零星E层发生率中的迁移和非迁移潮汐特征

IF 0.6 Q4 ENGINEERING, ELECTRICAL & ELECTRONIC Advances in Radio Science Pub Date : 2023-03-21 DOI:10.5194/ars-20-85-2023
C. Jacobi, K. Kandieva, C. Arras
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引用次数: 0

摘要

摘要我们分析了FORMOSAT-3/COSMIC星座电离层GPS无线电掩星测量中获得的零星E(ES)层出现率(OR)。最大OR为95–105 海拔公里。中纬度ES层主要是由于潮汐存在时的风切变,最强的信号是迁移的昼夜分量。特别是在南半球,也可以看到非迁移成分,如昼夜西波2和半日西波1,尤其是在高纬度地区。在赤道附近,夏季和秋季出现强烈的日向东波数3分量和半日向东波数2分量。昼夜分量和四分之一日分量比昼夜分量和半日分量弱。
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Migrating and nonmigrating tidal signatures in sporadic E layer occurrence rates
Abstract. We analyse sporadic E (ES) layer occurrence rates (OR) obtained from ionospheric GPS radio occultation measurements by the FORMOSAT-3/COSMIC constellation. Maximum OR are seen at 95–105 km altitude. Midlatitude ES layers are mainly due to wind shear in the presence of tides, and the strongest signals are the migrating diurnal and semidiurnal components. Especially in the Southern Hemisphere, nonmigrating components such as a diurnal westward wave 2 and a semidiurnal westward wave 1 are also visible, especially at higher latitudes. Near the equator, a strong diurnal eastward wavenumber 3 component and a semidiurnal eastward wavenumber 2 component occur in summer and autumn. Terdiurnal and quarterdiurnal components are weaker than the diurnal and semidiurnal ones.
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来源期刊
Advances in Radio Science
Advances in Radio Science ENGINEERING, ELECTRICAL & ELECTRONIC-
CiteScore
0.90
自引率
0.00%
发文量
3
审稿时长
45 weeks
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