该文首先简要介绍了无线电掩星探测技术及其发展现状和传统Abel变换方法面临的问题。为改进传统Abel变换反演方法,利用电子密度廓线的分离假设,引进了分离假设反演法。随后利用国际电离层参考模式IRI2007给出1000个掩星事件截面的模拟...该文首先简要介绍了无线电掩星探测技术及其发展现状和传统Abel变换方法面临的问题。为改进传统Abel变换反演方法,利用电子密度廓线的分离假设,引进了分离假设反演法。随后利用国际电离层参考模式IRI2007给出1000个掩星事件截面的模拟数据及COSMIC卫星星座的一天实测数据,进行比较计算,并对结果进行了分析,验证了分离假设反演法的有效性。文中还给出了垂直电子总量VTEC(Vertical Total Electron Content)先验场的获取途径。最后,对分离假设反演法的进一步研究的方向进行了探讨。展开更多
The ionospheric scale height around the peak height of F2 layer(HmF2)is a very important parameter defining the profile of topside ionosphere.Based on observations of the EISCAT ESR radar,we statistically study the Hm...The ionospheric scale height around the peak height of F2 layer(HmF2)is a very important parameter defining the profile of topside ionosphere.Based on observations of the EISCAT ESR radar,we statistically study the HmF2 at high latitudes.In order to derive the HmF2,a least square method is adopted to fit the electron density profile above the peak height of F2 layer(hmF2)from observations of the ESR radar.The result shows that it is in well agreement between the topside profiles deduced from the fitted HmF2 and the actual measuring topside profile with a height range from hmF2 to 300 km above the hmF2.Therefore,HmF2 can be considered as a constant in this range.With observations of the ESR between 1997 and 2008,we analyze the statistical characteristics of polar HmF2 with local time,season,and solar activity under quiet geomagnetic conditions(Kp≤2),respectively.Variations of HmF2 in quiet days show a diurnal trend with a maximum in the morning and a minimum in the afternoon.The HmF2 always has the highest seasonal amplitude in summer under three kinds of solar activities.The seasonal magnitude of the HmF2 in winter remains between that in spring and that in autumn under low solar activity,while it is the lowest under moderate and high solar activities.We also compare measured HmF2 with those derived by IRI2007,which indicates that IRI2007 model can only approximately provide the average values of polar HmF2 in quiet days but is limited in presenting diurnal and solar activity variations of HmF2.展开更多
文摘该文首先简要介绍了无线电掩星探测技术及其发展现状和传统Abel变换方法面临的问题。为改进传统Abel变换反演方法,利用电子密度廓线的分离假设,引进了分离假设反演法。随后利用国际电离层参考模式IRI2007给出1000个掩星事件截面的模拟数据及COSMIC卫星星座的一天实测数据,进行比较计算,并对结果进行了分析,验证了分离假设反演法的有效性。文中还给出了垂直电子总量VTEC(Vertical Total Electron Content)先验场的获取途径。最后,对分离假设反演法的进一步研究的方向进行了探讨。
基金The National Natural Science Foundation of China (Grant Nos. 41174140, 41221003 and 41374168)The Research Fund for the Doctoral Program of Higher Education of China (Grant No. 20110141110043)+1 种基金Chinese Academy of Sciences, Program for New Century Excellent Talents in University (Grant No. NCET-13-0446)The Fundamental Research Funds for the Central Universities (Grant No. 2012212020206)
文摘The ionospheric scale height around the peak height of F2 layer(HmF2)is a very important parameter defining the profile of topside ionosphere.Based on observations of the EISCAT ESR radar,we statistically study the HmF2 at high latitudes.In order to derive the HmF2,a least square method is adopted to fit the electron density profile above the peak height of F2 layer(hmF2)from observations of the ESR radar.The result shows that it is in well agreement between the topside profiles deduced from the fitted HmF2 and the actual measuring topside profile with a height range from hmF2 to 300 km above the hmF2.Therefore,HmF2 can be considered as a constant in this range.With observations of the ESR between 1997 and 2008,we analyze the statistical characteristics of polar HmF2 with local time,season,and solar activity under quiet geomagnetic conditions(Kp≤2),respectively.Variations of HmF2 in quiet days show a diurnal trend with a maximum in the morning and a minimum in the afternoon.The HmF2 always has the highest seasonal amplitude in summer under three kinds of solar activities.The seasonal magnitude of the HmF2 in winter remains between that in spring and that in autumn under low solar activity,while it is the lowest under moderate and high solar activities.We also compare measured HmF2 with those derived by IRI2007,which indicates that IRI2007 model can only approximately provide the average values of polar HmF2 in quiet days but is limited in presenting diurnal and solar activity variations of HmF2.
