Statistical analysis of low-latitude spread F observed over Puer, China, during 2015–2016
Abstract Statistical analysis of spread F (SF), recorded at Puer (PUR, 22.7° N, 101.05° E, Dip Latitude 12.9° N) during 2015–2016, was carried out to reveal its characteristics at the northern equatorial ionization anomaly. In our study, SF was categorized into four types, frequency spread F (FSF),...
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doaj-328d6253d3294d69b7e866e324d29c3b2020-12-13T12:38:57ZengSpringerOpenEarth, Planets and Space1880-59812019-12-017111910.1186/s40623-019-1114-7Statistical analysis of low-latitude spread F observed over Puer, China, during 2015–2016Ting Lan0Chunhua Jiang1Guobin Yang2Yuannong Zhang3Jing Liu4Zhengyu Zhao5Department of Space Physics, School of Electronic Information, Wuhan UniversityDepartment of Space Physics, School of Electronic Information, Wuhan UniversityDepartment of Space Physics, School of Electronic Information, Wuhan UniversityDepartment of Space Physics, School of Electronic Information, Wuhan UniversityInstitute of Earthquake Science, China Earthquake AdministrationDepartment of Space Physics, School of Electronic Information, Wuhan UniversityAbstract Statistical analysis of spread F (SF), recorded at Puer (PUR, 22.7° N, 101.05° E, Dip Latitude 12.9° N) during 2015–2016, was carried out to reveal its characteristics at the northern equatorial ionization anomaly. In our study, SF was categorized into four types, frequency spread F (FSF), range spread F (RSF), mix spread F (MSF) and strong range spread F (SSF). The statistical results presented that FSF and MSF were dominant over Puer. Most types of SF appeared mostly in summer months, except the maximum occurrence of SSF in equinox months. Moreover, observations of SF events also showed that the solar activity and magnetic activity dependence of SF varied with seasons. Compared with observations at other region, the present results suggest that medium-scale traveling ionospheric disturbances (MSTIDs) may play a key role in generation of SF in low-latitude region.https://doi.org/10.1186/s40623-019-1114-7IonosphereSpread FIonosondeMSTIDs |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Ting Lan Chunhua Jiang Guobin Yang Yuannong Zhang Jing Liu Zhengyu Zhao |
spellingShingle |
Ting Lan Chunhua Jiang Guobin Yang Yuannong Zhang Jing Liu Zhengyu Zhao Statistical analysis of low-latitude spread F observed over Puer, China, during 2015–2016 Earth, Planets and Space Ionosphere Spread F Ionosonde MSTIDs |
author_facet |
Ting Lan Chunhua Jiang Guobin Yang Yuannong Zhang Jing Liu Zhengyu Zhao |
author_sort |
Ting Lan |
title |
Statistical analysis of low-latitude spread F observed over Puer, China, during 2015–2016 |
title_short |
Statistical analysis of low-latitude spread F observed over Puer, China, during 2015–2016 |
title_full |
Statistical analysis of low-latitude spread F observed over Puer, China, during 2015–2016 |
title_fullStr |
Statistical analysis of low-latitude spread F observed over Puer, China, during 2015–2016 |
title_full_unstemmed |
Statistical analysis of low-latitude spread F observed over Puer, China, during 2015–2016 |
title_sort |
statistical analysis of low-latitude spread f observed over puer, china, during 2015–2016 |
publisher |
SpringerOpen |
series |
Earth, Planets and Space |
issn |
1880-5981 |
publishDate |
2019-12-01 |
description |
Abstract Statistical analysis of spread F (SF), recorded at Puer (PUR, 22.7° N, 101.05° E, Dip Latitude 12.9° N) during 2015–2016, was carried out to reveal its characteristics at the northern equatorial ionization anomaly. In our study, SF was categorized into four types, frequency spread F (FSF), range spread F (RSF), mix spread F (MSF) and strong range spread F (SSF). The statistical results presented that FSF and MSF were dominant over Puer. Most types of SF appeared mostly in summer months, except the maximum occurrence of SSF in equinox months. Moreover, observations of SF events also showed that the solar activity and magnetic activity dependence of SF varied with seasons. Compared with observations at other region, the present results suggest that medium-scale traveling ionospheric disturbances (MSTIDs) may play a key role in generation of SF in low-latitude region. |
topic |
Ionosphere Spread F Ionosonde MSTIDs |
url |
https://doi.org/10.1186/s40623-019-1114-7 |
work_keys_str_mv |
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