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An energy balance study of the lower topside ionosphere using the Arecibo incoherent scatter radar and heating facilities

机译:上部较低的能量平衡研究使用阿雷西博电离层非相干散射雷达和取暖设施

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In this paper we describe the results of an experiment to study electron and ion temperature enhancements during an HF modification experiment at the Arecibo Observatory. This experiment is unique in that we pointed the radar away from the interaction region in the F region in order to study heat conduction along the field lines. Although electron temperature enhancements have been frequently observed when high-power radio waves are injected into the ionosphere, observations generally have occurred in the interaction region and the regions of elevated electron temperatures have been accompanied by small ion temperature increases (50–200 K). Like many such experiments, this one was conducted during winter solar minimum, when f 0 F 2 is low during the night at midlatitudes, but this experiment also had the advantage of the upgraded Arecibo HF facility, first used in 1997. The electron temperature enhancements were accompanied by a significant increase in the ion temperature (nearly 500 K). The observation away from the interaction region allowed the application of the time-dependent heating equation without having to estimate local heating effects (i.e., by keeping the conduction and loss terms in the energy balance calculation and neglecting the source term). More specifically, the heating rate of conduction was quantified by manipulating the heat equation. Thus the primary purpose was to observe the temperatures as the heat was conducted away from the F region ionosphere. We have observed the gradients in the electron temperature caused by the heater, estimated the conduction along the field lines, and studied the transfer of energy from the hot electrons to the ions and neutrals. At lower altitudes, near the electron-temperature peak, we show that O+ cooling is dominant, whereas in the lower topside H+ cooling is the most important. Experiments of the type described here could be enhanced with the new dual-beam system at Arecibo in conjunction with a heating facility.
机译:在本文中,我们描述的结果实验研究电子和离子温度在高频增强改性实验阿雷西博天文台。独一无二的,我们指出了雷达距离F地区以交互区域研究导热沿电场线。虽然电子温度增强当大功率电台经常被观察到波注入电离层,观察一般发生在相互作用区域和高的地区电子温度都伴随着小离子温度上升(50 - 200 K)许多这样的实验,这一个在冬天太阳,当0 f 2很低在夜间在情理之中,但这实验也有升级的优点阿雷西博高频设备,在1997年第一次使用。电子温度的改进伴随着一个显著增加离子温度(近500 K),观察了从交互区域允许加热时间的应用方程,而无需估计局部加热影响(例如,通过保持传导和损失能量平衡计算和条款忽视了源项)。传导的升温速率是量化操纵热方程。目的是观察温度的热是远离F地区进行的电离层。电子温度引起的加热器,估计,沿着电场线传导,和研究能量从高温的转移电子的离子和中性色。海拔,电子温度峰值附近,我们表明O +冷却是占主导地位,而在低干舷H +冷却是最重要的。这里所描述的实验类型增强与阿雷西博的新的双光束系统结合供热设施。

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