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Determination of the Seebeck Coefficient and Other Thermoelectric Parametersusing Specific Resistivity and Concentration of Charge Carriers of N-Si0.96Ge0.04 Alloy Irradiated by 60Co γ-photons 利用 60Co γ 光子辐照 N-Si0.96Ge0.04 合金的比电阻率和电荷载体浓度确定塞贝克系数和其他热电参数
Pub Date : 2024-02-03 DOI: 10.9734/psij/2024/v28i1817
Rafiel Tkhinvaleli, Lasha Loria, Zurab Adamia, Irakli Nakhutsrishvili
The thermoelectric alloy N-Si0.96Ge0.04-P irradiated by 60Co gamma-photons is been studied. The temperature dependences of the Seebeck coefficient, power and electronic quality factors, as well as the universal electrical conductivity and effective masses of electrons in the interval (250400)°C are calculated. All these dependences are different from the results previously obtained for SixGe1-x with other compositions (except for effective mass). This should be associated with a significant difference in specific resistivities and concentrations of charge carriers.
研究了由 60Co γ 光子辐照的 N-Si0.96Ge0.04-P 热电合金。计算了塞贝克系数、功率和电子品质因数的温度相关性,以及(250-400)°C区间的通用导电率和电子有效质量。所有这些依赖关系都不同于之前对其他成分的 SixGe1-x 得出的结果(有效质量除外)。这应该与特定电阻率和电荷载流子浓度的显著差异有关。
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引用次数: 0
Geomagnetic Storm Variation of Vertical Total Electron Content (VTEC) Over Some Euro-African Stations 一些欧非站点上空垂直总电子含量(VTEC)的地磁暴变化
Pub Date : 2024-02-03 DOI: 10.9734/psij/2024/v28i1818
O. J. Ugonabo, E. B. Ugwu, K. Okpala, Godsfavour C. Amanekwe
Geomagnetic storms are events which have physical effects on some ionospheric parameters that, to some extent,affects  the state and dynamics of the ionosphere  with important implications on GNSS applications. Here, the total electron content (TEC) of Brussels (50.80oN, 04.37oE), Madrid (40.43oN, 04.25oW) and Irkutsk (52.22oN, 104.32oE), which are all mid-latitude European stations are compared with Libreville (00.35oN, 09.67oE) and Lusaka (15.43oS, 28.32oE) which are equatorial and low-latitude stations respectively. This study is done over two geomagnetic storms that took place in the solstice period of 2004. Deviations of storm time VTEC from solar quiet (Sq) averages are calculated, analysed and presented. Similarities and differences of storm effects are observed in the European stations with enhancements and depressions. Diurnal solar quiet day variations showed high VTEC during the post-noon hours for all the stations. The VTEC deviations during storm time at Libreville lie within, for Lusaka it is. For the mid-latitude European stations, the deviations are lower such that  is recorded at Brussels while  is recorded for both Irkutsk and Madrid. Enhancement of VTEC during the daytime storm period is attributable to the super-fountain effect caused by the prompt penetration electric fields (PPEFs) into the ionosphere and magnetosphere while low VTEC at night-time is attributed to the process of recombination.   Understanding the behaviour of the ionosphere during geomagnetic storms is important and necessary for a better understanding of the applications of GNSS.
地磁暴是对某些电离层参数产生物理影响的事件,在一定程度上影响电离层的状态和动态,对全球导航卫星系统的应用具有重要影响。在此,将布鲁塞尔(北纬 50.80oN,东经 04.37oE)、马德里(北纬 40.43oN,西经 04.25oW)和伊尔库茨克(北纬 52.22oN,东经 104.32oE)这些欧洲中纬度台站的电子总含量(TEC)分别与利伯维尔(北纬 00.35oN,东经 09.67oE)和卢萨卡(南纬 15.43oS,东经 28.32oE)这些赤道和低纬度台站进行比较。这项研究是针对 2004 年至日期间发生的两次地磁暴进行的。对风暴时间 VTEC 与太阳静止(Sq)平均值的偏差进行了计算、分析和展示。在欧洲观测站观察到了风暴效应的相似和不同之处,有的增强,有的减弱。日静日变化显示,所有观测站午后时段的 VTEC 都很高。利伯维尔暴风雨期间的 VTEC 偏差在以内,卢萨卡则在以内。欧洲中纬度台站的偏差较小,布鲁塞尔的偏差为,而伊尔库茨克和马德里的偏差均为。白天风暴期间的 VTEC 增强可归因于电离层和磁层的快速穿透电场 (PPEFs) 造成的超级喷泉效应,而夜间的 VTEC 偏低可归因于重新组合过程。 了解地磁暴期间电离层的行为对于更好地了解全球导航卫星系统的应用十分重要和必要。
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引用次数: 0
Geomagnetic Storm Variation of Vertical Total Electron Content (VTEC) Over Some Euro-African Stations 一些欧非站点上空垂直总电子含量(VTEC)的地磁暴变化
Pub Date : 2024-02-03 DOI: 10.9734/psij/2024/v28i1818
O. J. Ugonabo, E. B. Ugwu, K. Okpala, Godsfavour C. Amanekwe
Geomagnetic storms are events which have physical effects on some ionospheric parameters that, to some extent,affects  the state and dynamics of the ionosphere  with important implications on GNSS applications. Here, the total electron content (TEC) of Brussels (50.80oN, 04.37oE), Madrid (40.43oN, 04.25oW) and Irkutsk (52.22oN, 104.32oE), which are all mid-latitude European stations are compared with Libreville (00.35oN, 09.67oE) and Lusaka (15.43oS, 28.32oE) which are equatorial and low-latitude stations respectively. This study is done over two geomagnetic storms that took place in the solstice period of 2004. Deviations of storm time VTEC from solar quiet (Sq) averages are calculated, analysed and presented. Similarities and differences of storm effects are observed in the European stations with enhancements and depressions. Diurnal solar quiet day variations showed high VTEC during the post-noon hours for all the stations. The VTEC deviations during storm time at Libreville lie within, for Lusaka it is. For the mid-latitude European stations, the deviations are lower such that  is recorded at Brussels while  is recorded for both Irkutsk and Madrid. Enhancement of VTEC during the daytime storm period is attributable to the super-fountain effect caused by the prompt penetration electric fields (PPEFs) into the ionosphere and magnetosphere while low VTEC at night-time is attributed to the process of recombination.   Understanding the behaviour of the ionosphere during geomagnetic storms is important and necessary for a better understanding of the applications of GNSS.
地磁暴是对某些电离层参数产生物理影响的事件,在一定程度上影响电离层的状态和动态,对全球导航卫星系统的应用具有重要影响。在此,将布鲁塞尔(北纬 50.80oN,东经 04.37oE)、马德里(北纬 40.43oN,西经 04.25oW)和伊尔库茨克(北纬 52.22oN,东经 104.32oE)这些欧洲中纬度台站的电子总含量(TEC)分别与利伯维尔(北纬 00.35oN,东经 09.67oE)和卢萨卡(南纬 15.43oS,东经 28.32oE)这些赤道和低纬度台站进行比较。这项研究是针对 2004 年至日期间发生的两次地磁暴进行的。对风暴时间 VTEC 与太阳静止(Sq)平均值的偏差进行了计算、分析和展示。在欧洲观测站观察到了风暴效应的相似和不同之处,有的增强,有的减弱。日静日变化显示,所有观测站午后时段的 VTEC 都很高。利伯维尔暴风雨期间的 VTEC 偏差在以内,卢萨卡则在以内。欧洲中纬度台站的偏差较小,布鲁塞尔的偏差为,而伊尔库茨克和马德里的偏差均为。白天风暴期间的 VTEC 增强可归因于电离层和磁层的快速穿透电场 (PPEFs) 造成的超级喷泉效应,而夜间的 VTEC 偏低可归因于重新组合过程。 了解地磁暴期间电离层的行为对于更好地了解全球导航卫星系统的应用十分重要和必要。
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引用次数: 0
Determination of the Seebeck Coefficient and Other Thermoelectric Parametersusing Specific Resistivity and Concentration of Charge Carriers of N-Si0.96Ge0.04 Alloy Irradiated by 60Co γ-photons 利用 60Co γ 光子辐照 N-Si0.96Ge0.04 合金的比电阻率和电荷载体浓度确定塞贝克系数和其他热电参数
Pub Date : 2024-02-03 DOI: 10.9734/psij/2024/v28i1817
Rafiel Tkhinvaleli, Lasha Loria, Zurab Adamia, Irakli Nakhutsrishvili
The thermoelectric alloy N-Si0.96Ge0.04-P irradiated by 60Co gamma-photons is been studied. The temperature dependences of the Seebeck coefficient, power and electronic quality factors, as well as the universal electrical conductivity and effective masses of electrons in the interval (250400)°C are calculated. All these dependences are different from the results previously obtained for SixGe1-x with other compositions (except for effective mass). This should be associated with a significant difference in specific resistivities and concentrations of charge carriers.
研究了由 60Co γ 光子辐照的 N-Si0.96Ge0.04-P 热电合金。计算了塞贝克系数、功率和电子品质因数的温度相关性,以及(250-400)°C区间的通用导电率和电子有效质量。所有这些依赖关系都不同于之前对其他成分的 SixGe1-x 得出的结果(有效质量除外)。这应该与特定电阻率和电荷载流子浓度的显著差异有关。
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引用次数: 0
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