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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Main Authors: Ting Lan, Chunhua Jiang, Guobin Yang, Yuannong Zhang, Jing Liu, Zhengyu Zhao
Format: Article
Language:English
Published: SpringerOpen 2019-12-01
Series:Earth, Planets and Space
Subjects:
Online Access:https://doi.org/10.1186/s40623-019-1114-7
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spelling 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
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