<?xml version="1.0" encoding="ISO-8859-1"?>
<metadatalist>
	<metadata ReferenceType="Journal Article">
		<site>mtc-m21d.sid.inpe.br 808</site>
		<holdercode>{isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S}</holdercode>
		<identifier>8JMKD3MGP3W34T/4A7L7MB</identifier>
		<repository>sid.inpe.br/mtc-m21d/2023/11.13.13.45</repository>
		<lastupdate>2023:11.13.13.45.51 urlib.net/www/2021/06.04.03.40 administrator</lastupdate>
		<metadatarepository>sid.inpe.br/mtc-m21d/2023/11.13.13.45.51</metadatarepository>
		<metadatalastupdate>2024:05.02.18.31.39 urlib.net/www/2021/06.04.03.40 administrator {D 2023}</metadatalastupdate>
		<doi>10.1029/2023JA031360</doi>
		<issn>2169-9402</issn>
		<label>self-archiving-INPE-MCTIC-GOV-BR</label>
		<citationkey>SilvaSMASAVDRLCWMLDFIL:2023:HiElFl</citationkey>
		<title>High-Energy Electron Flux Enhancement Pattern in the Outer Radiation Belt in Response to the Interplanetary Coronal Mass Ejections</title>
		<year>2023</year>
		<month>Nov.</month>
		<typeofwork>journal article</typeofwork>
		<secondarytype>PRE PI</secondarytype>
		<numberoffiles>1</numberoffiles>
		<size>3843 KiB</size>
		<author>Silva, Ligia Alves da,</author>
		<author>Shi, J.,</author>
		<author>Marchezi, J. P.,</author>
		<author>Agapitov, O. V.,</author>
		<author>Sibeck, D.,</author>
		<author>Alves, Livia Ribeiro,</author>
		<author>Vieira, Luis Eduardo Antunes,</author>
		<author>Deggeroni, Vinicius,</author>
		<author>Resende, Laysa Cristina Araújo,</author>
		<author>Lopez, F.,</author>
		<author>Costa, Joaquim Eduardo Rezende,</author>
		<author>Wang, C.,</author>
		<author>Moro, Juliano,</author>
		<author>Li, H.,</author>
		<author>Dal Lago, Alisson,</author>
		<author>Ferreira, Karen Júlia Coldebella,</author>
		<author>Inostroza Lara, Ana Maria,</author>
		<author>Liu, Z.,</author>
		<resumeid></resumeid>
		<resumeid></resumeid>
		<resumeid></resumeid>
		<resumeid></resumeid>
		<resumeid></resumeid>
		<resumeid></resumeid>
		<resumeid></resumeid>
		<resumeid></resumeid>
		<resumeid></resumeid>
		<resumeid></resumeid>
		<resumeid>8JMKD3MGP5W/3C9JHF8</resumeid>
		<resumeid></resumeid>
		<resumeid></resumeid>
		<resumeid></resumeid>
		<resumeid>8JMKD3MGP5W/3C9JGH3</resumeid>
		<orcid>0000-0002-8822-5030</orcid>
		<orcid></orcid>
		<orcid>0000-0002-2904-6411</orcid>
		<orcid>0000-0001-6427-1596</orcid>
		<orcid>0000-0003-3240-7510</orcid>
		<orcid>0000-0002-5680-7271</orcid>
		<orcid>0000-0002-9376-475X</orcid>
		<orcid>0000-0002-0725-6055</orcid>
		<orcid>0000-0001-6968-6184</orcid>
		<orcid>0000-0001-5881-1365</orcid>
		<orcid></orcid>
		<orcid>0000-0001-6991-9398</orcid>
		<orcid>0000-0003-4078-2222</orcid>
		<orcid></orcid>
		<orcid>0000-0002-4361-6492</orcid>
		<orcid>0000-0001-5498-9430</orcid>
		<group>DIHPA-CGCE-INPE-MCTI-GOV-BR</group>
		<group></group>
		<group></group>
		<group></group>
		<group></group>
		<group>DIHPA-CGCE-INPE-MCTI-GOV-BR</group>
		<group>DIHPA-CGCE-INPE-MCTI-GOV-BR</group>
		<group>GESAST-CEA-DIPGR-INPE-MCTI-GOV-BR</group>
		<group>DICEP-CGCE-INPE-MCTI-GOV-BR</group>
		<group></group>
		<group>DICEP-CGCE-INPE-MCTI-GOV-BR</group>
		<group></group>
		<group>COESU-CGGO-INPE-MCTI-GOV-BR</group>
		<group></group>
		<group>DIHPA-CGCE-INPE-MCTI-GOV-BR</group>
		<group>GESAST-CEA-DIPGR-INPE-MCTI-GOV-BR</group>
		<group>GESATM-CEA-DIPGR-INPE-MCTI-GOV-BR</group>
		<affiliation>Instituto Nacional de Pesquisas Espaciais (INPE)</affiliation>
		<affiliation>Chinese Academy of Sciences</affiliation>
		<affiliation>University of New Hampshire</affiliation>
		<affiliation>University of California</affiliation>
		<affiliation>NASA Goddard Space Flight Center</affiliation>
		<affiliation>Instituto Nacional de Pesquisas Espaciais (INPE)</affiliation>
		<affiliation>Instituto Nacional de Pesquisas Espaciais (INPE)</affiliation>
		<affiliation>Instituto Nacional de Pesquisas Espaciais (INPE)</affiliation>
		<affiliation>Instituto Nacional de Pesquisas Espaciais (INPE)</affiliation>
		<affiliation>The University of Texas</affiliation>
		<affiliation>Instituto Nacional de Pesquisas Espaciais (INPE)</affiliation>
		<affiliation>Chinese Academy of Sciences</affiliation>
		<affiliation>Instituto Nacional de Pesquisas Espaciais (INPE)</affiliation>
		<affiliation>Chinese Academy of Sciences</affiliation>
		<affiliation>Instituto Nacional de Pesquisas Espaciais (INPE)</affiliation>
		<affiliation>Instituto Nacional de Pesquisas Espaciais (INPE)</affiliation>
		<affiliation>Instituto Nacional de Pesquisas Espaciais (INPE)</affiliation>
		<affiliation>Chinese Academy of Sciences</affiliation>
		<electronicmailaddress>ligia.alves01@gmail.com</electronicmailaddress>
		<electronicmailaddress></electronicmailaddress>
		<electronicmailaddress></electronicmailaddress>
		<electronicmailaddress></electronicmailaddress>
		<electronicmailaddress></electronicmailaddress>
		<electronicmailaddress>livia.alves@inpe.br</electronicmailaddress>
		<electronicmailaddress>luis.vieira@inpe.br</electronicmailaddress>
		<electronicmailaddress>vinicius.deggeroni@inpe.br</electronicmailaddress>
		<electronicmailaddress>laysa.resende@inpe.br</electronicmailaddress>
		<electronicmailaddress></electronicmailaddress>
		<electronicmailaddress>joaquim.costa@inpe.br</electronicmailaddress>
		<electronicmailaddress></electronicmailaddress>
		<electronicmailaddress>juliano.moro@inpe.br</electronicmailaddress>
		<electronicmailaddress></electronicmailaddress>
		<electronicmailaddress>alisson.dallago@inpe.br</electronicmailaddress>
		<electronicmailaddress>karen.ferreira@inpe.br</electronicmailaddress>
		<journal>Journal of Geophysical Research: Space Physics</journal>
		<volume>128</volume>
		<number>11</number>
		<pages>e2023JA031360</pages>
		<transferableflag>1</transferableflag>
		<contenttype>External Contribution</contenttype>
		<versiontype>publisher</versiontype>
		<abstract>The high-energy electron flux enhancement pattern in the outer radiation belt is observed under the influence of the Interplanetary Coronal Mass Ejections (ICMEs). Ten events were selected during the Van Allen Probes era, with the high-energy electron flux enhancement starting close to L* = 4. A schematic diagram of the main physical processes responsible for this kind of high-energy electron flux enhancement is presented, considering the energy deposited in the inner magnetosphere under the influence of ICMEs. Superposed Epoch Analysis is applied to the interplanetary medium parameters, the magnetopause standoff distance, the storm-time geomagnetic activity indices, the Ultra-Low Frequency (ULF) waves, and the whistler-mode chorus waves. A compressed magnetopause, Bz component preferentially southward and storm indices considerably high are observed at the beginning of the electron flux enhancements. The modeled parameters of the chorus waves at the dayside/nightside sectors show the high acceleration efficiency at the beginning of the electron flux enhancement pattern II. These results suggest that the local acceleration driven by chorus waves is essential to these electron flux enhancements at low L*. In contrast, although the ULF waves are detected at the beginning of the studied electron flux enhancements, their contribution is insignificant.</abstract>
		<area>CEA</area>
		<language>en</language>
		<targetfile>JGR Space Physics - 2023 - Silva - High&#8208;Energy Electron Flux Enhancement Pattern in the Outer Radiation Belt in Response to.pdf</targetfile>
		<usergroup>simone</usergroup>
		<visibility>shown</visibility>
		<archivingpolicy>denypublisher6 allowfinaldraft</archivingpolicy>
		<readpermission>allow from all</readpermission>
		<documentstage>not transferred</documentstage>
		<nexthigherunit>8JMKD3MGPCW/3F2PBEE</nexthigherunit>
		<nexthigherunit>8JMKD3MGPCW/46KTFK8</nexthigherunit>
		<nexthigherunit>8JMKD3MGPCW/46KUBT5</nexthigherunit>
		<dissemination>WEBSCI; AGU; MGA; COMPENDEX.</dissemination>
		<hostcollection>urlib.net/www/2021/06.04.03.40</hostcollection>
		<username>simone</username>
		<agreement>agreement.html .htaccess .htaccess2</agreement>
		<lasthostcollection>urlib.net/www/2021/06.04.03.40</lasthostcollection>
		<url>http://mtc-m21d.sid.inpe.br/rep-/sid.inpe.br/mtc-m21d/2023/11.13.13.45</url>
	</metadata>
</metadatalist>