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Christopher J. Mertens James M. Russell III Martin G. Mlynczak Chiao-Yao She Francis J. Schmidlin Richard A. Goldberg Manuel López-Puertas Peter P. Wintersteiner Richard H. Picard Jeremy R. Winick Xiaojing Xu 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
The Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) experiment is one of four instruments on NASA’s Thermosphere–Ionosphere–Energetics and Dynamics (TIMED) satellite. SABER measures broadband infrared limb emission and derives vertical profiles of kinetic temperature (Tk) from the lower stratosphere to approximately 120 km, and vertical profiles of carbon dioxide (CO2) volume mixing ratio (vmr) from approximately 70 km to 120 km. In this paper we report on SABER Tk/CO2 data in the mesosphere and lower thermosphere (MLT) region from the version 1.06 dataset. The continuous SABER measurements provide an excellent dataset to understand the evolution and mechanisms responsible for the global two-level structure of the mesopause altitude. SABER MLT Tk comparisons with ground-based sodium lidar and rocket falling sphere Tk measurements are generally in good agreement. However, SABER CO2 data differs significantly from TIME-GCM model simulations. Indirect CO2 validation through SABER-lidar MLT Tk comparisons and SABER-radiation transfer comparisons of nighttime 4.3 μm limb emission suggest the SABER-derived CO2 data is a better representation of the true atmospheric MLT CO2 abundance compared to model simulations of CO2 vmr. 相似文献
184.
R.D. Gehrz E.E. Becklin I. de Pater D.F. Lester T.L. Roellig C.E. Woodward 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
The Stratospheric Observatory for Infrared Astronomy (SOFIA) is a joint US/German Project to develop and operate a gyrostabilized 2.5-m telescope in a Boeing 747-SP. This observatory will allow astronomical observations from 0.3 μm to sub-millimeter wavelengths at stratospheric altitudes as high as 45,000 ft where the atmosphere is not only cloud-free, but largely transparent at infrared wavelengths. The dynamics and chemistry of interstellar matter, and the details of embedded star formation will be key science goals. In addition, SOFIA’s unique portability will enable large-telescope observations at sites required to observe transient phenomena and location specific events. SOFIA will offer the convenient accessibility of a ground-based telescope for servicing, maintenance, and regular technology upgrades, yet will also have many of the performance advantages of a space-based telescope. Initially, SOFIA will fly with nine first-generation focal plane instruments that include broad-band imagers, moderate resolution spectrographs that will resolve broad features from dust and large molecules, and high resolution spectrometers capable of studying the chemistry and detailed kinematics of molecular and atomic gas. First science flights will begin in 2010, leading to a full operations schedule of about 120 8–10 h flights per year by 2014. The next call for instrument development that can respond to scientifically exciting new technologies will be issued in 2010. We describe the SOFIA facility and outline the opportunities for observations by the general scientific community with cutting edge focal plane technology. We summarize the operational characteristics of the first-generation instruments and give specific examples of the types of fundamental scientific studies these instruments are expected to make. 相似文献
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对光纤激光焊接2.5mm厚TC4对接接头的拉伸力学性能进行研究,其研究方法为在常规的拉伸试验中,附加同步的红外热像测量,实时记录拉伸全过程中试样在力作用下温度场的变化。常规测试结果表明:接头与母材的强度相当,延伸率只达到母材的59.53%。试样温度场测试结果表明:当接头和母材受到的轴向载荷低于屈服强度对应载荷时,接头在热影响区部位会产生较大的应力集中,但接头和母材均未产生明显的塑性变形;当载荷等于屈服强度对应载荷时,均在宏观屈服点之前发生了微观的塑性变形;当载荷等于抗拉强度对应载荷时,接头发生剧烈塑性变形区域的长度只达到母材的35%,且接头与母材发生剧烈塑性变形区域的长度随拉伸过程的进行逐渐增加。 相似文献
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A multi-scale narrow band correlated-k distribution(MSNBCK) model is developed to simulate infrared radiation(IR) from an exhaust system of a typical aircraft engine.In this model,an approximate approach instead of statistically uncorrelated assumption is used to treat overlapping bands in gas mixture.It significantly reduces the requirement for computing power through converting the exponential increase of computing power consumption with the increase of participating gas species to linear increase.Besides,MSNBCK model has a great advantage compared with conventional methods which can estimate each species' contribution to the total gas mixture radiation intensity.Line by line(LBL) results,experimental data and other results in the references are used to evaluate this new model,which demonstrates its advantage in terms of accuracy and computing efficiency.By coupling this model and finite volume method(FVM) into radiative transfer equation(RTE),a comparative study is conducted to simulate IR signature from the exhaust system.The results indicate that wall's IR emission should be considered in both 3-5 μm and8-14 μm bands while gases' IR emission plays an important role only in 3-5 μm band.For plume IR radiation,carbon dioxide's emission is much more significant than that of water vapor in both3-5μm and 8-14 μm bands.Especially in 3-5 μm band,the water vapor's IR signal can even be neglected compared with that of carbon dioxide. 相似文献
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为了获得涡扇发动机二元喷管热喷流的红外辐射特性,分别对喷口面积相等且宽高比分别为1,4,8,12和16的二元喷管的热喷流的红外辐射特性进行了测试,并与轴对称喷管进行了对比。喷管内涵通道的气流温度为500℃,外涵通道的气流温度为环境温度,内、外涵气流的流量比为1:3。通过实验,获得了各个喷管的热喷流在3~5μm波段的红外光谱辐射强度分布和积分强度。结果表明,采用宽高比大于1的二元喷管能够有效降低热喷流的红外辐射,但是在宽高比大于8以后二元喷管热喷流的红外辐射不再随宽高比的增加而明显减小。 相似文献
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