Gt. Marklund et T. Karlsson, Characteristics of the auroral particle acceleration in the upward and downward current regions, PHYS CH P C, 26(1-3), 2001, pp. 81-96
Citations number
46
Categorie Soggetti
Earth Sciences
Journal title
PHYSICS AND CHEMISTRY OF THE EARTH PART C-SOLAR-TERRESTIAL AND PLANETARY SCIENCE
To understand auroral particle acceleration it is necessary to consider the
entire auroral current circuit, from the generator in the outer magnetosph
ere to the auroral ionosphere, decoupled from each other by field-aligned p
otential drops in both the upward and downward current regions. This paper
focusses on the characteristics of such potential drops responsible for the
accelerated electrons that produce the aurora and for the upward accelerat
ion of ions and electrons. First, some features of the converging electric
field structures in the upward current region are discussed based predomina
ntly on results from Viking observations within and above the acceleration
region. These include the relationship between the high-altitude potential
and the ionospheric potential associated with auroral area; ways to estimat
e the field-aligned potential drop from in situ satellite measurements of f
ields and particles; the role of low-frequency electric field fluctuations
for acceleration and heating of auroral particles. ii brief review is then
given of recent Freja results on characteristics of the downward curl ent r
egion, such as the intense diverging electric field structures that give ri
se to upward acceleration of ionospheric electrons and perpendicular ion he
ating. Different theoretical models have been proposed to explain these phe
nomena. It is clear that the plasma density on auroral field lines and the
ionospheric density play a fundamental role for where and when potential st
ructures a reformed in the upward and downward current region. For a curren
t generator feeding the auroral currents, particle acceleration is necessar
y to maintain the current through regions of low plasma density. The altitu
de distribution of the field-aligned potential will thus depend strongly on
the local ambient plasma conditions, and this vary with local time, season
and magnetic activity level. These characteristics could be investigated i
n detail by combining: measurements from various spacecraft (such as Viking
, Polar, Freja, FAST, and Astrid-2) at different altitudes with respect to
the the field-aligned potential distribution. (C) 2001 Elsevier Science Ltd
. All rights reserved.