On the post-sunset rise of the equatorial F layer and superposed upwellings and bubbles
Usual practice has been to describe the post‐sunset rise (PSSR) of the equatorial F layer with the vertical drift velocity measured overhead, as a function of local time, by a ground‐based sensor. However, with the finding that large‐scale wave structure (LSWS) develops with its own eastward polariz...
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Veröffentlicht in: | Geophysical research letters 2007-02, Vol.34 (4), p.n/a |
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description | Usual practice has been to describe the post‐sunset rise (PSSR) of the equatorial F layer with the vertical drift velocity measured overhead, as a function of local time, by a ground‐based sensor. However, with the finding that large‐scale wave structure (LSWS) develops with its own eastward polarization electric field, during a PSSR, the measured upward velocity must now be thought of as containing two components, one associated with PSSR, and the other with LSWS. This distinction may hold the key to understanding the lack of correlation, on a day‐to‐day basis, between measured vertical drift and ensuing plasma structure in the form of plasma bubbles. Measurements of backscatter from the bottomside of the F layer, using a three‐beam radar at Pohnpei, are presented in this paper to further validate this interpretation. |
doi_str_mv | 10.1029/2006GL028832 |
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However, with the finding that large‐scale wave structure (LSWS) develops with its own eastward polarization electric field, during a PSSR, the measured upward velocity must now be thought of as containing two components, one associated with PSSR, and the other with LSWS. This distinction may hold the key to understanding the lack of correlation, on a day‐to‐day basis, between measured vertical drift and ensuing plasma structure in the form of plasma bubbles. 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Res. Lett</addtitle><description>Usual practice has been to describe the post‐sunset rise (PSSR) of the equatorial F layer with the vertical drift velocity measured overhead, as a function of local time, by a ground‐based sensor. However, with the finding that large‐scale wave structure (LSWS) develops with its own eastward polarization electric field, during a PSSR, the measured upward velocity must now be thought of as containing two components, one associated with PSSR, and the other with LSWS. This distinction may hold the key to understanding the lack of correlation, on a day‐to‐day basis, between measured vertical drift and ensuing plasma structure in the form of plasma bubbles. Measurements of backscatter from the bottomside of the F layer, using a three‐beam radar at Pohnpei, are presented in this paper to further validate this interpretation.</description><subject>Earth sciences</subject><subject>Earth, ocean, space</subject><subject>equatorial spread F</subject><subject>Exact sciences and technology</subject><subject>large-scale wave structure</subject><subject>post-sunset rise of equatorial F layer</subject><issn>0094-8276</issn><issn>1944-8007</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2007</creationdate><recordtype>article</recordtype><recordid>eNp9kE1P3DAQhi3USmwXbvwAX8qpoeOPxMkRUVgQK5CWAkfLdiZt2pBkPYlg_32zLGp74jTW-HkfjV7GjgScCJDFVwmQLZYg81zJPTYThdZJDmA-sBlAMb2lyfbZJ6JfAKBAiRl7vG358BN539GQ0NgSDjzWhLyrXve4Ht3Qxdo1_II3boORu7bkNPYYpwyWfOyfsWnq9ge9_vjR-wbpgH2sXEN4-Dbn7P7i_PvZZbK8XVydnS6ToHMBSS6CTFOtRClLbzymvpIi05XGUGkvRB6q3CkdMJM-aANQGuXRaOF0yBCVmrPjnbeP3XpEGuxTTWE6yLXYjWRFkaaZSbfglx0YYkcUsbJ9rJ9c3FgBdtue_b-9Cf_85nUUXFNF14aa_mXyTE7SYuLkjnuuG9y867SL1VJKM_U-Z8kuVNOAL39DLv62mVEmtY83C3snv62guHyw1-oPOJGM1g</recordid><startdate>200702</startdate><enddate>200702</enddate><creator>Tsunoda, Roland T.</creator><creator>Ecklund, Warner L.</creator><general>Blackwell Publishing Ltd</general><general>American Geophysical Union</general><scope>BSCLL</scope><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>F1W</scope><scope>H96</scope><scope>KL.</scope><scope>L.G</scope></search><sort><creationdate>200702</creationdate><title>On the post-sunset rise of the equatorial F layer and superposed upwellings and bubbles</title><author>Tsunoda, Roland T. ; Ecklund, Warner L.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c4810-81c255431d2db7be5bf2164f4ecf4b118cf8a34ce62bc4700d73be741a4c6ee33</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2007</creationdate><topic>Earth sciences</topic><topic>Earth, ocean, space</topic><topic>equatorial spread F</topic><topic>Exact sciences and technology</topic><topic>large-scale wave structure</topic><topic>post-sunset rise of equatorial F layer</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Tsunoda, Roland T.</creatorcontrib><creatorcontrib>Ecklund, Warner L.</creatorcontrib><collection>Istex</collection><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) 2: Ocean Technology, Policy & Non-Living Resources</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) Professional</collection><jtitle>Geophysical research letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Tsunoda, Roland T.</au><au>Ecklund, Warner L.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>On the post-sunset rise of the equatorial F layer and superposed upwellings and bubbles</atitle><jtitle>Geophysical research letters</jtitle><addtitle>Geophys. Res. Lett</addtitle><date>2007-02</date><risdate>2007</risdate><volume>34</volume><issue>4</issue><epage>n/a</epage><issn>0094-8276</issn><eissn>1944-8007</eissn><coden>GPRLAJ</coden><abstract>Usual practice has been to describe the post‐sunset rise (PSSR) of the equatorial F layer with the vertical drift velocity measured overhead, as a function of local time, by a ground‐based sensor. However, with the finding that large‐scale wave structure (LSWS) develops with its own eastward polarization electric field, during a PSSR, the measured upward velocity must now be thought of as containing two components, one associated with PSSR, and the other with LSWS. This distinction may hold the key to understanding the lack of correlation, on a day‐to‐day basis, between measured vertical drift and ensuing plasma structure in the form of plasma bubbles. Measurements of backscatter from the bottomside of the F layer, using a three‐beam radar at Pohnpei, are presented in this paper to further validate this interpretation.</abstract><cop>Washington, DC</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1029/2006GL028832</doi><tpages>5</tpages><oa>free_for_read</oa></addata></record> |
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subjects | Earth sciences Earth, ocean, space equatorial spread F Exact sciences and technology large-scale wave structure post-sunset rise of equatorial F layer |
title | On the post-sunset rise of the equatorial F layer and superposed upwellings and bubbles |
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