfA的太阳能集团处于令人羡慕的位置，以实现卓越。 正是在这种环境下，这个小组正在接受NSF的支持，以扩大其多样性和协同作用，通过补充他们的力量与初级教师任命与建模和/或理论的专业知识。 这个机会不仅是个人成功的理想时机，也是IfA太阳物理研究生教育计划的理想时机，该计划在过去两年中显着扩大。 夏威夷的科学家们也处于令人羡慕的地位，他们在DKIST上有12.5%的保证观测时间，这是推动新教师成功的无价商品。 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。这个奖项反映了NSF的法定使命，并通过使用基金会的知识价值和更广泛的影响审查标准进行评估，被认为值得支持。

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