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SWIFT-DASH: Spatial Heterodyne Spectroscopy Approach to Stratospheric Wind and Ozone Measurement

机译:SWIFT-DASH:平流层风和臭氧测量的空间外差光谱法

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摘要

Passive wind measurements using Doppler shifts from atmospheric emissions were well demonstrated by the Wind Imaging Interferometer (WINDII) and the High Resolution Doppler Imager (HRDI) instruments on the National Aeronautics and Space Administration's (NASA's) Upper Atmosphere Research Satellite, operated from 1991 to 2005. For WINDII these emissions were from visible region upper atmospheric airglow in the altitude range from 80 to 300 km. Application of the same technique in the stratosphere requires using thermal emission from a minor constituent, and an ozone line near 1133 cm(-1) (about 8.8 mu m) has been identified as a suitable target line. The WINDII method employed a Doppler Michelson Interferometer, in which the wind is measured from phase shifts of a single spectral line. Isolating a single ozone spectral line is a major challenge but using Spatial Heterodyne Spectroscopy (SHS) offers a way to resolve a number of interferogram spectral components (fringes) within a narrow spectral range. The instrument is a Michelson interferometer similar to WINDII but one in which the two mirrors are replaced by diffraction gratings. A developmental instrument capable of measuring the phase shifts from several ozone lines within a spectral range of 4 cm(-1) has been designed, built, and operated in the laboratory. Simulated retrievals using the measurement parameters of this instrument demonstrate the capability of wind measurement with an accuracy better than 3 m s(-1) over an altitude range of 24 to 60 km. The retrieval employs four spectral lines for wind and three fringe frequencies for ozone concentration (of about 30 possible), each of which provides an optimal measurement for a particular altitude range. Ozone concentrations are also provided with an accuracy better than 10% from 20 to 50 km. Further detailed tests of this instrument are planned for the future. This work is supported by the Canadian Space Agency.
机译:1991年至2005年运行的美国国家航空航天局(NASA)上层大气研究卫星上的风成像干涉仪(WINDII)和高分辨率多普勒成像仪(HRDI)仪器很好地证明了使用多普勒偏移大气的被动风测量结果对于WINDII,这些排放物是在80至300 km高度范围内的可见区域高层大气辉光产生的。在平流层中应用相同技术需要使用微量成分的热辐射,并且已确定将1133 cm(-1)(约8.8微米)附近的臭氧线作为合适的目标线。 WINDII方法使用多普勒·迈克尔逊干涉仪,其中风是根据单个光谱线的相移测量的。隔离一条臭氧光谱线是一个主要挑战,但是使用空间外差光谱(SHS)提供了一种在狭窄光谱范围内解决许多干涉图光谱成分(条纹)的方法。该仪器是类似于WINDII的迈克尔逊干涉仪,但其中的两个反射镜被衍射光栅代替。在实验室中已经设计,制造和运行了一种能够测量4 cm(-1)光谱范围内的多个臭氧线的相移的开发仪器。使用该仪器的测量参数进行的模拟反演表明,在24至60 km的海拔范围内,风测量的精度优于3 m s(-1)。检索使用四条​​谱线记录风向,使用三条谱线记录臭氧浓度(大约30种可能),每条谱线为特定的海拔范围提供最佳测量。在20至50 km范围内,臭氧浓度的准确度也优于10%。计划在将来对该仪器进行进一步的详细测试。这项工作得到了加拿大航天局的支持。

著录项

  • 来源
    《Atmosphere-ocean》 |2015年第1期|50-57|共8页
  • 作者单位

    York Univ, Ctr Res Earth & Space Sci, Toronto, ON M3J 2R7, Canada;

    York Univ, Ctr Res Earth & Space Sci, Toronto, ON M3J 2R7, Canada;

    York Univ, Ctr Res Earth & Space Sci, Toronto, ON M3J 2R7, Canada;

    York Univ, Ctr Res Earth & Space Sci, Toronto, ON M3J 2R7, Canada;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    spectroscopy; winds; ozone; Michelson;

    机译:光谱;风;臭氧;米歇尔森;

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