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A new strategy for ionospheric remote sensing using the 130.4/135.6 nm airglow intensity ratios

XiaoHan Yin JianQi Qin Larry J.Paxton

地球与行星物理(英文)2023,Vol.7Issue(4):445-459,15.
地球与行星物理(英文)2023,Vol.7Issue(4):445-459,15.DOI:10.26464/epp2023042

A new strategy for ionospheric remote sensing using the 130.4/135.6 nm airglow intensity ratios

A new strategy for ionospheric remote sensing using the 130.4/135.6 nm airglow intensity ratios

XiaoHan Yin 1JianQi Qin 1Larry J.Paxton2

作者信息

  • 1. School of Earth and Space Sciences,Peking University,Beijing 100871,China
  • 2. Applied Physics Laboratory,Johns Hopkins University,Laurel,MD 20723,USA
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摘要

关键词

nighttime ionosphere/far-ultraviolet remote sensing/130.4/135.6 nm airglow intensity ratio/peak height of the F2 region(hmF2)/TIMED observation

Key words

nighttime ionosphere/far-ultraviolet remote sensing/130.4/135.6 nm airglow intensity ratio/peak height of the F2 region(hmF2)/TIMED observation

引用本文复制引用

XiaoHan Yin,JianQi Qin,Larry J.Paxton..A new strategy for ionospheric remote sensing using the 130.4/135.6 nm airglow intensity ratios[J].地球与行星物理(英文),2023,7(4):445-459,15.

基金项目

This work was supported by the National Natural Science Founda-tion of China through Grant 8206100245 and by the Chinese Meteorological Administration through Grant FY-APP-ZX-2022.0222.The GUVI data were provided through support from the NASA Mission Operations and Data Analysis(MO&DA)program and are available from http://guvitimed.jhuapl.edu/data_products.The GUVI instrument was designed and built by the Aerospace Corporation and Johns Hopkins University based on the design of the Defense Meteorological Satellite Program(DMSP)Special Sensor Ultraviolet Spectrographic Imager(SSUSI).The principal investigator is Andrew B.Christensen,and the chief scientist and co-principal investigator is Larry J.Paxton.The GIRO data are publicly available from http://spase.info/SMWG/Observa-tory/GIRO. (MO&DA)

地球与行星物理(英文)

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