采用上流有限元法定量分析了离子迁移率和离子复合率对±800 k V特高压直流输电线路地面合成场强和离子流密度的影响。结果表明,离子迁移率对地面合成场强影响不大,而地面离子流密度随着迁移率的增大呈线性变化;两者均随离子复合率...采用上流有限元法定量分析了离子迁移率和离子复合率对±800 k V特高压直流输电线路地面合成场强和离子流密度的影响。结果表明,离子迁移率对地面合成场强影响不大,而地面离子流密度随着迁移率的增大呈线性变化;两者均随离子复合率的增大而减小,且复合率对地面离子流密度计算的影响大于对地面合成场强的影响。展开更多
The accuracy of dielectronic recombination （DR） data for astrophysics related ions plays a key role in astrophysical plasma modeling. The absolute DR rate coefficient of Fe^17＋ ions was measured at the main cooler ...The accuracy of dielectronic recombination （DR） data for astrophysics related ions plays a key role in astrophysical plasma modeling. The absolute DR rate coefficient of Fe^17＋ ions was measured at the main cooler storage ring at the Institute of Modern Physics, Lanzhou, China. The experimental electron-ion collision energy range covers the first Rydberg series up to n = 24 for the DR resonances associated with the 2p1/2 →^2 p3/2△n= 0 core excitations. A theoretical calculation was performed by using FAC code and compared with the measured DR rate coefficient. Overall reasonable agreement was found between the experimental results and calculations. Moreover, the plasma rate coefficient was deduced from the experimental DR rate coefficient and compared with the available results from the literature. At the low energy range, significant discrepancies were found, and the measured resonances challenge state-of-the-art theory at low collision energies.展开更多
基金Supported by the National Key R&D Program of China(2017YFA0402300)the National Natural Science Foundation of China through(11320101003,U1732133,11611530684)Key Research Program of Frontier Sciences,CAS(QYZDY-SSW-SLH006)
文摘The accuracy of dielectronic recombination （DR） data for astrophysics related ions plays a key role in astrophysical plasma modeling. The absolute DR rate coefficient of Fe^17＋ ions was measured at the main cooler storage ring at the Institute of Modern Physics, Lanzhou, China. The experimental electron-ion collision energy range covers the first Rydberg series up to n = 24 for the DR resonances associated with the 2p1/2 →^2 p3/2△n= 0 core excitations. A theoretical calculation was performed by using FAC code and compared with the measured DR rate coefficient. Overall reasonable agreement was found between the experimental results and calculations. Moreover, the plasma rate coefficient was deduced from the experimental DR rate coefficient and compared with the available results from the literature. At the low energy range, significant discrepancies were found, and the measured resonances challenge state-of-the-art theory at low collision energies.
