Yang Y F, Lu J Y, Wang J S, et al. 2013. Influence of interplanetary magnetic field and solar wind on auroral brightness in different regions. J. Geophys. Res., 118(1): 209-217.
[2]
Blixt E M, Kosch M J, Semeter J. 2005. Relative drift between black aurora and the ionospheric plasma. Ann. Geophys., 23(5): 1611-1621.
[3]
Blixt E M, Semeter J, Ivchenko N. 2006. Optical flow analysis of the aurora borealis. IEEE Geoscience and Remote Sensing Letters, 3(1): 159-163.
[4]
Corpetti T, Mémin , Pérez P. 2002. Dense estimation of fluid flows. IEEE Transactions on Pattern Analysis and Machine Intelligence, 24(3): 365-380.
[5]
Haerendel G, Buchert S, La Hoz C, et al. 1993. On the proper motion of auroral arcs. Journal of Geophysical Research, 98(A4): 6087-6099.
[6]
Horn B K P, Schunck B G. 1981. Determining optical flow. Artificial Intelligence, 17(1-3): 185-203.
[7]
Hu H Q, Liu R Y, Yang H G, et al. 1999. The auroral occurrence over Zhongshan Station, Antarctica. Chinese Journal of Polar Science, 10(2): 101-109.
[8]
Kauristie K, Syrj？suo M T, Amm O, et al. 2001. A Statistical study of evening sector arcs and electrojets. Advances in Space Research, 28(11): 1605-1610.
[9]
Kimball J, Hallinan T J. 1998. Observations of black auroral patches and of their relationship to other types of aurora. Journal of Geophysical Research, 103(A7): 14671-14682.
[10]
Marklund G T. 1984. Auroral arc classification scheme based on the observed arc-associated electric field pattern. Planetary and Space Science, 32(2): 193-211.
[11]
Qiu Q, Yang H G, Lu Q M, et al. 2013. Widths of dayside auroral arcs observed at the Chinese Yellow River Station. Journal of Atmospheric and Solar-Terrestrial Physics, 102: 222-227.
[12]
Verri A, Poggio T. 1987. Against quantitative optical flow.//Proceedings of the 1st International Conference on Computer Vision. London England, 171-180.
[13]
Wang Q, Liang J M, Hu Z J, et al. 2010. Spatial texture based automatic classification of dayside aurora in all-sky images. Journal of Atmospheric and Solar-Terrestrial Physics, 72(5-6): 498-508.
[14]
Yang H, Sato N, Makita K, et al. 2000. Synoptic observations of auroras along the postnoon oval: a survey with all-sky TV observations at Zhongshan, Antarctica. Journal of Atmospheric and Solar-Terrestrial Physics, 62(9): 787-797.
[15]
Yang Q J, Liang J M, Hu Z J, et al. 2012a. Auroral sequence representation and classification using hidden markov models. IEEE Transactions on Geoscience and Remote Sensing, 50(12): 5049-5060.
[16]
Yang Q J, Liang J M, Hu Z J, et al. 2012b. Automatic recognition of poleward moving auroras from all-sky image sequences based on HMM and SVM. Planetary and Space Science, 69(1): 40-48.
[17]
Yang Y F, Lu J Y, Wang J S, et al. 2011. Different response of dayside auroras to increases in solar wind dynamic pressure. J. Geophys. Res., 116(A8): A08314.
