O/N2 changes during 1-4 October 2002 storms:: IMAGE SI-13 and TIMED/GUVI observations -: art. no. A10308

被引:155
作者
Zhang, Y
Paxton, LJ
Morrison, D
Wolven, B
Kil, H
Meng, CI
Mende, SB
Immel, TJ
机构
[1] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA
[2] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
关键词
thermospheric composition change; magnetic storm;
D O I
10.1029/2004JA010441
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
[1] Thermospheric O/N-2 column density ratios referenced at a N-2 column density of 10(17) cm(-2) are obtained using the IMAGE SI-13 and TIMED/GUVI far-ultraviolet (FUV) dayglow data, AURIC simulation results, and MSIS86 model. Each of the magnetic storms occurring during a 4-day period ( 1 - 4 October 2002) caused significant O/N-2 depletion that was detected by both of the IMAGE SI-13 and GUVI instruments. The depletion extended down to latitudes of 10degrees and - 5degrees in the Northern and Southern Hemispheres, respectively. Simultaneous measurements show an excellent agreement between the SI-13 and GUVI O/N-2 on both global and local scales. The IMAGE SI-13 O/N-2 data provide direct optical evidence that the O/N-2 depletion corotates with the Earth. The GUVI O/N-2 indicate the depletion in both of the hemispheres is not symmetric owing to the seasonal effect and differences in heating and convection induced winds. Both the IMAGE SI-13 and GUVI O/N-2 maps also provide a good opportunity for future modeling efforts.
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页数:16
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