太阳活动对中山站F2层峰值电子浓度的影响

doi:10.3724/SP.J.1084.2013.00142

极地研究 ›› 2013, Vol. 25 ›› Issue (2): 142-149.DOI: 10.3724/SP.J.1084.2013.00142

太阳活动对中山站F2层峰值电子浓度的影响

徐盛^1,2张北辰²刘瑞源²郭立新¹刘俊明²武业文¹胡红桥²黄德宏²

¹西安电子科技大学理学院，陕西西安 710071； ²中国极地研究中心国家海洋局极地科学重点实验室，上海 200136

收稿日期:2013-02-28 修回日期:2013-03-31 出版日期:2013-06-30 发布日期:2013-06-30
通讯作者: 徐盛
基金资助:
国家自然科学基金;国家重点基础研究发展计划

THE EFFECT OF SOLAR ACTIVITY ON THE N_mF2 AT ZHONGSHAN STATION

Xu Sheng^1,2，Zhang Beichen²，Guo Lixin¹，Liu Ruiyuan²，Liu Junming²，Wu Yewen¹，Hu Hongqiao²，Huang Dehong²

¹Xidian University, Xi’an 710071, China;
²Polar Research Institute of China, Shanghai 200136, China

Received:2013-02-28 Revised:2013-03-31 Online:2013-06-30 Published:2013-06-30

摘要/Abstract

摘要： 利用中山站1995—2006年的电离层垂测数据统计分析了当地电离层F2层峰值电子浓度（N_mF2）对太阳活动变化的依赖性，研究发现在中山站N_mF2月中值随修正太阳10.7厘米通量指数F10.7P增大而增大，其饱和或放大趋势不明显。除冬季12—16 UT、20—2 UT与夏季2—11 UT以外的绝大部分时刻，两者具有良好的线性关系。N_mF2月中值随F10.7P变化斜率随季节、地方时而变化。在日变化中，N_mF2随F10.7P变化斜率极大值出现在磁中午附近，明显大于其他时刻，在夜侧变化斜率整体较小，且在分季和冬季的夜侧以及夏季全天，其斜率随地方时变化不大。在年变化中，日侧斜率最大值出现在两分季，冬季次之，夏季最小；而夜侧斜率在夏半年（10月—3月）整体上要大于冬半年（4月—9月）。结合中山站位于极隙区纬度的特殊地理位置，分析了上述N_mF2变化特征的可能原因。

关键词: 电离层, F2层峰值电子浓度, 太阳10.7厘米通量指数

Abstract: We investigated the solar activity dependence of the ionospheric F2 peak electron density (N_mF2) at Zhongshan Station from 1995 to 2006. We found that N_mF2 increased linearly with solar activity indices. There were also correlations between N_mF2, local time and seasonal changes. Diurnally, N_mF2 was maximal at magnetic noon, larger than other time obviously. There was a weak relationship between N_mF2 and solar activity during the night, with almost no change over time. Annually, the maximum correlation appeared during the equinoxes. There were double peak values in the equinoxes, which were even greater than in the summer of the southern hemisphere. The changes in the slope were relatively smooth in the summer of the southern hemisphere. In the southern hemisphere winter, there was only a change in the slope near the magnetic noon, with almost no changes at other times. At Zhongshan Station, there was usually a strong linear relationship between N_mF2 and P. There was no obvious saturation or amplification effect at Zhongshan compared with middle and low latitudes. We analyzed possible reasons for the N_mF2 variations, linked to the special geographic latitude of the Zhongshan Station.

Key words: ionosphere, F2 layer peak electron density, solar 10.7 cm radio flux

徐盛张北辰刘瑞源郭立新刘俊明武业文胡红桥黄德宏. 太阳活动对中山站F2层峰值电子浓度的影响[J]. 极地研究, 2013, 25(2): 142-149.

Xu Sheng，Zhang Beichen，Guo Lixin，Liu Ruiyuan，Liu Junming，Wu Yewen，Hu Hongqiao，Huang Dehong. THE EFFECT OF SOLAR ACTIVITY ON THE N_mF2 AT ZHONGSHAN STATION[J]. ADVANCES IN POLAR SCIENCE, 2013, 25(2): 142-149.

参考文献

[1] RISHBETH H, C. S. G. K. SETTY. The F-layer at sunrise [J]. J Atmos Terr Phys, 1961, 20(4): 263-76.

[2] RISHBETH H, O. K. GARRIOTT Introduction to Ionospheric Physics [J]. 331 pp Elsevier, 1969,

[3] RISHBETH H. Day-to-day ionospheric variations in a period of high solar activity [J]. J Atmos Terr Phys, 1993, 55(165-71.

[4] RICHARDS P G, D. G. TORR,B. W. REINISCH, GAMACHE, R. R., WILKINSON, P. J. F2 peak electron density at Millstone Hill and Hobart: Comparison of theory and measurement at solar maximum [J]. J GeophysRes, 1994, 99(A8): 15005-16.

[5] RICHARDS P G. Seasonal and solar cycle variations of the ionospheric peak electron density: Comparison of measurement and models [J]. J Geophys Res, 2001, 106(A7): 12803-19.

[6] KAWAMURA S, N. BALAN, Y. OTSUKA, S. FUKAO. Annual and semiannual variations of the midlatitude ionosphere under low solar activity [J]. J Geophys Res, 2002, 107(A8): SIA 8-1-SIA 8-10.

[7] KANE R P. Sunspots, solar radio noise, solar EUV and ionospheric foF2 [J]. J Atmos Terr Phys, 1992, 54(3-4): 463-6.

[8] BALAN N, G. J. BAILEY, B. JENKINS, P. B. RAO, R. J. MOFFETT. Variations of ionospheric ionization and related solar fluxes during an intense solar cycle [J]. J Geophys Res, 1994, 99(A2): 2243-53.

[9] LIU L, WAN W, NING B. Statistical modeling of ionospheric foF2 over Wuhan [J]. Radio Science, 2004, 39(2):

[10] LIU L, WAN W, NING B, et al. Solar activity variations of the ionospheric peak electron density [J]. Journal of Geophysical Research, 2006, 111(A8):

[11] KOURIS S S, J. K. NISSOPOULOS. Variation of foF2 with solar activity [J]. Advances in Space Research, 1994, 14(12): 51-4.

[12] MA R, XU J, WANG W, et al. Seasonal and latitudinal differences of the saturation effect between ionospheric NmF2 and solar activity indices [J]. Journal of Geophysical Research, 2009, 114(A10):

[13] MIKHAILOV A.V. V V M. Solar cycle variations of annual mean noon foF2 [J]. Advances in Space Research, 1995, 15(2): 79-82.

[14] PANCHEVA D, P. MUKHTAROV. A single-station spectral model of the monthly median foF2 and M (3000)F2 [J]. Studia Geophysica et Geodaetica, 1998, 42(2): 183-96.

[15] HINTEREGGER H E, K. FUKUI, B. R. GILSON. Observational, reference and model data on solar EUV, from measurements on AE-E [J]. Geophysical Research Letters, 1981, 8(11): 1147-50.

[16] CHEN Y, LIU L, LE H. Solar activity variations of nighttime ionospheric peak electron density [J]. Journal of Geophysical Research, 2008, 113(A11):

[17] 刘瑞源，贺龙松，钱嵩林. 南极中山站电离层数据集: 1995—1999 [M]. 上海: 上海科学技术文献出版社, 2000.

[18] 刘瑞源，钱嵩林，贺龙松. 南极中山站数字式电离层测高仪的初步观测结果 [J]. 地球物理学进展, 1997, 12(4): 109-18.

[19] 张北辰，刘瑞源，刘顺林. 极区电子沉降对电离层影响的模拟研究 [J]. 地球物理学报, 2001, 44(3): 289-95.

[20] 刘顺林，贺龙松，刘瑞源. 南极中山站冬季电离层的平均特性 [J]. 极地研究, 1997, 19(3):

[21] 朱爱琴，张北辰，黄际英. 南北极冬季F2层电离层特性对比研究 [J]. 极地研究, 2008, 20(1): 31-9.

[22] 何昉，张北辰. 太阳活动低年南北极电离层F2层观测与国际参考电离层对比研究 [J]. 极地研究, 2011, 23(3):

[23] SHEN C. S. Z M Y, WANG J. S., LIU S. L., XU J. Y. Features of the polar ionosphere over the Zhongshan station in Antarctic [J]. Chinese J Geophys (in Chinese), 2005, 48(1): 1-6.

[24] XU Z. H. L R Y, LIU S. L. Variations of the ionospheric F2 layer critical frequency at Zhongshan Station [J]. Chinese J Geophys (in Chinese), 2006, 49(1): 1-8.

[25] MOEN J, X. C. QIU, H. C. CARLSON, R. FUJII, I.W. MCCREA. On the diurnal variability in F2-region plasma density above the EISCAT Svalbard radar [J]. Ann Geophys, 2008, 26(2427-33.

[26] CAI H. T. S Y M, Y. FAN,Y. C. LIU, K. SCHLEGEL. Climatological features of electron density in the polar ionosphere from long-term observations of EISCAT/ESR radar [J]. Ann Geophys, 2007, 25(2561-9.

[27] HE L. S. L R Y, LIU S. L., LIU Y. H. Overall properties of F region around solar minimum at Zhongshan station , Antarctica [J]. Chinese J Geophys (in Chinese) 2000, 43(3): 289-95.

[28] 刘瑞源，杨惠根. 中国极区高空大气物理学观测研究进展 [J]. 极地研究, 2011, 23(4):

[29] HEIKKILA W J, WINNINGHAM, J. D. Penetration of magnetosheath plasma at low altitudes through the dayside magnetospheric cusps [J]. J Geophys Res, 1971, 76(883-97.

[30] CROWLEY G, CARLSON H, BASU S, et al. The dynamic ionospheric polar hole [J]. Radio Science, 1993, 28(3): 401-13.

[31] HEPPNER J, MAYNARD N. Empirical high-latitude electric field models [J]. Journal of Geophysical Research, 1987, 92(A5): 4467-89.

[32] BRINTON H C, GREBOWSKY J M, BRACE L H. The High-Latitude Winter F Region at 300 km: Thermal Plasma Observations from AE-C [J]. Journal of Geophysical Research, 1978, 83(A10): 4767-76.

[33] HEPPNER J P. Empirical models of high-latitude electric fields [J]. Journal of Geophysical Research, 1977, 82(1115-25.

[34] FELDSTEN Y, STARKOV G. Dynamics of auroral belt and polar geomagnetic disturbances [J]. Planetary and Space Science, 1967, 15(2): 209-29.

太阳活动对中山站F2层峰值电子浓度的影响

THE EFFECT OF SOLAR ACTIVITY ON THE N_mF2 AT ZHONGSHAN STATION

PDF (PC)

可视化

摘要/Abstract

引用本文

使用本文

参考文献

相关文章 0

编辑推荐

Metrics

本文评价

太阳活动对中山站F2层峰值电子浓度的影响

THE EFFECT OF SOLAR ACTIVITY ON THE NmF2 AT ZHONGSHAN STATION

PDF (PC)

可视化

摘要/Abstract

引用本文

使用本文

参考文献

相关文章 0

编辑推荐

Metrics

本文评价

THE EFFECT OF SOLAR ACTIVITY ON THE N_mF2 AT ZHONGSHAN STATION