1.National Satellite Meteorological Center, China Meteorological Administration, Beijing, China
2.Key Laboratory of Space Weather, National Center for Space Weather, China Meteorological Administration, Beijing, China
3.Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun, China
4.State Key Laboratory of Applied Optics, Chinese Academy of Sciences, Changchun, China
5.Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China
6.Institutions of Earth Science, Chinese Academy of Sciences, Beijing, China
Xiao-Xin Zhang (xxzhang@cma.gov.cn)
Bo Chen (chenb@ciomp.ac.cn)
Published:2019,
Published Online:22 May 2019,
Received:08 January 2019,
Revised:18 April 2019,
Accepted:29 April 2019
Scan QR Code
Zhang, X. X. et al. Wide-field auroral imager onboard the Fengyun satellite. Light: Science & Applications, 8, 494-505 (2019).
Zhang, X. X. et al. Wide-field auroral imager onboard the Fengyun satellite. Light: Science & Applications, 8, 494-505 (2019). DOI: 10.1038/s41377-019-0157-7.
The newly launched Fengyun-3D (FY-3D) satellite carried a wide-field auroral imager (WAI) that was developed by Changchun Institute of Optics
Fine Mechanics and Physics
Chinese Academy of Sciences (CIOMP)
which will provide a large field of view (FOV)
high spatial resolution
and broadband ultraviolet images of the aurora and the ionosphere by imaging the N
2
LBH bands of emissions. The WAI consists of two identical cameras
each with an FOV of 68° in the along-track direction and 10° in the cross-track direction. The two cameras are tilted relative to each other to cover a fan-shaped field of size 130° × 10°. Each camera consists of an unobstructed four-mirror anastigmatic optical system
a BaF
2
filter
and a photon-counting imaging detector. The spatial resolution of WAI is ~10 km at the nadir point at a reference height of 110 km above the Earth's surface. The sensitivity is
>
0.01 counts s
-1
Rayleigh
-1
pixel
-1
(140-180 nm) for both cameras
which is sufficient for mapping the boundaries and the fine structures of the auroral oval during storms/substorms. Based on the tests and calibrations that were conducted prior to launch
the data processing algorithm includes photon signal decoding
geometric distortion correction
photometric correction
flat-field correction
line-of-sight projection and correction
and normalization between the two cameras. Preliminarily processed images are compared with DMSP SSUSI images. The agreement between the images that were captured by two instruments demonstrates that the WAI and the data processing algorithm operate normally and can provide high-quality scientific data f
or future studies on auroral dynamics.
Meier, R. R. Ultraviolet spectroscopy and remote sensing of the upper atmosphere.Space Sci. Rev.58, 1-185 (1991)..
Dashkevich, Z. V., Sergienko, T. I.&Ivanov, V. E. The Lyman-Birge-Hopfield bands in aurora.Planet. Space Sci.41, 81-87 (1993)..
Germany, G. A. et al. Use of FUV auroral emissions as diagnostic indicators.J. Geophys. Res. Space Phys.99, 383-388 (1994)..
Germany, G. A. et al. Determination of ionospheric conductivities from FUV auroral emissions.J. Geophys. Res. Space Phys.99, 23297-23305 (1994)..
Frank, L. A. et al. Global auroral imaging instrumentation for the Dynamics Explorer mission.Space Sci. Instrum.5, 369-393 (1981)..
Mende, S. B. et al. Far ultraviolet imaging from the IMAGE spacecraft. 1. System design.Space Sci. Rev.91, 243-270 (2000)..
Mende, S. B. et al. Far ultraviolet imaging from the IMAGE spacecraft. 2. Wideband FUV imaging.Space Sci. Rev.91, 271-285 (2000)..
Mende, S. B. et al. Far ultraviolet imaging from the IMAGE spacecraft. 3. Spectral imaging of Lyman-α and OI 135.6 nm.Space Sci. Rev.91, 287-318 (2000)..
Torr, M. R. et al. A far ultraviolet imager for the international solar-terrestrial physics mission.Space Sci. Rev.71, 329-383 (1995)..
Christensen, A. B. et al. Global ultraviolet imager (GUVI) for the NASA thermosphere-ionosphere-mesosphere energetics and dynamics (TIMED) mission.Proceedings of SPIE 2266, Optical Spectroscopic Techniques and Instrumentation for Atmospheric and Space Research(SPIE, San Diego, CA, United States, 1994).
Paxton, L. J. et al. Special sensor ultraviolet spectrographic imager: an instrument description.Proceedings of the Instrumentation for Planetary and Terrestrial Atmospheric Remote Sensing(SPIE, San Diego, CA, United States, 1992).
Strickland, D. J., Evans, J. S.&Paxton, L. J. Satellite remote sensing of thermospheric O/N2and solar EUV: 1. Theory.J. Geophys. Res. Space Phys.100, 12217-12226 (1995)..
Johnstone, A. D. Pulsating aurora.Nature274, 119-126 (1978)..
Frank, L. A. et al. The theta aurora.J. Geophys. Res. Space Phys.91, 3177-3224 (1986)..
Farrugia, C. J., Sandholt, P. E.&Burlaga, L. F. Auroral activity associated with Kelvin-Helmholtz instability at the inner edge of the low-latitude boundary layer.J. Geophys. Res. Space Phys.99, 19403-19411 (1994)..
Laundal, K. M.&Østgaard, N. Asymmetric auroral intensities in the Earth's northern and southern hemispheres.Nature460, 491-493 (2009)..
Han, D. S. et al. Throat aurora: the ionospheric signature of magnetosheath particles penetrating into the magnetosphere.Geophys. Res. Lett.43, 1819-1827 (2016)..
Tu, C. Y. et al. Space weather explorer—the KuaFu mission.Adv. Space Res.41, 190-209 (2008)..
Laikin, M.Lens Design4th edn (CRC Press, Boca Raton, FL, 2007).
Christensen, A. B. et al. Initial observations with the Global Ultraviolet Imager (GUVI) in the NASA TIMED satellite mission.J. Geophys. Res. Space Phys.108, 1451 (2003)..
Yang, H. B. et al. Thermal design and verification of transmission filter for wide angle aurora imager.Opt. Precis. Eng.22, 3019-3027 (2014)..
0
Views
2
Downloads
0
CSCD
Publicity Resources
Related Articles
Related Author
Related Institution