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Prominent Daytime TEC Enhancements Under the Quiescent Condition of January 2017
It is well known that the ionospheric electron densities in the F‐region usually undergo day‐to‐day variability with the magnitude of ~20–35%, associated with the solar as well as geomagnetic activities and the meteorological forcing from the lower atmosphere. In this study, we reported remarkable e...
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Published in: | Geophysical research letters 2020-07, Vol.47 (14), p.n/a |
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creator | Huang, Fuqing Lei, Jiuhou Zhang, Ruilong Li, Na Gu, Shengyang Yu, You Liu, Libo Owolabi, Charles Ning, Baiqi Li, Guozhu Zhong, Jiahao Dang, Tong Ren, Dexin Yi, Wen Luan, Xiaoli Xue, Xianghui Yu, Tao Li, Faquan Dou, Xiankang Yoshikawa, Akimasa |
description | It is well known that the ionospheric electron densities in the F‐region usually undergo day‐to‐day variability with the magnitude of ~20–35%, associated with the solar as well as geomagnetic activities and the meteorological forcing from the lower atmosphere. In this study, we reported remarkable enhancements in the total electron content (TEC) from the Beidou geostationary (GEO) satellites during the quiescent geophysical condition of January 2017 prior to the arrival of the sudden stratosphere warming (SSW). The daytime TEC around the equatorial ionization anomaly region increased by 75–160% and lasted for several days. The equatorial electrojet and Sq current in the ionospheric E‐region at low and middle latitudes showed the corresponding increase during the TEC enhancement interval. The possible contributions from the variations of solar EUV flux and geomagnetic activity are ruled out. Our further analysis showed that the diurnal tides in the temperature from Sounding of the Atmosphere using Broadband Emission Radiometry and the solar and lunar semidiurnal tides of neutral winds from two radars over China became strong during this period of interest. These results suggest that the lower atmospheric tidal forcing could contribute to the great and long‐duration TEC enhancement in the ionosphere even though the SSW had not happened yet.
Key Points
The abnormal ionospheric enhancements during the quiescent period were observed by the Beidou GEO TEC
Daytime TEC enhancements reached a magnitude of 75–160% around the EIA region and lasted many days
The meteorological forcing could produce such great ionospheric changes before the SSW arrival |
doi_str_mv | 10.1029/2020GL088398 |
format | article |
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Key Points
The abnormal ionospheric enhancements during the quiescent period were observed by the Beidou GEO TEC
Daytime TEC enhancements reached a magnitude of 75–160% around the EIA region and lasted many days
The meteorological forcing could produce such great ionospheric changes before the SSW arrival</description><identifier>ISSN: 0094-8276</identifier><identifier>EISSN: 1944-8007</identifier><identifier>DOI: 10.1029/2020GL088398</identifier><language>eng</language><publisher>Washington: John Wiley & Sons, Inc</publisher><subject>Atmosphere ; Atmospheric forcing ; Beidou GEO TEC ; BeiDou Navigation Satellite System ; Broadband ; Daytime ; Diurnal ; Diurnal tides ; Diurnal variations ; E region ; EEJ ; Electrojets ; Electron density ; Equatorial electrojet ; Equatorial ionization anomaly ; Equatorial regions ; F region ; Geomagnetic activity ; Geomagnetism ; Ionization ; Ionosphere ; Ionospheric electrons ; ionospheric variations ; Lower atmosphere ; lower atmospheric processes ; Radiometry ; Semidiurnal tides ; Solar EUV ; Sq current ; Sq currents ; SSW ; Stratosphere ; Stratospheric warming ; Tides ; Total Electron Content ; Winds</subject><ispartof>Geophysical research letters, 2020-07, Vol.47 (14), p.n/a</ispartof><rights>2020. American Geophysical Union. All Rights Reserved.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c3722-7e503c870d958d76c9fc2ff7b80f9a6cdd975cae54b011653e5b89800dbc72433</citedby><cites>FETCH-LOGICAL-c3722-7e503c870d958d76c9fc2ff7b80f9a6cdd975cae54b011653e5b89800dbc72433</cites><orcidid>0000-0002-1450-2496 ; 0000-0001-6433-6222 ; 0000-0002-4374-5083 ; 0000-0001-5773-0184 ; 0000-0003-3327-3526 ; 0000-0003-0733-8920 ; 0000-0001-5130-8185 ; 0000-0002-0411-8669 ; 0000-0003-3735-1325 ; 0000-0001-5668-9415 ; 0000-0003-3717-6811 ; 0000-0002-2852-0089 ; 0000-0002-6993-6507 ; 0000-0003-4915-8717 ; 0000-0002-7669-3590 ; 0000-0001-6080-7402 ; 0000-0002-4541-9900</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://onlinelibrary.wiley.com/doi/pdf/10.1029%2F2020GL088398$$EPDF$$P50$$Gwiley$$H</linktopdf><linktohtml>$$Uhttps://onlinelibrary.wiley.com/doi/full/10.1029%2F2020GL088398$$EHTML$$P50$$Gwiley$$H</linktohtml><link.rule.ids>314,780,784,11514,27924,27925,46468,46892</link.rule.ids></links><search><creatorcontrib>Huang, Fuqing</creatorcontrib><creatorcontrib>Lei, Jiuhou</creatorcontrib><creatorcontrib>Zhang, Ruilong</creatorcontrib><creatorcontrib>Li, Na</creatorcontrib><creatorcontrib>Gu, Shengyang</creatorcontrib><creatorcontrib>Yu, You</creatorcontrib><creatorcontrib>Liu, Libo</creatorcontrib><creatorcontrib>Owolabi, Charles</creatorcontrib><creatorcontrib>Ning, Baiqi</creatorcontrib><creatorcontrib>Li, Guozhu</creatorcontrib><creatorcontrib>Zhong, Jiahao</creatorcontrib><creatorcontrib>Dang, Tong</creatorcontrib><creatorcontrib>Ren, Dexin</creatorcontrib><creatorcontrib>Yi, Wen</creatorcontrib><creatorcontrib>Luan, Xiaoli</creatorcontrib><creatorcontrib>Xue, Xianghui</creatorcontrib><creatorcontrib>Yu, Tao</creatorcontrib><creatorcontrib>Li, Faquan</creatorcontrib><creatorcontrib>Dou, Xiankang</creatorcontrib><creatorcontrib>Yoshikawa, Akimasa</creatorcontrib><title>Prominent Daytime TEC Enhancements Under the Quiescent Condition of January 2017</title><title>Geophysical research letters</title><description>It is well known that the ionospheric electron densities in the F‐region usually undergo day‐to‐day variability with the magnitude of ~20–35%, associated with the solar as well as geomagnetic activities and the meteorological forcing from the lower atmosphere. In this study, we reported remarkable enhancements in the total electron content (TEC) from the Beidou geostationary (GEO) satellites during the quiescent geophysical condition of January 2017 prior to the arrival of the sudden stratosphere warming (SSW). The daytime TEC around the equatorial ionization anomaly region increased by 75–160% and lasted for several days. The equatorial electrojet and Sq current in the ionospheric E‐region at low and middle latitudes showed the corresponding increase during the TEC enhancement interval. The possible contributions from the variations of solar EUV flux and geomagnetic activity are ruled out. Our further analysis showed that the diurnal tides in the temperature from Sounding of the Atmosphere using Broadband Emission Radiometry and the solar and lunar semidiurnal tides of neutral winds from two radars over China became strong during this period of interest. These results suggest that the lower atmospheric tidal forcing could contribute to the great and long‐duration TEC enhancement in the ionosphere even though the SSW had not happened yet.
Key Points
The abnormal ionospheric enhancements during the quiescent period were observed by the Beidou GEO TEC
Daytime TEC enhancements reached a magnitude of 75–160% around the EIA region and lasted many days
The meteorological forcing could produce such great ionospheric changes before the SSW arrival</description><subject>Atmosphere</subject><subject>Atmospheric forcing</subject><subject>Beidou GEO TEC</subject><subject>BeiDou Navigation Satellite System</subject><subject>Broadband</subject><subject>Daytime</subject><subject>Diurnal</subject><subject>Diurnal tides</subject><subject>Diurnal variations</subject><subject>E region</subject><subject>EEJ</subject><subject>Electrojets</subject><subject>Electron density</subject><subject>Equatorial electrojet</subject><subject>Equatorial ionization anomaly</subject><subject>Equatorial regions</subject><subject>F region</subject><subject>Geomagnetic activity</subject><subject>Geomagnetism</subject><subject>Ionization</subject><subject>Ionosphere</subject><subject>Ionospheric electrons</subject><subject>ionospheric variations</subject><subject>Lower atmosphere</subject><subject>lower atmospheric processes</subject><subject>Radiometry</subject><subject>Semidiurnal tides</subject><subject>Solar EUV</subject><subject>Sq current</subject><subject>Sq currents</subject><subject>SSW</subject><subject>Stratosphere</subject><subject>Stratospheric warming</subject><subject>Tides</subject><subject>Total Electron Content</subject><subject>Winds</subject><issn>0094-8276</issn><issn>1944-8007</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><recordid>eNp9kNFLwzAQxoMoOKdv_gEBX61ekqZJHqVuUyk4ZXsubZqyjDWZSYvsv7djPvgkHNxx_Pjuuw-hWwIPBKh6pEBhUYCUTMkzNCEqTRMJIM7RBECNMxXZJbqKcQsADBiZoOUy-M4643r8XB162xm8muV45jaV06Yb9xGvXWMC7jcGfwzWRH2Ec-8a21vvsG_xW-WGKhwwBSKu0UVb7aK5-e1TtJ7PVvlLUrwvXvOnItFMUJoIw4FpKaBRXDYi06rVtG1FLaFVVaabRgmuK8PTGgjJODO8lmp8pqm1oCljU3R30t0H_zWY2JdbPwQ3nixpSgXPKBtriu5PlA4-xmDach9sN3otCZTHzMq_mY04PeHfdmcO_7Ll4rPIQBLKfgB6fmsz</recordid><startdate>20200728</startdate><enddate>20200728</enddate><creator>Huang, Fuqing</creator><creator>Lei, Jiuhou</creator><creator>Zhang, Ruilong</creator><creator>Li, Na</creator><creator>Gu, Shengyang</creator><creator>Yu, You</creator><creator>Liu, Libo</creator><creator>Owolabi, Charles</creator><creator>Ning, Baiqi</creator><creator>Li, Guozhu</creator><creator>Zhong, Jiahao</creator><creator>Dang, Tong</creator><creator>Ren, Dexin</creator><creator>Yi, Wen</creator><creator>Luan, Xiaoli</creator><creator>Xue, Xianghui</creator><creator>Yu, Tao</creator><creator>Li, Faquan</creator><creator>Dou, Xiankang</creator><creator>Yoshikawa, Akimasa</creator><general>John Wiley & Sons, Inc</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>7TN</scope><scope>8FD</scope><scope>F1W</scope><scope>FR3</scope><scope>H8D</scope><scope>H96</scope><scope>KL.</scope><scope>KR7</scope><scope>L.G</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0002-1450-2496</orcidid><orcidid>https://orcid.org/0000-0001-6433-6222</orcidid><orcidid>https://orcid.org/0000-0002-4374-5083</orcidid><orcidid>https://orcid.org/0000-0001-5773-0184</orcidid><orcidid>https://orcid.org/0000-0003-3327-3526</orcidid><orcidid>https://orcid.org/0000-0003-0733-8920</orcidid><orcidid>https://orcid.org/0000-0001-5130-8185</orcidid><orcidid>https://orcid.org/0000-0002-0411-8669</orcidid><orcidid>https://orcid.org/0000-0003-3735-1325</orcidid><orcidid>https://orcid.org/0000-0001-5668-9415</orcidid><orcidid>https://orcid.org/0000-0003-3717-6811</orcidid><orcidid>https://orcid.org/0000-0002-2852-0089</orcidid><orcidid>https://orcid.org/0000-0002-6993-6507</orcidid><orcidid>https://orcid.org/0000-0003-4915-8717</orcidid><orcidid>https://orcid.org/0000-0002-7669-3590</orcidid><orcidid>https://orcid.org/0000-0001-6080-7402</orcidid><orcidid>https://orcid.org/0000-0002-4541-9900</orcidid></search><sort><creationdate>20200728</creationdate><title>Prominent Daytime TEC Enhancements Under the Quiescent Condition of January 2017</title><author>Huang, Fuqing ; Lei, Jiuhou ; Zhang, Ruilong ; Li, Na ; Gu, Shengyang ; Yu, You ; Liu, Libo ; Owolabi, Charles ; Ning, Baiqi ; Li, Guozhu ; Zhong, Jiahao ; Dang, Tong ; Ren, Dexin ; Yi, Wen ; Luan, Xiaoli ; Xue, Xianghui ; Yu, Tao ; Li, Faquan ; Dou, Xiankang ; Yoshikawa, Akimasa</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c3722-7e503c870d958d76c9fc2ff7b80f9a6cdd975cae54b011653e5b89800dbc72433</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2020</creationdate><topic>Atmosphere</topic><topic>Atmospheric forcing</topic><topic>Beidou GEO TEC</topic><topic>BeiDou Navigation Satellite System</topic><topic>Broadband</topic><topic>Daytime</topic><topic>Diurnal</topic><topic>Diurnal tides</topic><topic>Diurnal variations</topic><topic>E region</topic><topic>EEJ</topic><topic>Electrojets</topic><topic>Electron density</topic><topic>Equatorial electrojet</topic><topic>Equatorial ionization anomaly</topic><topic>Equatorial regions</topic><topic>F region</topic><topic>Geomagnetic activity</topic><topic>Geomagnetism</topic><topic>Ionization</topic><topic>Ionosphere</topic><topic>Ionospheric electrons</topic><topic>ionospheric variations</topic><topic>Lower atmosphere</topic><topic>lower atmospheric processes</topic><topic>Radiometry</topic><topic>Semidiurnal tides</topic><topic>Solar EUV</topic><topic>Sq current</topic><topic>Sq currents</topic><topic>SSW</topic><topic>Stratosphere</topic><topic>Stratospheric warming</topic><topic>Tides</topic><topic>Total Electron Content</topic><topic>Winds</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Huang, Fuqing</creatorcontrib><creatorcontrib>Lei, Jiuhou</creatorcontrib><creatorcontrib>Zhang, Ruilong</creatorcontrib><creatorcontrib>Li, Na</creatorcontrib><creatorcontrib>Gu, Shengyang</creatorcontrib><creatorcontrib>Yu, You</creatorcontrib><creatorcontrib>Liu, Libo</creatorcontrib><creatorcontrib>Owolabi, Charles</creatorcontrib><creatorcontrib>Ning, Baiqi</creatorcontrib><creatorcontrib>Li, Guozhu</creatorcontrib><creatorcontrib>Zhong, Jiahao</creatorcontrib><creatorcontrib>Dang, Tong</creatorcontrib><creatorcontrib>Ren, Dexin</creatorcontrib><creatorcontrib>Yi, Wen</creatorcontrib><creatorcontrib>Luan, Xiaoli</creatorcontrib><creatorcontrib>Xue, Xianghui</creatorcontrib><creatorcontrib>Yu, Tao</creatorcontrib><creatorcontrib>Li, Faquan</creatorcontrib><creatorcontrib>Dou, Xiankang</creatorcontrib><creatorcontrib>Yoshikawa, Akimasa</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Oceanic Abstracts</collection><collection>Technology Research Database</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>Engineering Research Database</collection><collection>Aerospace Database</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) 2: Ocean Technology, Policy & Non-Living Resources</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Civil Engineering Abstracts</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) Professional</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Geophysical research letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Huang, Fuqing</au><au>Lei, Jiuhou</au><au>Zhang, Ruilong</au><au>Li, Na</au><au>Gu, Shengyang</au><au>Yu, You</au><au>Liu, Libo</au><au>Owolabi, Charles</au><au>Ning, Baiqi</au><au>Li, Guozhu</au><au>Zhong, Jiahao</au><au>Dang, Tong</au><au>Ren, Dexin</au><au>Yi, Wen</au><au>Luan, Xiaoli</au><au>Xue, Xianghui</au><au>Yu, Tao</au><au>Li, Faquan</au><au>Dou, Xiankang</au><au>Yoshikawa, Akimasa</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Prominent Daytime TEC Enhancements Under the Quiescent Condition of January 2017</atitle><jtitle>Geophysical research letters</jtitle><date>2020-07-28</date><risdate>2020</risdate><volume>47</volume><issue>14</issue><epage>n/a</epage><issn>0094-8276</issn><eissn>1944-8007</eissn><abstract>It is well known that the ionospheric electron densities in the F‐region usually undergo day‐to‐day variability with the magnitude of ~20–35%, associated with the solar as well as geomagnetic activities and the meteorological forcing from the lower atmosphere. In this study, we reported remarkable enhancements in the total electron content (TEC) from the Beidou geostationary (GEO) satellites during the quiescent geophysical condition of January 2017 prior to the arrival of the sudden stratosphere warming (SSW). The daytime TEC around the equatorial ionization anomaly region increased by 75–160% and lasted for several days. The equatorial electrojet and Sq current in the ionospheric E‐region at low and middle latitudes showed the corresponding increase during the TEC enhancement interval. The possible contributions from the variations of solar EUV flux and geomagnetic activity are ruled out. Our further analysis showed that the diurnal tides in the temperature from Sounding of the Atmosphere using Broadband Emission Radiometry and the solar and lunar semidiurnal tides of neutral winds from two radars over China became strong during this period of interest. These results suggest that the lower atmospheric tidal forcing could contribute to the great and long‐duration TEC enhancement in the ionosphere even though the SSW had not happened yet.
Key Points
The abnormal ionospheric enhancements during the quiescent period were observed by the Beidou GEO TEC
Daytime TEC enhancements reached a magnitude of 75–160% around the EIA region and lasted many days
The meteorological forcing could produce such great ionospheric changes before the SSW arrival</abstract><cop>Washington</cop><pub>John Wiley & Sons, Inc</pub><doi>10.1029/2020GL088398</doi><tpages>10</tpages><orcidid>https://orcid.org/0000-0002-1450-2496</orcidid><orcidid>https://orcid.org/0000-0001-6433-6222</orcidid><orcidid>https://orcid.org/0000-0002-4374-5083</orcidid><orcidid>https://orcid.org/0000-0001-5773-0184</orcidid><orcidid>https://orcid.org/0000-0003-3327-3526</orcidid><orcidid>https://orcid.org/0000-0003-0733-8920</orcidid><orcidid>https://orcid.org/0000-0001-5130-8185</orcidid><orcidid>https://orcid.org/0000-0002-0411-8669</orcidid><orcidid>https://orcid.org/0000-0003-3735-1325</orcidid><orcidid>https://orcid.org/0000-0001-5668-9415</orcidid><orcidid>https://orcid.org/0000-0003-3717-6811</orcidid><orcidid>https://orcid.org/0000-0002-2852-0089</orcidid><orcidid>https://orcid.org/0000-0002-6993-6507</orcidid><orcidid>https://orcid.org/0000-0003-4915-8717</orcidid><orcidid>https://orcid.org/0000-0002-7669-3590</orcidid><orcidid>https://orcid.org/0000-0001-6080-7402</orcidid><orcidid>https://orcid.org/0000-0002-4541-9900</orcidid></addata></record> |
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subjects | Atmosphere Atmospheric forcing Beidou GEO TEC BeiDou Navigation Satellite System Broadband Daytime Diurnal Diurnal tides Diurnal variations E region EEJ Electrojets Electron density Equatorial electrojet Equatorial ionization anomaly Equatorial regions F region Geomagnetic activity Geomagnetism Ionization Ionosphere Ionospheric electrons ionospheric variations Lower atmosphere lower atmospheric processes Radiometry Semidiurnal tides Solar EUV Sq current Sq currents SSW Stratosphere Stratospheric warming Tides Total Electron Content Winds |
title | Prominent Daytime TEC Enhancements Under the Quiescent Condition of January 2017 |
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