印度IGS GPS站观测的第24太阳周期电离层VTEC的长期变化

S. Kundu, S. Sasmal, S. Chakrabarti
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引用次数: 2

摘要

利用印度低纬度IGS站IISC, Bangalore(13.02ᴼN, 77.57ᴼE)的IGS (International Geodesic Survey)双频GPS数据,计算电离层总电子含量(TEC),研究太阳活动的变化。为了研究TEC随太阳活动的变化,我们选择了一个完整的太阳周期24(2007-2020)。我们研究了TEC随太阳黑子数的变化,黑子数是太阳活动的定量指标。我们观察了TEC随太阳通量和极紫外通量等太阳活动参数的变化。估算的TEC在2007 - 2014年期间由最小值逐渐增加到最大值,然后在2015-2020年期间再次减小到最小值,这与太阳黑子数在整个太阳周期内的变化有关。我们利用GPS-TEC数据对整个太阳周期使用EOF分解模型。利用EOF-TEC方法观测了TEC的日、季、年变化及其随太阳活动的变化趋势。EOF-TEC数据与GPS-TEC数据高度相关,相关系数为0.9323。该模型的RMSE值为5.7891,NRMSE值为16%,性能也较好。我们还利用IRI-2016 TEC研究了TEC随太阳活动的日、年变化,并验证了我们的观测数据和模型数据。ir -TEC相对较低,但其对太阳活动的依赖性与GPS-TEC和EOF-TEC值吻合较好。在整个太阳活动周期内,该低纬度站的日TEC在下午13:00-17:00达到最大值。我们观察到,从季节变化来看,GPS-TEC值在春分时最大。分点GPS-TEC最大,其次是冬季和夏季。EOF-TEC也有类似的结果。在整个太阳周期内,TEC、太阳黑子、太阳通量(F10.7 cm)和极紫外通量呈正相关。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Long Term Ionospheric VTEC Variation During Solar cycle 24 as Observed from Indian IGS GPS Station
— We use the IGS (International Geodesic Survey) dual-frequency GPS data of Indian low latitude IGS Station IISC, Bangalore (13.02 ᴼN, 77.57 ᴼE), to compute the Total Electron Content (TEC) to study the solar activity variation of the ionosphere. To study the TEC variation with solar activity, we choose a complete solar cycle 24 during the period 2007-2020. We study the variation of TEC with sunspot numbers which is the quantitative measure of the solar activity. We observe the variation of TEC with the solar activity parameter such as solar flux and the EUV flux. The estimated TEC gradually increases from a minimum to maximum during 2007 to 2014 and then again decreases during 2015-2020 to a minimum which follows the sunspot numbers variation over the complete solar cycle. We use the EOF decomposition model using GPS-TEC data for the entire solar cycle. The diurnal, seasonal, annual TEC variation and its corresponding trend with solar activity are observed using the EOF-TEC method. The EOF-TEC data is highly correlated to GPS-TEC data with a value of correlation coefficient of 0.9323. The performance of the model is also good with the RMSE value of 5.7891 and the NRMSE value is 16%. We also use the IRI-2016 TEC to study the diurnal, annual variation of TEC with solar activity and verify our observed and model data. The IRI-TEC is comparatively low but the solar activity dependence of TEC matches with the GPS-TEC and EOF-TEC values satisfactorily. the diurnal TEC attains a maximum value at the afternoon 13:00-17:00 IST for this low latitude station which is observed for all TEC throughout the solar cycle. We observe that for seasonal variation, the value of GPS-TEC is maximum for the equinox. The equinoctial GPS-TEC is maximum followed by winter and summer. A similar kind of outcome is found in EOF-TEC. We show the positive correlation between TEC, sunspot, solar flux (F10.7 cm), and EUV flux for the entire solar cycle.
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