Edinburgh Research Explorer

On Modeling the April 21, 2002 SEP event

Research output: Contribution to conferencePaper

  • G. Li
  • G. P. Zank
  • W. K. Rice
  • G. M. Mason
  • M. I. Desai
  • R. Mewaldt
  • C. M. Cohen
  • M. D. Looper

Related Edinburgh Organisations

Original languageEnglish
Pages433
StatePublished - 1 Dec 2002
EventAmerican Geophysical Union, Fall Meeting 2002 - , United Kingdom
Duration: 6 Dec 200210 Dec 2002

Conference

ConferenceAmerican Geophysical Union, Fall Meeting 2002
CountryUnited Kingdom
Period6/12/0210/12/02

Abstract

Gradual solar energetic particle (SEP) events, where particles are often accelerated to 10's MeV (sometimes even GeV) energies, are often associated with CME-driven shocks. Thus, interpreting the observational data requires understanding the structure of the shock, the acceleration process, and the subsequent transport of energetic particles. Theoretically, the underlying acceleration mechanism is thought to be first-order Fermi acceleration, also known as diffusive shock acceleration. Such a mechanism leads naturally to power-law particle spectra, which are often observed. To connect observations with the underlying theory, a comprehensive model that tracks particle acceleration and transport is necessary. In this work, we describe our model of particle acceleration and transport at CME-driven shocks and compare the model simulation with a particular event - the April 21st, 2002 event. We chose this event for its relatively clean intensity-time profile which is relatively free of contributions from other events. The parent shock is thought to be driven by a CME associated with active region 9906 (S03 W56) and was magnetically well connected to Earth. Velocity dispersion observed during the onset of the event is a signature of particles being accelerated near the Sun and their subsequent transport through the interplanetary medium to 1 AU. In this work, we have modeled the intensity-time profiles and particle energy spectra obtained over a broad range of energies between ~ 0.08~MeV/nucleon through ~ 100~MeV/nucleon from instruments on ACE, Wind, and SAMPEX. We find excellent agreement between our model simulations and the observations, suggesting that this approach may provide an important step toward understanding and tracking the influence of large SEP events in the interplanetary and geospace environments.

    Research areas

  • 2118 Energetic particles, solar, 7513 Coronal mass ejections, 7803 Active perturbation experiments, 7851 Shock waves

Event

American Geophysical Union, Fall Meeting 2002

6/12/0210/12/02

United Kingdom

Event: Conference

ID: 19679600