Mesoscale field-aligned irregularity structures (FAIs) of airglow associated with medium-scale traveling ionospheric disturbances (MSTIDs)

被引:46
作者
Sun, Longchang [1 ,2 ]
Xu, Jiyao [1 ]
Wang, Wenbin [3 ]
Yue, Xinan [4 ]
Yuan, Wei [1 ]
Ning, Baiqi [5 ]
Zhang, Donghe [6 ]
de Meneses, F. C. [1 ]
机构
[1] Chinese Acad Sci, Natl Space Sci Ctr, State Key Lab Space Weather, Beijing, Peoples R China
[2] Chinese Acad Sci, Grad Univ, Beijing, Peoples R China
[3] Natl Ctr Atmospher Res, High Altitude Observ, Boulder, CO 80307 USA
[4] Univ Corp Atmospher Res, COSMIC Program Off, Boulder, CO USA
[5] Chinese Acad Sci, Inst Geol & Geophys, Beijing, Peoples R China
[6] Peking Univ, Dept Geophys, Beijing 100871, Peoples R China
基金
中国国家自然科学基金; 美国国家科学基金会;
关键词
MIDLATITUDE SPREAD-F; STATISTICAL CHARACTERISTICS; THERMOSPHERIC WINDS; REGION IONOSPHERE; PLASMA DEPLETIONS; FRONT CAMPAIGN; NORTHERN CHINA; MILLSTONE-HILL; MU RADAR; IMAGES;
D O I
10.1002/2014JA020944
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper, we report the evolution (generation, amplification, and dissipation) of optically observed mesoscale field-aligned irregularity structures (FAIs) (similar to 150 km) associated with a medium-scale traveling ionospheric disturbance (MSTID) event. There have not been observations of mesoscale FAIs of airglow before. The mesoscale FAIs were generated in an airglow-depleted front of southwestward propagating MSTIDs that were simultaneously observed by an all-sky imager, a GPS monitor, and a digisonde around Xinglong (40.4 degrees N, 30.5 degrees magnetic latitude), China, on 17/18 February 2012. A normalized cross-correlation method has been used to obtain the velocities of mesoscale FAIs and MSTIDs. The mesoscale FAIs had an obvious northwestward relative velocity to main-body MSTIDs (about 87.0 m/s on average). The direction of this relative velocity was roughly parallel to the depleted fronts. Furthermore, the evolution of the mesoscale FAIs was mostly controlled by the intensity of the depleted fronts. Occurred in a highly elevated ionosphere that had a total electron content depletion associated with large negative airglow perturbations (-25%), the mesoscale FAIs grew rapidly when they experienced southeastward wind, which had a speed of about 100 m/s and were measured by a Fabry-Perot interferometer. A northeastward polarization electric field within a depleted airglow front can play a controlling role in the development of the mesoscale FAIs. The electric field can significantly elevate the ionosphere and move the mesoscale FAIs northwestward by the E x B drift. The processes for the generation and development of the polarization electric field and the mesoscale FAIs, however, need further study.
引用
收藏
页码:9839 / 9858
页数:20
相关论文
共 66 条
[61]   A new Fabry-Perot interferometer for upper atmosphere research [J].
Wu, Q ;
Gablehouse, RD ;
Solomon, SC ;
Killeen, TL ;
She, CY .
INSTRUMENTS, SCIENCE, AND METHODS FOR GEOSPACE AND PLANETARY REMOTE SENSING, 2004, 5660 :218-227
[62]   Observational facts in revealing a close relation between acoustic-gravity waves and midlatitude spread F [J].
Xiao, Sai-guan ;
Xiao, Zuo ;
Shi, Jian-kui ;
Zhang, Dong-he ;
Feng, Xue-shang ;
Hao, Yong-qiang ;
Huang, Wei-quan .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2009, 114
[63]   Analysis of equatorial plasma bubble zonal drift velocities in the Pacific sector by imaging techniques [J].
Yao, D. ;
Makela, J. J. .
ANNALES GEOPHYSICAE, 2007, 25 (03) :701-709
[64]   Three-dimensional simulation of the coupled Perkins and Es-layer instabilities in the nighttime midlatitude ionosphere [J].
Yokoyama, Tatsuhiro ;
Hysell, David L. ;
Otsuka, Yuichi ;
Yamamoto, Mamoru .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2009, 114
[65]   First three-dimensional simulation of the Perkins instability in the nighttime midlatitude ionosphere [J].
Yokoyama, Tatsuhiro ;
Otsuka, Yuichi ;
Ogawa, Tadahiko ;
Yamamoto, Mamoru ;
Hysell, David L. .
GEOPHYSICAL RESEARCH LETTERS, 2008, 35 (03)
[66]   FPI observations of nighttime mesospheric and thermospheric winds in China and their comparisons with HWM07 [J].
Yuan, W. ;
Liu, X. ;
Xu, J. ;
Zhou, Q. ;
Jiang, G. ;
Ma, R. .
ANNALES GEOPHYSICAE, 2013, 31 (08) :1365-1378