The potential for radiometric retrievals of halocarbon concentrations from the MIPAS-E instrument

Halocarbons, such as CFC-11, CFC-12 and HCFC-22, are important trace gases in the atmosphere through their role as greenhouse gases and their influence on stratospheric ozone chemistry. This paper focuses on an initial study using integration of spectral radiance measurements from a spaceborne limb sounding Fourier Transform Spectrometer (FTS) to retrieve these compounds in the upper troposphere and lower stratosphere (UTLS). The instrument employed in this study is the Michelson Interferometer for Passive Atmospheric Sounding onboard ENVISAT (MIPAS-E) which obtains spectral data in the altitude range of 6–68 km at an unapodized spectral resolution of 0.025 cm⁻¹. We have used optimal estimation techniques to retrieve vertical information for these compounds using a radiometric approach.

It is shown that significant retrieval information is obtained at up to five measured levels in the UTLS for CFC-11, up to six for CFC-12 and up to two levels for HCFC-22. An initial error analysis indicates significant sensitivity of our retrievals to variability in operationally retrieved pressure and temperature data. For each halocarbon, gain, offset and spectroscopic uncertainties generally each contribute less than 10% to the total error. Finally, tracer correlations are used to compare the datasets to equivalent relationships derived here from version 2 ATMOS data with very good agreements for CFC-12 but with more variability in the CFC-11 comparisons.     

空间光学遥感器天然辐射效应数据库研究

空间环境是诱发卫星异常和故障的主要原因之一。光学遥感器作为卫星最重要的有效载荷之一，在空间会受到空间辐射环境的影响。因此在研制光学遥感器的同时，需要同时考虑空间辐射环境因素，文章就空间光学遥感器天然辐射效应数据库的设计和应用进行了介绍。     

嫦娥工程数据接收分系统

嫦娥工程是我国发展深空探测走出的关键一步,意义重大。为和平应用空间资源,加强国际间的合作,在嫦娥工程中较完整地采用了CCSDS标准数据结构。文中介绍嫦娥工程数据接收分系统的主要功能、指标、组成以及目前的进展状态。     

民用运输类飞机合格审定性能试飞方法研究

结合Y7－200A飞机型号合格审定试飞情况，对一般科目试飞、模拟冰型试飞及自然结冰试飞方法进行了研究及探讨。主要侧重于试飞方法的改进及对相关条款的理解，同时对试飞过程中遇到的难点及解决情况进行了介绍。所得结论为今后运输类飞机合格审定提供了借鉴，可供类似型号合格审定参考使用。     

高效率E类功率放大器在某调频电台发射机中的应用

高效率E类功率放大器是一种新型的开关模式功率放大器,由Sokals发明,Raab作了理论上的分析,但至今还不完善,近年来,工程应用研究是讨论的主要课题。本文根据某调频电台发射机的具体情况,讨论了它的设计方法和理论,并给出了试验结果。实验结果表明,应用了E类放大器之后,发射机的输出功率增加,整机效率提高,电池寿命延长,通信距离增加,效果明显改善,体现了应用高效率E类放大器的优越性。     

应用Pro/E软件设计时几个问题的探讨

详细介绍了应用Pro／E软件进行设计的过程中在工作目录的设置、小数位置的设置、单位制的设置和转换、系统颜色的改变以及对特征的重定义等方面遇到的问题和解决方法。     

基于Pro/E和ANSYS的齿轮接触应力的有限元分析

为了避免因齿轮折断、齿面损伤及塑性变形等因素引发的生产事故,有必要对齿轮接触状态的强度性能进行分析和评估。基于Pro/E平台,通过参数化方法建立齿轮模型,用IGES文件格式将模型导入ANSYS软件中,用有限元方法对齿轮节点处的接触应力进行了分析,进而精确分析了齿轮结构强度和可靠性。     

电离层峰下结构的数值模拟

在考虑由扩散与中性风引起的动力学输运与有原子离子Ｏ＾＋（＾４Ｓ），Ｏ＾＋（＾２Ｄ）与Ｏ＾＋（＾２Ｐ）以及分子离子Ｏ２＾＋，ＮＯ＾＋，Ｎ２＾＋参加光化学反应的电离层－热层体系中，提出一个一维时变的电离层剖面数值模型，通过数值计算着重讨论了武昌地区Ｆ２层峰以下，尤其是Ｅ／Ｆ与Ｆ１／Ｆ２谷区的电离层形态与有关过程，得到如下结论：（１）对于原子离子，单一成分Ｏ＾＋（＾４Ｓ）的光化学反应与输运，也有助于形成     

Application of dynamic recrystallization model in AZ12 magnesium alloy rolling process

To deeply understand the dynamic recrystallization behavior of as-cast AZ12 magnesium alloy in deformation process, the uniaxial hot compression experiments were implemented through systematic isothermal compression experiments. The true strain of thermal compression experiments was set to 50% with temperatures of 200, 250, 300, 350, 400 °C and the strain rates of 0.001, 0.01, 0.1, 1 s^?1. The Dynamic Recrystallization (DRX) kinetic model of AZ12 magnesium alloy was established and the accuracy of this model was verified. The model is used to predict the volume fraction of the sheet obtained by rolling through different rolling passes under the condition of consistent total reduction (50%). And the predicted results are in good agreement with the experimental results.     

Statistical ionospheric E layer properties measured with the Cyprus Digisonde and comparisons with IRI predictions

This paper reports the diurnal, seasonal, and long term variability of the E layer critical frequency (foE) and peak height (hmE) derived from Digisonde measurements from 2009 to 2016 at the low-middle latitude European station of Nicosia, Cyprus (geographical coordinates: 35°N, 33°E, geomagnetic lat. 29.38°N, I = 51.7°). Manually scaled monthly median values of foE and hmE are compared with IRI-2012 predictions with a view to assess the predictability of IRI. Results show that in general, IRI slightly overestimates foE values both at low and high solar activity. At low solar activity, overestimations are mostly limited to 0.25?MHz (equivalent electron density, 0.775?×?10³?el/m^?3) but can go as high as 0.5?MHz (equivalent electron density, 3.1?×?10³?el/m^?3, during noon) around equinox. In some months, underestimations, though sporadic in nature, up to 0.25?MHz are noted (mostly during sunrise and sunset). At high solar activity, a similar pattern of over-/underestimation is evident. During the entire period of study, over-/under estimations are mostly limited to 0.25?MHz. In very few cases, these exceed 0.25?MHz but are limited to 0.5?MHz. Analysis of hmE reveals that: (1) hmE remains almost constant during ±2 to ±4?h around local noon, (2) hmE values are higher in winter than in spring, summer and autumn, (3) there are two maxima near sunrise and sunset with a noontime minimum in between. During the entire period of study, significant differences between observed hmE and the IRI predictions have been noted. IRI fails to predict hmE and outputs a constant value of 110?km, which is higher than most of the observed values. Over- and under estimations range from 3 to 13?km and from 0 to 3?km respectively.