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A&A 419, 793-799 (2004)
DOI: 10.1051/0004-6361:20034513
Ion heating in an auroral potential structure
A. Anastasiadis1, I. A. Daglis1 and C. Tsironis21 National Observatory of Athens, Institute for Space Applications and Remote Sensing, 15236 Penteli, Greece
e-mail: daglis@space.noa.gr
2 Department of Physics, Aristotle University of Thessaloniki, 54124 Thessaloniki, Greece
e-mail: ctsironis@astro.auth.gr
(Received 15 October 2003 / Accepted 26 February 2004 )
Abstract
We investigate the interaction of O
+ ions with a
one-dimensional potential well, using Hamiltonian formulation.
Heating of plasma originating in the terrestrial ionosphere plays
a catalytic role in solar-driven magnetic storms, which dissipate
energy globally within the magnetosphere of the earth. An
interesting candidate for ionospheric plasma heating is a
potential well located at auroral arcs in the high-latitude
magnetosphere. We consider a potential with an exponential form,
having a characteristic length
Lx. The oxygen ions
drift towards the auroral arc in the presence of a constant
magnetic field
Bz and a constant electric field
Ey. The orbits of individual ions for different
initial conditions - phase angle and kinetic energy - are
traced. Our results show that, depending upon the initial
conditions, test particles can be either accelerated or
decelerated. Furthermore, we perform a parametric study for the
interactions of mono-energetic and Maxwellian type of initial ion
distribution - using random phase angle injection of the
particles - with respect to our main model parameter, the
characteristic length of the potential
Lx. We conclude
that for characteristic lengths comparable to twice the ion
gyroradius, the O
+ population is accelerated.
Key words: acceleration of particles -- plasmas
Offprint request: A. Anastasiadis, anastasi@space.noa.gr
© ESO 2004
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