基于COSMIC-1(constellation observing system for meteorology,ionosphere and climate-1)掩星的电子密度数据,利用四阶球谐函数建立了全球电离层的电子密度模型,探究了电子密度随经度、纬度、高度、地方时和季节的变化规律。研究结...基于COSMIC-1(constellation observing system for meteorology,ionosphere and climate-1)掩星的电子密度数据,利用四阶球谐函数建立了全球电离层的电子密度模型,探究了电子密度随经度、纬度、高度、地方时和季节的变化规律。研究结果表明:(1)350~550 km处的电子密度主要集中在25°S~25°N的范围内,呈现出明显的地磁纬度相关性;(2)在12:00 UT时,350 km处的电子密度最大,250 km处的电子密度次之,450 km和550 km的电子密度较小;(3)从地方时角度来看,电子密度峰值主要集中在12:00~16:00 LT;(4)从季节变化角度来看,春季和秋季的电子密度峰值最大,冬季次之,夏季最小,这与电离层的半年变化和年度变化一致。该模型能够较好地体现电子密度的变化规律。展开更多
The Total Electron Content (TEC) during three great storms, from April to August 2000, was collected by means of a GPS receiver located in Jingzhou (30.4° N, 112.2° E). The time-latitude-dependent features o...The Total Electron Content (TEC) during three great storms, from April to August 2000, was collected by means of a GPS receiver located in Jingzhou (30.4° N, 112.2° E). The time-latitude-dependent features of ionospheric storms are identified using TEC difference images based on the deviations of TEC during storm relative to quiet time. The responses of ionospheric TEC to magnetic storms were analyzed. The results show that: 1) In middle and low latitude, ionospheric storms effects are more apparent in local day time than at night: 2) Ionospheric storm effects are more dominant near the hump of the equatorial anomaly region than in other regions of TEC measurements; 3) The positive effects during the main phase of ionospheric storm may be caused by electric fields in low latitude; 4) During the recovery period of ionospheric storm, the negative phase of storm may be due to the perturbation of the neutral gas composition.展开更多
The total electron content (TEC) data during the total eclipse of March 9, 1997 were collected, which were observed by means of nine GPS receivers located at the eastern Asia. The responses of total TEC to the eclipse...The total electron content (TEC) data during the total eclipse of March 9, 1997 were collected, which were observed by means of nine GPS receivers located at the eastern Asia. The responses of total TEC to the eclipse were analyzed. The results show that: 1) the eclipse led to apparent decrement in TEC that lasted for six to eight hours; 2) the maximum decrement occurred after the middle of the eclipse with time delays varying from twenty minutes to about three hours; 3) the maximum absolute deviations of TEC on the eclipse day do not show a simple and consistent relationship to the maximum solar obscuration.展开更多
文摘基于COSMIC-1(constellation observing system for meteorology,ionosphere and climate-1)掩星的电子密度数据,利用四阶球谐函数建立了全球电离层的电子密度模型,探究了电子密度随经度、纬度、高度、地方时和季节的变化规律。研究结果表明:(1)350~550 km处的电子密度主要集中在25°S~25°N的范围内,呈现出明显的地磁纬度相关性;(2)在12:00 UT时,350 km处的电子密度最大,250 km处的电子密度次之,450 km和550 km的电子密度较小;(3)从地方时角度来看,电子密度峰值主要集中在12:00~16:00 LT;(4)从季节变化角度来看,春季和秋季的电子密度峰值最大,冬季次之,夏季最小,这与电离层的半年变化和年度变化一致。该模型能够较好地体现电子密度的变化规律。
基金the National Natural Science Foundation of China(499840 0 1)
文摘The Total Electron Content (TEC) during three great storms, from April to August 2000, was collected by means of a GPS receiver located in Jingzhou (30.4° N, 112.2° E). The time-latitude-dependent features of ionospheric storms are identified using TEC difference images based on the deviations of TEC during storm relative to quiet time. The responses of ionospheric TEC to magnetic storms were analyzed. The results show that: 1) In middle and low latitude, ionospheric storms effects are more apparent in local day time than at night: 2) Ionospheric storm effects are more dominant near the hump of the equatorial anomaly region than in other regions of TEC measurements; 3) The positive effects during the main phase of ionospheric storm may be caused by electric fields in low latitude; 4) During the recovery period of ionospheric storm, the negative phase of storm may be due to the perturbation of the neutral gas composition.
文摘The total electron content (TEC) data during the total eclipse of March 9, 1997 were collected, which were observed by means of nine GPS receivers located at the eastern Asia. The responses of total TEC to the eclipse were analyzed. The results show that: 1) the eclipse led to apparent decrement in TEC that lasted for six to eight hours; 2) the maximum decrement occurred after the middle of the eclipse with time delays varying from twenty minutes to about three hours; 3) the maximum absolute deviations of TEC on the eclipse day do not show a simple and consistent relationship to the maximum solar obscuration.
