Collaborative Research: GEM--Radiation Belt Losses Using Combined Global Hybrid and Test Particle Simulations

Information

  • NSF Award
  • 2131013
Owner
  • Award Id
    2131013
  • Award Effective Date
    8/1/2021 - 3 years ago
  • Award Expiration Date
    7/31/2025 - 5 months from now
  • Award Amount
    $ 385,656.00
  • Award Instrument
    Standard Grant

Collaborative Research: GEM--Radiation Belt Losses Using Combined Global Hybrid and Test Particle Simulations

This award is funded in whole or in part under the American Rescue Plan Act of 2021 (Public Law 117-2). The radiation belts around the Earth consist mainly of relativistic particles that are trapped from the solar wind and cosmic rays. This region of space is extremely dynamic. In the inner magnetosphere, the part of the radiation belts closer to Earth, ultra-low frequency (ULF) waves play important roles in the acceleration and loss of particles. This project will investigate these processes with 3-D hybrid simulations combined with test-particle electron calculations, guided by multipoint space observations. Results will have broad application to understanding magnetospheres of the Earth and other planets. The work supports a Ph.D. student and two undergraduate students.<br/><br/>The project will establish the role of ULF waves, including electromagnetic ion cyclotron (EMIC) waves and kinetic Alfven waves (KAWs), in the radiation belt electron loss as well as electron radial diffusion. The science questions that will be answered include: (1) What internal or external processes control the generation and global structure, including ion wave-particle interactions, of EMIC waves and KAWs in the inner magnetosphere? How are EMIC/Alfven waves excited by localized injections from the tail or external compressions? (2) What are the transport coefficients of energetic electrons in these EMIC waves and KAWs, and what are the associated electron scattering and precipitation into the loss cone? (3) What are the effects of ULF waves and external compressional pulses on electron radial transport? The team will conduct relativistic test-particle electron calculations in 3-D global hybrid simulations. The hybrid models, describing fully kinetic ion physics, include an inner magnetospheric hybrid model in dipole geometry and the Auburn global hybrid code in 3-D (ANGIE3D) based on the self-consistent solar wind-magnetosphere interaction. The simulations will be validated with observations of the near-equatorial measurements from NOAA and NASA operated satellites and low-altitude measurements from satellites, CubeSats, and balloon experiments.<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
    7/20/2021 - 3 years ago
  • Max Amd Letter Date
    7/20/2021 - 3 years ago
  • ARRA Amount

Institutions

  • Name
    Andrews University
  • City
    Berrien Springs
  • State
    MI
  • Country
    United States
  • Address
    Andrews University
  • Postal Code
    491040670
  • Phone Number
    2694713100

Investigators

  • First Name
    Jay
  • Last Name
    Johnson
  • Email Address
    jrj@andrews.edu
  • Start Date
    7/20/2021 12:00:00 AM
  • First Name
    Eun-Hwa
  • Last Name
    Kim
  • Email Address
    ehkim@pppl.gov
  • Start Date
    7/20/2021 12:00:00 AM

Program Element

  • Text
    MAGNETOSPHERIC PHYSICS
  • Code
    5750

Program Reference

  • Text
    COVID-Disproportionate Impcts Inst-Indiv