An explanation for the seasonal dependence of midlatitude sporadic E layers

被引:122
|
作者
Haldoupis, C. [1 ]
Pancheva, D.
Singer, W.
Meek, C.
MacDougall, J.
机构
[1] Univ Crete, Dept Phys, GR-71003 Iraklion, Crete, Greece
[2] Univ Bath, Dept Elect & Elect Engn, Bath BA2 7AY, Avon, England
[3] Leibniz Inst Atmospher Phys, D-18225 Kuhlungsborn, Germany
[4] Univ Saskatchewan, Inst Space & Atmospher Studies, Dept Phys & Engn Phys, Saskatoon, SK S7N 5E2, Canada
[5] Univ Western Ontario, Dept Phys, London, ON N6A 5B9, Canada
关键词
D O I
10.1029/2007JA012322
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
[1] The midlatitude sporadic E layers form when metallic ions of meteoric origin in the lower thermosphere are converged vertically in a wind shear. The occurrence and strength of sporadic E follow a pronounced seasonal dependence marked by a conspicuous summer maximum. Although this is known since the early years of ionosonde studies, its cause has remained a mystery as it cannot be accounted for by the windshear theory of E-s formation. We show here that the marked seasonal dependence of sporadic E correlates well with the annual variation of sporadic meteor deposition in the upper atmosphere. The later has been established recently from long-term measurements using meteor radar interferometers in the Northern and Southern Hemispheres. Knowing that the occurrence and strength of sporadic E layers depends directly on the metal ion content, which apparently is determined primarily by the meteoric deposition, the present study offers a cause-and-effect explanation for the long-going mystery of sporadic E layer seasonal dependence.
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页数:7
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