State Key Laboratory of Magnetic Resonance and Atomic and Molecular
Physics, Wuhan Institute of Physics and Mathematics, Chinese Academy of
Sciences, Wuhan National Laboratory for Optoelectronics, Wuhan 430071,
China
Weiwei He
City College, Wuhan University of Science and Technology, Wuhan,
Hubei 430083, China
Yutao Feng
Key Laboratory of Spectral Imaging Technology of Chinese Academy of
Sciences, Xi'an Institute of Optics and Precision Mechanics, Chinese Academy
of Sciences, Xi'an 710119, China
Yuanhui Xiong
State Key Laboratory of Magnetic Resonance and Atomic and Molecular
Physics, Wuhan Institute of Physics and Mathematics, Chinese Academy of
Sciences, Wuhan National Laboratory for Optoelectronics, Wuhan 430071,
China
Faquan Li
State Key Laboratory of Magnetic Resonance and Atomic and Molecular
Physics, Wuhan Institute of Physics and Mathematics, Chinese Academy of
Sciences, Wuhan National Laboratory for Optoelectronics, Wuhan 430071,
China
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The 1.27 μm O2 dayglow is well-suited for remote sensing in near-space. The main goal of this paper is to discuss the effect of OH radiance on the wind and temperature measurements derived from limb-viewing observations of the O2 dayglow. It is apparent from the simulations that the presence of OH radiance as an interfering species decreases the wind and temperature accuracy at all altitudes, but this effect can be reduced considerably by improving OH radiance knowledge.
The 1.27 μm O2 dayglow is well-suited for remote sensing in near-space. The main goal of this...
