Anisotropic core ion temperatures associated with strong zonal flows and upflows

被引:19
作者
Archer, W. E. [1 ]
Knudsen, D. J. [1 ]
Burchill, J. K. [1 ]
Patrick, M. R. [1 ]
St Maurice, J. P. [2 ]
机构
[1] Univ Calgary, Dept Phys & Astron, Calgary, AB T2N 1N4, Canada
[2] Univ Saskatchewan, Dept Phys & Engn Phys, Saskatoon, SK, Canada
基金
加拿大自然科学与工程研究理事会;
关键词
IONOSPHERIC ACCELERATION MECHANISM; VELOCITY DISTRIBUTIONS; AURORAL IONOSPHERE; COLLISION MODEL; F-REGION; EISCAT;
D O I
10.1002/2014GL062695
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
The Swarm satellites observe strongly anisotropic ion temperatures at 500 km altitude. The ion temperature anisotropy ratios going up to 5 for the strongest electric fields presented in this paper. The largest observed anisotropy ratios exceed the values predicted by theories of collisional heating in strong flows by a factor of 2, indicating that collisional cross sections should perhaps be revised for O+ ion colliding with O. Temperature anisotropy is also found not to be a simple function of electric field strength. This could be understood in terms a time delay needed to advect hot anisotropic ion velocity distributions from strongly collisional regions below 400 km to weakly collisional regions at 500 km and above. The mirror force associated with these events is insufficient to account for the observed upward flows (> 500 m/s). For gyroresonant heating to be consistent with our observations, an additional mechanism for field-aligned acceleration is required.
引用
收藏
页码:981 / 986
页数:6
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