Abstract

Abstract. Polarization array based polarization Michelson wind field detection interferometer is a new type of interferometer for detecting atmospheric temperature and wind field velocity. We proposed a theoretical model and design of the novel static polarization wind imaging interferometer (NSPWII). It consists of a group of polarizers and waveplates, a polarization beamsplitter, a field widened Michelson interferometer, a pyramid prism, and a polarization array. Based on the principle of polarization interference, a polarization array composed of four polarizers with 45° polarization directions differences is directly in front of the detector, and four modulated light beams from the pyramid prism pass through the four polarizers. Then, interferograms with four different intensity are imaged on the detector simultaneously, which further provides the atmospheric temperature and wind field velocity. The advantages of this instrument are static (no moving parts), achromatic, and temperature compensated. It is capable of measuring the upper atmospheric wind field in real time with a high precision.

Highlights

  • The Earth’s atmosphere is a natural barrier to protect the life on Earth and plays an important role in maintaining the climate stability of the Earth

  • We propose a novel static polarization wind imaging interferometer (NSPWII)

  • It consists of a polarizer, a polarization beamsplitter (PBS), two glass arms for field widening, three quarter wave plates (QWP), and two total reflection mirrors

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Summary

INTRODUCTION

The Earth’s atmosphere is a natural barrier to protect the life on Earth and plays an important role in maintaining the climate stability of the Earth. Due to a variety of reasons, the Earth’s atmosphere has been damaged, causing a series of problems such as the hole in the ozone layer and global climate change. Solving these problems first requires high-precision, large-scale atmospheric dynamic detection. The passive detection of the upper atmospheric wind field is based on the interference imaging spectroscopy and the Doppler effect of electromagnetic waves It uses the airglow (aurora) in the upper atmosphere as the detection source, and detects the modulation of interference fringes using the interferometer with a large optical path difference. The double-blind peer-review was conducted on the basis of the full paper

PRINCIPLE
FIELD WIDENING DESIGN
MODELING AND SIMULATION
CONCLUSION
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