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首页> 外文期刊>Annales Geophysicae >Self-consistent modelling of the daytime electron density profile in the ionospheric F region
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Self-consistent modelling of the daytime electron density profile in the ionospheric F region

机译:电离层F区白天电子密度分布的自洽建模

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A theoretical self-consistent method for thedescription of daytime Ne(h) profiles in the ionospheric Fregion measured by EISCAT is proposed. It is based on the use of a theoreticalF-region model and measured electron density, Ne(h),electron, Te(h), and ion temperature, Ti(h),and field-aligned plasma drift Vl(h) profiles. The methoddescribes the observed Ne(h) profile with high accuracy forquiet and disturbed conditions. Two versions of the method are considered: inthe first the exospheric temperature Tex is derivedfrom a procedure minimizing [log(Ne(h)obs / Ne(h)cal]2, in the second Tex is deduced from the ion energyconservation in the F region. The method allows us to infer from theincoherent-scatter observations: concentrations of atomic oxygen, [O], molecularoxygen, [O2], molecular nitrogen, [N2]the vertical plasma drift, W, the exospheric temperature. Tex, and the shape parameter S in the neutraltemperature profile. The ratio ([O+]/Ne) calculatedby the theoretical model is used to correct Te(h), Ti(h) and Ne(h) profiles routinely measured with EISCAT which are knownto depend strongly on the actual applied ion-composition model. Such acorrection is especially important for geomagnetically disturbed periods whenthe F region is strongly enriched with molecular ions. We conclude that four ofthe six thermospheric parameters, namely [O], [N2], W and Tex can beconfidently inferred from the EISCAT observations, while the other two derivedparameters, [O2] ans S are less reliable.The method can be used for the analysis of long-term (seasonal, solar cycle) aswell as for day-to-day variations of the thermospheric parameters and theF-region ion composition using daytime incoherent-scatter observations.
机译:提出了一种用EISCAT方法描述电离层F区日间 N e (h)轮廓的理论自洽方法。它基于理论上的F区域模型和测得的电子密度 N e (h),电子, T e (h),离子温度 T i (h)和场取向等离子体漂移 V l (h)个人资料。该方法描述了观测到的 N e (h)轮廓,在安静和受干扰的条件下具有高精度。考虑了该方法的两个版本:首先,通过最小化[log( N e ( h) obs / N e (h) cal ] 2 ,在第二个 T ex 由F区域的离子能量守恒推论得出,该方法使我们可以从非相干散射观测值推论:原子氧浓度[ O],分子氧,[O ​​ 2 ],分子氮,[N 2 ]垂直等离子体漂移, W ,大气温度。 i> T ex 和中性温度曲线中的形状参数 S 。比率([O + ] / N e )用于校正 T e (h),T i (h 和N e (h)谱图,通常使用EISCAT进行常规测量,这在很大程度上取决于实际应用的离子组成模型。或F区域富含分子离子的地磁干扰时期。我们得出结论,六个热层参数中的四个,即[O],[N 2 ], W 和 T ex ,而其他两个导出的参数[O 2 ] ans S 则不那么可靠。该方法可用于分析术语(季节,太阳周期)以及热天球参数和F区离子组成的日间变化(使用白天非相干散射观测)。

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