skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Event study of deep energetic particle injections during substorm

Journal Article · · Journal of Geophysical Research
DOI:https://doi.org/10.1029/97JA03686· OSTI ID:678747

The origin of multiple energetic particle injections into the inner magnetosphere is addressed using a rare opportunity of measuring the energetic particle fluxes at different radial distances under known electric and magnetic fields. During a strong substorm on February 10, 1991, the CRRES spacecraft measured {ital E} and {ital B} fields and high-energy particle fluxes near the magnetic equator at r{approximately}5R{sub e}, whereas particle injections, their azimuthal locations, and some other parameters were simultaneously monitored by three geostationary spacecraft and ground networks. We show a multitude of impulsive short-duration injection events which correlate with 1{endash}2 min long pulses of dawn-dusk electric field. The observations suggest that some {ital E} field pulses recorded deep in the inner magnetosphere were fast magnetosonic waves radiated by the current disruption region. This supports the concept of impulsive dissipation event as an elementary building block of substorm expansion. Furthermore, our modeling results indicate that most of the flux variations of energetic particles can be explained by the global convective transport and corresponding particle acceleration. However, we emphasize that, depending on particle spectra and radial flux gradient, one can observe either flux increase, or decrease, or no variation (often seen in different energy ranges simultaneously and at the same point) as a response to the electric field pulse. Both the cloud of injected particles and magnetic field dipolarization region had a sharp inner boundary (injection front) which propagated inward at the convection speed. We document the complicated structure of this front, consisting of a diamagnetic hot proton layer followed by the dipolarization front which contains enhanced energetic electron fluxes. Further study is required to understand how common this structure is and, if common, how it may be formed. {copyright} 1998 American Geophysical Union

OSTI ID:
678747
Journal Information:
Journal of Geophysical Research, Vol. 103, Issue A5; Other Information: PBD: May 1998
Country of Publication:
United States
Language:
English

Similar Records

Geotail observations of substorm onset in the inner magnetotail
Journal Article · Thu Jan 01 00:00:00 EST 1998 · Journal of Geophysical Research · OSTI ID:678747

Longitudinal structure of substorm injections at synchronous orbit
Journal Article · Mon Aug 01 00:00:00 EDT 1983 · J. Geophys. Res.; (United States) · OSTI ID:678747

Midtail plasma flows and the relationship to near-Earth substorm activity: A case study
Journal Article · Thu Dec 01 00:00:00 EST 1994 · Journal of Geophysical Research · OSTI ID:678747