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Are plasma bubbles a prerequisite for the formation of broad plasma depletions in the equatorial F region?
Formation of broad plasma depletions (BPDs) at night in the equatorial F region is understood in association with plasma bubbles. However, we report BPDs that do not show a connection with bubbles. The characteristics of BPDs are investigated using the observations of the Communication/Navigation Ou...
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Published in: | Geophysical research letters 2013-07, Vol.40 (14), p.3491-3495 |
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creator | Kil, Hyosub Lee, Woo Kyoung |
description | Formation of broad plasma depletions (BPDs) at night in the equatorial F region is understood in association with plasma bubbles. However, we report BPDs that do not show a connection with bubbles. The characteristics of BPDs are investigated using the observations of the Communication/Navigation Outage Forecasting System (C/NOFS) satellite on 31 December 2008, 28 July 2010, and 1 February 2011. On those days, BPDs are detected in the longitude regions where C/NOFS did not detect bubbles prior to the detection of BPDs. The coincident C/NOFS and radar observations over Jicamarca in Peru show the occurrence of BPDs at the time when backscatter echoes are absent and at the height below backscatter echoes. These observations indicate that bubbles are not a prerequisite for those BPDs. The detections of those BPDs can be explained by the uplift of the equatorial F region peak height above the satellite orbit.
Key Points
Equatorial broad plasma depletions develop in the absence of bubbles
Broad plasma depletions occur when the ionosphere is lifted
Broad plasma depletions are the signature of bottomside irregularities |
doi_str_mv | 10.1002/grl.50693 |
format | article |
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Key Points
Equatorial broad plasma depletions develop in the absence of bubbles
Broad plasma depletions occur when the ionosphere is lifted
Broad plasma depletions are the signature of bottomside irregularities</description><identifier>ISSN: 0094-8276</identifier><identifier>EISSN: 1944-8007</identifier><identifier>DOI: 10.1002/grl.50693</identifier><identifier>CODEN: GPRLAJ</identifier><language>eng</language><publisher>Washington, DC: Blackwell Publishing Ltd</publisher><subject>Backscattering ; Bubbles ; Depletion ; Earth sciences ; Earth, ocean, space ; Echoes ; equatorial ionosphere ; Equatorial regions ; Exact sciences and technology ; F region ; Irregularities ; Plasma ; Plasma bubbles</subject><ispartof>Geophysical research letters, 2013-07, Vol.40 (14), p.3491-3495</ispartof><rights>2013. American Geophysical Union. All Rights Reserved.</rights><rights>2014 INIST-CNRS</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c3983-4af7c969850d23f8557ed1df8ed6fa4c422488e8f0b569cc4556c8acfd3f70243</citedby><cites>FETCH-LOGICAL-c3983-4af7c969850d23f8557ed1df8ed6fa4c422488e8f0b569cc4556c8acfd3f70243</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://onlinelibrary.wiley.com/doi/pdf/10.1002%2Fgrl.50693$$EPDF$$P50$$Gwiley$$H</linktopdf><linktohtml>$$Uhttps://onlinelibrary.wiley.com/doi/full/10.1002%2Fgrl.50693$$EHTML$$P50$$Gwiley$$H</linktohtml><link.rule.ids>314,776,780,11494,27903,27904,46446,46870</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=27681536$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>Kil, Hyosub</creatorcontrib><creatorcontrib>Lee, Woo Kyoung</creatorcontrib><title>Are plasma bubbles a prerequisite for the formation of broad plasma depletions in the equatorial F region?</title><title>Geophysical research letters</title><addtitle>Geophys. Res. Lett</addtitle><description>Formation of broad plasma depletions (BPDs) at night in the equatorial F region is understood in association with plasma bubbles. However, we report BPDs that do not show a connection with bubbles. The characteristics of BPDs are investigated using the observations of the Communication/Navigation Outage Forecasting System (C/NOFS) satellite on 31 December 2008, 28 July 2010, and 1 February 2011. On those days, BPDs are detected in the longitude regions where C/NOFS did not detect bubbles prior to the detection of BPDs. The coincident C/NOFS and radar observations over Jicamarca in Peru show the occurrence of BPDs at the time when backscatter echoes are absent and at the height below backscatter echoes. These observations indicate that bubbles are not a prerequisite for those BPDs. The detections of those BPDs can be explained by the uplift of the equatorial F region peak height above the satellite orbit.
Key Points
Equatorial broad plasma depletions develop in the absence of bubbles
Broad plasma depletions occur when the ionosphere is lifted
Broad plasma depletions are the signature of bottomside irregularities</description><subject>Backscattering</subject><subject>Bubbles</subject><subject>Depletion</subject><subject>Earth sciences</subject><subject>Earth, ocean, space</subject><subject>Echoes</subject><subject>equatorial ionosphere</subject><subject>Equatorial regions</subject><subject>Exact sciences and technology</subject><subject>F region</subject><subject>Irregularities</subject><subject>Plasma</subject><subject>Plasma bubbles</subject><issn>0094-8276</issn><issn>1944-8007</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><recordid>eNp1kV1rFDEUhoMouFYv_AcBEfRi2pPJx2SupBS7Ky6VFkvBm5DJJDVrdjJNZtD-e7O7bS8Er07gPM9LeA9CbwkcE4D65DaFYw6ipc_QgrSMVRKgeY4WAG151414iV7lvAEACpQs0OY0WTwGnbcad3PXBZuxxmOyyd7NPvvJYhcTnn7u51ZPPg44OtylqPtHsbdjsLtNxn7Ys0XWU0xeB3yOk70tu0-v0QunQ7ZvHuYRuj7__P1sVa2_Lb-cna4rQ1tJK6ZdY1rRSg59TZ3kvLE96Z20vXCaGVbXTEorHXRctMYwzoWR2rieugZqRo_Qh0PumOLdbPOktj4bG4IebJyzIpwRRqCmO_TdP-gmzmkov1NEsBoo401dqI8HyqSYc7JOjclvdbpXBNSudVVaV_vWC_v-IVFno4NLejA-PwnlAJJwKgp3cuB--2Dv_x-ollfrx-TqYPg82T9Phk6_lGhow9XNxVItv65-XMLqQgn6F2ZBn6Q</recordid><startdate>20130728</startdate><enddate>20130728</enddate><creator>Kil, Hyosub</creator><creator>Lee, Woo Kyoung</creator><general>Blackwell Publishing Ltd</general><general>American Geophysical Union</general><general>John Wiley & Sons, Inc</general><scope>BSCLL</scope><scope>IQODW</scope><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></search><sort><creationdate>20130728</creationdate><title>Are plasma bubbles a prerequisite for the formation of broad plasma depletions in the equatorial F region?</title><author>Kil, Hyosub ; Lee, Woo Kyoung</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c3983-4af7c969850d23f8557ed1df8ed6fa4c422488e8f0b569cc4556c8acfd3f70243</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2013</creationdate><topic>Backscattering</topic><topic>Bubbles</topic><topic>Depletion</topic><topic>Earth sciences</topic><topic>Earth, ocean, space</topic><topic>Echoes</topic><topic>equatorial ionosphere</topic><topic>Equatorial regions</topic><topic>Exact sciences and technology</topic><topic>F region</topic><topic>Irregularities</topic><topic>Plasma</topic><topic>Plasma bubbles</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Kil, Hyosub</creatorcontrib><creatorcontrib>Lee, Woo Kyoung</creatorcontrib><collection>Istex</collection><collection>Pascal-Francis</collection><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>Kil, Hyosub</au><au>Lee, Woo Kyoung</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Are plasma bubbles a prerequisite for the formation of broad plasma depletions in the equatorial F region?</atitle><jtitle>Geophysical research letters</jtitle><addtitle>Geophys. Res. Lett</addtitle><date>2013-07-28</date><risdate>2013</risdate><volume>40</volume><issue>14</issue><spage>3491</spage><epage>3495</epage><pages>3491-3495</pages><issn>0094-8276</issn><eissn>1944-8007</eissn><coden>GPRLAJ</coden><abstract>Formation of broad plasma depletions (BPDs) at night in the equatorial F region is understood in association with plasma bubbles. However, we report BPDs that do not show a connection with bubbles. The characteristics of BPDs are investigated using the observations of the Communication/Navigation Outage Forecasting System (C/NOFS) satellite on 31 December 2008, 28 July 2010, and 1 February 2011. On those days, BPDs are detected in the longitude regions where C/NOFS did not detect bubbles prior to the detection of BPDs. The coincident C/NOFS and radar observations over Jicamarca in Peru show the occurrence of BPDs at the time when backscatter echoes are absent and at the height below backscatter echoes. These observations indicate that bubbles are not a prerequisite for those BPDs. The detections of those BPDs can be explained by the uplift of the equatorial F region peak height above the satellite orbit.
Key Points
Equatorial broad plasma depletions develop in the absence of bubbles
Broad plasma depletions occur when the ionosphere is lifted
Broad plasma depletions are the signature of bottomside irregularities</abstract><cop>Washington, DC</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1002/grl.50693</doi><tpages>5</tpages></addata></record> |
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source | Wiley-Blackwell AGU Digital Archive |
subjects | Backscattering Bubbles Depletion Earth sciences Earth, ocean, space Echoes equatorial ionosphere Equatorial regions Exact sciences and technology F region Irregularities Plasma Plasma bubbles |
title | Are plasma bubbles a prerequisite for the formation of broad plasma depletions in the equatorial F region? |
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