A MODEL OF ACCELERATION OF ANOMALOUS COSMIC RAYS BY RECONNECTION IN THE HELIOSHEATH
- Department of Astronomy, University of Wisconsin, Madison, WI 53706 (United States)
- Department of Physics and Astronomy, George Mason University, 4400 University Drive, Fairfax, VA 22030 (United States)
We discuss a model of cosmic ray acceleration that accounts for the observations of anomalous cosmic rays (ACRs) by Voyager 1 and 2. The model appeals to fast magnetic reconnection rather than shocks as the driver of acceleration. The ultimate source of energy is associated with magnetic field reversals that occur in the heliosheath. It is expected that the magnetic field reversals will occur throughout the heliosheath, but especially near the heliopause where the flows slow down and diverge with respect to the interstellar wind and also in the boundary sector in the heliospheric current sheet. While the first-order Fermi acceleration theory within reconnection layers is in its infancy, the predictions do not contradict the available data on ACR spectra measured by the spacecraft. We argue that the Voyager data are one of the first pieces of evidence favoring the acceleration within regions of fast magnetic reconnection, which we believe to be a widely spread astrophysical process.
- OSTI ID:
- 21372036
- Journal Information:
- Astrophysical Journal, Vol. 703, Issue 1; Other Information: DOI: 10.1088/0004-637X/703/1/8; ISSN 0004-637X
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
COSMOLOGY AND ASTRONOMY
ACCELERATION
ASTROPHYSICS
COSMIC RADIATION
INTERPLANETARY SPACE
MAGNETIC FIELD REVERSAL
MAGNETIC RECONNECTION
MAGNETOHYDRODYNAMICS
SOLAR WIND
VOYAGER SPACE PROBES
FLUID MECHANICS
HYDRODYNAMICS
IONIZING RADIATIONS
MAGNETIC FIELD CONFIGURATIONS
MECHANICS
PHYSICS
RADIATIONS
SOLAR ACTIVITY
SPACE
SPACE VEHICLES
STELLAR ACTIVITY
STELLAR WINDS
VEHICLES