Optical spectrum analyzers and typical applications in astronomy and remote sensing

Author:

Yan C. S.12ORCID,Chen Y. W.34ORCID,Yang H. M.5ORCID,Ahokas E.3ORCID

Affiliation:

1. Library, Zhejiang University 1 , Hangzhou 310058, China

2. State Key Laboratory of Modern Optical Instrumentation 2 , Hangzhou 310058, China

3. Finnish Geospatial Research Institute 3 , Espoo 02151, Finland

4. College of Information Science and Electronic Engineering, Zhejiang University 4 , Hangzhou 310058, China

5. Shanghai University for Science and Technology 5 , Shanghai 200093, China

Abstract

Scientists are increasingly relying on astronomical and remote sensing technologies to gain deeper insights into the Earth and the universe. In these fields, the optical spectrum analyzer (OSA) or spectrometer plays a pivotal role. This Review offers a comprehensive overview of the fundamental principles, key parameters, and applications of various branches of traditional OSAs, including prisms, gratings, interferometers, tunable filters, and reconstructive spectrometers. We specifically focus on their latest major applications in astronomy and remote sensing. Additionally, we present a mathematical model of the generalized reconstructive spectrometer and provide a summary of its principles pertaining to spectral mapping, reconstruction, and imaging. Despite its limited aperture and étendue, the reconstructive spectrometer holds great potential for future use in astronomy and remote sensing due to its compact size and exceptional ultrahigh spectral resolution.

Funder

Key Laboratory of Space Active Opto-Electronics Technology

Science and Technology Innovation Plan of Shanghai Science and Technology Commission

Academy of Finland

Publisher

AIP Publishing

Subject

Instrumentation

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