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SHINE: Solar Energetic Particles Mediating Interplanetary Shocks Close to the Sun

SHINE: Solar Energetic Particles Mediating Interplanetary Shocks Close to the Sun
闪耀:太阳高能粒子介导靠近太阳的行星际激波
批准号:
2401162
负责人:
Parisa Mostafavi
金额:
$57.97万
依托单位:
依托单位国家:
美国
项目类别:
Continuing Grant
财政年份:
2024
资助国家:
美国
项目状态:
未结题
起止时间:
2024-03-01 至 2027-02-28

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英文摘要
Solar energetic particles (SEPs) are high-energy particles that can propagate from the Sun all the way to the surface of the Earth, which can cause significant disruptions to communication systems. Their generation mechanisms remain a subject of much debate, with strong coronal and interplanetary discontinuities or shocks driven by coronal mass ejections (CME) being likely responsible. Previous observations studied these shocks at different solar distances from the Earth’s orbit to the outer heliosphere, but were limited to distances mostly outside the Earth’s orbit (1 au). Currently, however, observations with Parker Solar Probe (PSP) and Solar Orbiter (SolO) allow us to build a more complete picture by probing extensively distances below 1 au. A key consequence of studying this region, which is the goal of this project, is that these in-situ observations will provide SEP and shock measurements that are dramatically less affected by transport effects as the spacecraft progressively get closer to the Sun.The data from PSP and SolO will be analyzed for periods when these spacecraft observe shock events with exceptionally high SEP intensities. The results will address the significant issue of energetic particle acceleration by shocks near the Sun and how the particles affect the structure of these young shocks. Additionally, as energetic-particle-mediated shocks are predicted to occur in various astrophysical settings across a broad range of spatial and temporal scales, our comprehensive search for such structures very close to our Sun may fundamentally contribute to our understanding of well-known ‘cosmic ray’-mediated collisionless shocks. The science goals of this project are to (1) quantify SEP-mediated shocks, (2) assess SEP impact on shock mediation, and (3) explore shock-SEP relationships. This project will support an early-career female scientist and an undergraduate student from the APL CIRCUIT Program to work on this project which will be promoting research and education.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.
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海外基金
基于“夸父一号”HXI载荷和Solar Orbiter /STIX的耀斑X射线暴多视角观测及研究
  • 批准号:
    12303063
  • 项目类别:
    青年科学基金项目
  • 资助金额:
    30万元
  • 批准年份:
    2023
  • 负责人:
    夏凡小雨
  • 依托单位: