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Solar Activity Indices for Ionospheric Parameters in the 23rd and 24th Cycles
Geomagnetism and Aeronomy ( IF 0.7 ) Pub Date : 2020-04-03 , DOI: 10.1134/s0016793220010053 M. G. Deminov , E. V. Nepomnyashchaya , V. N. Obridko
中文翻译:
第23和第24个周期中电离层参数的太阳活动指标
更新日期:2020-04-03
Geomagnetism and Aeronomy ( IF 0.7 ) Pub Date : 2020-04-03 , DOI: 10.1134/s0016793220010053 M. G. Deminov , E. V. Nepomnyashchaya , V. N. Obridko
Abstract—
Characteristics of changes in the solar activity indices (the flux of the solar radio emission at a wavelength of 10.7 cm F and the new version of the relative sunspot number Ri) and the ionospheric index of this activity T in the 23rd and 24th solar cycles, which were low by the amplitude of solar and geomagnetic activity, are analyzed. The running mean over 12 months and smoothed (by a 24-month filter) values of these indices are considered in the analysis. It is found that the relation between the T and F indices was on average stable for these cycles and did not differ from the previous solar cycles. The relation between the T and Ri indices changed with time in the 23rd and 24th cycles and was different from the previous cycles. Moreover, a distinct hysteresis effect in the dependence of the smoothed values of T on Ri was observed in the 24th cycle when different values of T corresponded to a fixed value of Ri in the growing and declining phases of the solar cycle. This effect was absent in the dependence of T on F. Thus, it is confirmed that the F index is a more exact indicator of solar activity for the ionosphere than Ri.中文翻译:
第23和第24个周期中电离层参数的太阳活动指标