Superposed epoch analysis of the ionospheric convection evolution during substorms : onset latitude dependence
Superposed epoch analysis of the ionospheric convection evolution during substorms : onset latitude dependence
复制标题
亚暴期间电离层对流演化的叠加历元分析:爆发纬度依赖性
DOI:
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发表时间:
2008
期刊:
影响因子:
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通讯作者:
T. Yeoman
中科院分区:
文献类型:
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作者:
A. Grocott;J. Wild;S. Milan;T. Yeoman
Using data from the Super Dual Auroral Radar Network (SuperDARN) we investigate the ionospheric con- vection response to magnetospheric substorms. Substorms were identified using the Far Ultraviolet (FUV) instrument on board the Imager for Magnetopause-to-Aurora Global Ex- ploration (IMAGE) spacecraft, and were then binned accord- ing to the magnetic latitude of their onset. A superposed epoch analysis of the ionospheric convection patterns for each onset-latitude bin was then performed using radar data for the interval 60 min before onset to 90 min after. It is found that lower onset-latitude substorms are associated with generally more enhanced convection than the higher latitude substorms, although they suffer from a significant localised reduction of the flow in the midnight sector during the expan- sion phase. Higher-latitude substorms are associated with a significant and rapid increase in the nightside convection fol- lowing substorm onset, with all onset-latitude bins showing an enhancement over onset values by 60 min into the ex- pansion phase. A rudimentary inspection of the concurrent auroral evolution suggests that the duration of the flow reduc- tion following substorm onset is dependent on the strength and duration of the expansion phase aurora and its associated conductivity enhancement.
影响因子:
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作者:
J. Wild;A. Grocott
通讯作者:
J. Wild;A. Grocott