Study of the Detection Mode of Upper Atmospheric Wind Field Based on Lorentzian Profile Aurora

[in Chinese]; [in Chinese]; [in Chinese]; [in Chinese]

Journals >Acta Optica Sinica >Volume 25 >Issue 6 >Page 721 > Article

Acta Optica Sinica
Vol. 25, Issue 6, 721 (2005)

Study of the Detection Mode of Upper Atmospheric Wind Field Based on Lorentzian Profile Aurora

[in Chinese]^1、2、*, [in Chinese]¹, [in Chinese]¹, and [in Chinese]¹

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¹[in Chinese]

²[in Chinese]

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[in Chinese], [in Chinese], [in Chinese], [in Chinese]. Study of the Detection Mode of Upper Atmospheric Wind Field Based on Lorentzian Profile Aurora[J]. Acta Optica Sinica, 2005, 25(6): 721 Copy Citation Text

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References

[3] G. G. Shepherd, G. Thulllier, W. A. Gault et al.. WINDII, the wind imaging interferometer on the upper atmosphere research satellite[J]. J. Geophysical Research, 1993, 98(D6): 10725～10750

[4] Shepherd G G. Application of Doppler michelson imaging to upper atmosphere wind measurement: WINDII and beyond[J]. Appl. Opt., 1996, 35(16): 2764～2773

[5] G. B. Burns, P. F. B. Williams, R. P. Lowe et al.. Argon auroral emissions[J]. J. Atmospheric and Solar-Terrestrial Physics, 2002, 64: 2013～2017

[9] William A. Gault, Stoyan I Sargoytchev, Gordon G. Shepherd. Divided-mirror scanning technique for a small Michelson interferometer[C]. Proc. SPIE, 1996, 2830:15～18

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[1] Tang Yuanhe, GuoTing, Gao Haiyang. Modulation Transfer Function of Modified Sagnac Imaging Interferometer[J]. Acta Optica Sinica, 2010, 30(6): 1651

[in Chinese], [in Chinese], [in Chinese], [in Chinese]. Study of the Detection Mode of Upper Atmospheric Wind Field Based on Lorentzian Profile Aurora[J]. Acta Optica Sinica, 2005, 25(6): 721

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