What is the outer source of anomalous cosmic rays?

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SUMMARY

Researchers have identified that a portion of anomalous cosmic rays (ACRs) originates from interactions with dust grains in the Edgeworth-Kuiper Belt, rather than solely from neutral atoms in the local interstellar cloud. This discovery, detailed in the Geophysical Research Letters paper, reveals that sputtered atoms from comet-sized objects near Pluto's orbit contribute to the composition of ACRs, which include significant amounts of easily ionized elements like carbon, silicon, and iron. The findings enhance our understanding of the mass distribution and composition of the Edgeworth-Kuiper Belt and the plasma-dust interactions in stellar environments.

PREREQUISITES
  • Understanding of anomalous cosmic rays (ACRs)
  • Familiarity with the Edgeworth-Kuiper Belt
  • Knowledge of solar wind interactions
  • Basic concepts of plasma-dust interactions
NEXT STEPS
  • Research the composition and dynamics of the Edgeworth-Kuiper Belt
  • Study the mechanisms of solar wind and its effects on cosmic rays
  • Explore the role of sputtering in cosmic ray generation
  • Investigate plasma-dust interactions in various stellar environments
USEFUL FOR

Astronomers, astrophysicists, and researchers interested in cosmic ray origins, solar system formation, and the dynamics of the Edgeworth-Kuiper Belt will benefit from this discussion.

wolram
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http://www.sciencedaily.com/releases/2002/10/021031071017.htm

ScienceDaily (Oct. 31, 2002) — WASHINGTON - Researchers have found that a portion of anomalous cosmic rays -- charged particles accelerated to enormous energies by the solar wind -- results from interactions with dust grains from a belt of comet-sized objects near Pluto's orbit. These objects make up what is known as the Kuiper Belt, a remnant of the formation of the solar system.
 
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Here's the actual Geophysical Research Letters paper...

The Outer Source of Pickup Ions and Anomalous Cosmic Rays
Abstract. The traditionally accepted source of Anomalous Cosmic
Rays (ACRs) is neutral atoms penetrating the heliosphere from
the local interstellar cloud (LIC). The ACR composition should be
depleted in easily ionized atoms such as C, Si, and Fe. However, significant
fluxes of these ions are observed in ACRs and their source
has not been previously identified. We show that there is an “outer
source” of pickup ions, and hence ACRs, caused by sputtered atoms
(subsequently ionized and picked up by the solar wind) from small
grains generated via collisions of objects in the Edgeworth-Kuiper
Belt. The outer source accounts for the abundance and composition
of the additional population of ACRs. The discovery that
ACRs are generated from material in the Edgeworth-Kuiper Belt
provides an exciting new tool for understanding the mass distribution
and composition of the Edgeworth-Kuiper Belt, and for probing
the plasma-dust interactions in stellar environments.

N. A. Schwadron
Southwest Research Institute, San Antonio, Texas
M. Combi
Department of Atmospheric, Oceanic and Space Science, The University of Michigan, Ann Arbor
W. Huebner, D. J. McComas
Southwest Research Institute, San Antonio, Texas
http://people.bu.edu/nathanas/pub/OuterSource.pdf
 
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