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An analysis of the momentum forcing in the high-latitude lower thermosphere

机译:一个分析的动力强迫高纬度地区较低的热大气层

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We analyze the dynamics of the high-latitude thermsopheric wind system below 170 km for negative IMF B z by using a fully nonlinear model with a realistic distribution of the forcing. A transition of the forcing patterns and their relative contribution to the high-latitude lower thermospheric wind system occurs around 123 km under various conditions, weak or strong IMF, summer or winter. Winds around and above 123 km are sustained by the gradient-wind balance among divergent/convergent pressure gradient, Coriolis, and horizontal momentum advection (mainly centrifugal) accelerations. Below 123 km winds are maintained by the approximate balance of divergent/convergent pressure gradient, Coriolis, and Hall ion drag accelerations through modified geostrophy. The dominant contribution to the wind tendency (time rate of change) is the rotational component of the ion drag acceleration. The wind tendency above 123 km tends to resemble rotational Pedersen ion drag acceleration well, which reflects a rotated pattern of the E × B velocity. Near and below 123 km the wind tendency is also affected by the rotational component of the Hall ion drag acceleration whose pattern no longer closely resembles the pattern of the E × B velocity, and the wind pattern can differ significantly from that well above 123 km. Simulations for different strengths of the IMF and different seasons indicate that largely divergent/convergent Coriolis and horizontal momentum advection accelerations tend approximately to balance with the horizontal pressure gradient (as well as with divergent/convergent ion drag at lower altitudes) under various conditions. As the forcing increases the radius of curvature of the strong winds also tends to increase, so that the centrifugal acceleration does not increase quadratically with the maximum wind speed, and the tendency for a rough balance between the Coriolis and horizontal momentum advection accelerations in the duskside vortex above 123 km is maintained.
机译:我们分析的动态高纬度地区170公里以下thermsopheric风系统-国际货币基金组织(IMF) B z通过使用一个完全非线性模型现实迫使分布。迫使模式及其过渡相对贡献高纬度低thermospheric风系发生约123公里在各种条件下,弱或强国际货币基金组织(IMF),夏天还是冬天。持续的梯度风之间的平衡发散、收敛的压力梯度,科里奥利和水平动量平流(主要是离心加速度。是由近似平衡的维护发散、收敛的压力梯度,科里奥利通过修改和霍尔离子阻力加速度地转状态。趋势(时间变化率)旋转组件的离子阻力加速度。倾向倾向于像超过123公里旋转皮德森离子阻力加速度,这反映了一种旋转模式E×B速度。也是受到的转动分量吗大厅里没有离子的负加速度模式长相似的模式E×B速度,风模式可以有所不同显著的高于123公里。模拟不同优势的国际货币基金组织表明,很大程度上和不同的季节发散收敛科里奥利和水平动量平流加速度往往大约平衡水平压力梯度(以及发散/聚合离子拖在较低的海拔高度)在不同的条件下。增加了强大的曲率半径风也会增加,这样离心加速度并不增加与最大风速平方粗略的倾向之间的平衡科里奥利和水平动量平流加速度的duskside涡上方123公里是维护。

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