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

Information

  • NSF Award
  • 2401162
Owner
  • Award Id
    2401162
  • Award Effective Date
    3/1/2024 - 2 months ago
  • Award Expiration Date
    2/28/2027 - 2 years from now
  • Award Amount
    $ 186,527.00
  • Award Instrument
    Continuing Grant

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

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.<br/><br/>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.<br/><br/>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.

  • Program Officer
    Lisa Winterlwinter@nsf.gov7032928519
  • Min Amd Letter Date
    2/5/2024 - 2 months ago
  • Max Amd Letter Date
    2/5/2024 - 2 months ago
  • ARRA Amount

Institutions

  • Name
    Johns Hopkins University
  • City
    BALTIMORE
  • State
    MD
  • Country
    United States
  • Address
    3400 N CHARLES ST
  • Postal Code
    212182608
  • Phone Number
    4439971898

Investigators

  • First Name
    Matthew
  • Last Name
    Hill
  • Email Address
    matt.hill@jhuapl.edu
  • Start Date
    2/5/2024 12:00:00 AM
  • First Name
    Parisa
  • Last Name
    Mostafavi
  • Email Address
    Parisa.Mostafavi@jhuapl.edu
  • Start Date
    2/5/2024 12:00:00 AM
  • First Name
    Athanasios
  • Last Name
    Kouloumvakos
  • Email Address
    Athanasios.Kouloumvakos@jhuapl.edu
  • Start Date
    2/5/2024 12:00:00 AM

Program Element

  • Text
    SOLAR-TERRESTRIAL
  • Code
    1523