Mid-latitude Spread F long-term occurrence characteristics as a function of latitude over Europe

被引:5
作者
Paul, K. S. [1 ]
Haralambous, H. [1 ,2 ]
Singh, A. K. [1 ]
Gulyaeva, T. L. [3 ]
Panchenko, V. A. [3 ]
机构
[1] Frederick Res Ctr, Nicosia, Cyprus
[2] Frederick Univ, Nicosia, Cyprus
[3] IZMIRAN, Moscow 108840, Russia
关键词
Mid-latitude spread F; Latitudinal variation; Solar activity; Travelling ionospheric disturbances; OCCURRENCE PROBABILITY; UPPER-ATMOSPHERE; RANGE SPREAD; IONOSPHERE; MORPHOLOGY; DENSITY; STATION;
D O I
10.1016/j.asr.2022.05.022
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
Mid-latitude spread F has been investigated in past studies, mostly over the Southern Hemisphere. It has been correlated with geomagnetic activity, travelling ionospheric disturbances (TIDs) and F region uplifts, with Perkins instability proposed as the primary seeding mechanism. In this paper, we focus on the latitude effect on the diurnal and seasonal occurrence rate of mid-latitude spread F over the two stations of Nicosia (geographic Lat: 35.29 degrees N, Long: 33.38 degrees E) and Moscow (geographic Lat: 55.50 degrees N, Long: 37.30 degrees E) that reside over the same longitude sector. The period of investigation encompasses a full solar cycle extending from 2009 to 2020. We observe remarkable differences in spread F occurrence characteristics over the two stations both seasonally and diurnally, emphasizing the fact that higher and lower mid-latitude stations over European latitudes are governed by different underlying mechanisms that give rise to spread F events. (C) 2022 COSPAR. Published by Elsevier B.V. All rights reserved.
引用
收藏
页码:710 / 722
页数:13
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