DocumentCode :
124874
Title :
Discrete auroral arcs generated by ionospheric feedback instability
Author :
Nan Jia ; Streltsov, Anatoly V.
Author_Institution :
Thayer Sch. of Eng., Dartmouth Coll., Hanover, NH, USA
fYear :
2014
fDate :
8-11 Jan. 2014
Firstpage :
1
Lastpage :
1
Abstract :
Summary form only given. Currently, the hypothesis that discrete auroral arcs are produced by fluxes of magnetospheric electrons accelerated along the ambient magnetic field into the ionosphere by linear/non-linear mechanisms associated with magnetic field-aligned currents (FACs) carried by ultra-low-frequency (ULF) Alfvén waves is confirmed by a large number of experimental and theoretical works. This correlation arises from the fact that dispersive Alfvén waves have a component of the electric field parallel to the ambient magnetic field. This field can accelerate electrons into the ionosphere and produce some types of the discrete aurora. Two main questions studies of ULF waves and the discrete aurora seek to answer are: 1) What physical mechanism(s) generates the ULF waves? 2) What parameters of the coupled magnetosphere-ionosphere system define frequency, dynamics, and spatial structure of these waves? Ionospheric Feedback instability (IFI) is one of the most self-consistent physic models that aims to answer these two questions. The basic idea of IFI is that ULF waves can be generated due to the active interaction between FAC and ionospheric plasma under some favorable conditions, for example, large electric field and low plasma density in the ionosphere. Our study uses a newly developed three-dimensional MHD model to investigate the discrete auroral arcs generated by IFI. The effects of Hall conductivity, convective nonlinearity in both ionosphere and magnetic field on the dynamics of discrete auroral arcs are studies through this model. It is found that our model can explain formation and spatial scales of homogeneous discrete auroral arcs, largescale auroral folds, and small-scale curls in active aurora. Furthermore, the simulation results from the model successfully reproduce discrete auroral arcs with homogeneous/inhomogeneous structures. These numerical results are in good agreement with observed data during the substorm event on Octobe- 29, 2008 in Alaska.
Keywords :
aurora; convection; ionosphere; magnetic storms; magnetohydrodynamic waves; magnetosphere; plasma instability; plasma magnetohydrodynamics; 3D MHD model; AD 2008 10 29; Alfven wave dynamics; Alfven wave frequency; Alfven wave spatial structure; Hall conductivity effects; ULF wave generation; ambient magnetic field; convective nonlinearity; coupled magnetosphere-ionosphere system; dispersive Alfven waves; homogeneous discrete auroral arcs; ionospheric feedback instability; large scale auroral folds; magnetic field aligned currents; magnetospheric electron flux; nonlinear electron acceleration mechanisms; small scale active aurora curls; substorm; ultralow frequency Alfven waves; Acceleration; Educational institutions; Electric fields; Ionosphere; Magnetic fields; Magnetosphere; Numerical models;
fLanguage :
English
Publisher :
ieee
Conference_Titel :
Radio Science Meeting (USNC-URSI NRSM), 2014 United States National Committee of URSI National
Conference_Location :
Boulder, CO
Print_ISBN :
978-1-4799-3119-4
Type :
conf
DOI :
10.1109/USNC-URSI-NRSM.2014.6928091
Filename :
6928091
Link To Document :
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