<?xml version='1.0' encoding='UTF-8'?><codeBook xmlns="ddi:codebook:2_5" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="ddi:codebook:2_5 https://ddialliance.org/Specification/DDI-Codebook/2.5/XMLSchema/codebook.xsd" version="2.5"><docDscr><citation><titlStmt><titl>The mechanism of plasma electron hole transverse instability</titl><IDNo agency="DOI">doi:10.7910/DVN/X6XQTM</IDNo></titlStmt><distStmt><distrbtr source="archive">Harvard Dataverse</distrbtr><distDate>2018-09-25</distDate></distStmt><verStmt source="archive"><version date="2018-09-25" type="RELEASED">1</version></verStmt><biblCit>I. H. Hutchinson, 2018, "The mechanism of plasma electron hole transverse instability", https://doi.org/10.7910/DVN/X6XQTM, Harvard Dataverse, V1, UNF:6:VCd4fG0yqyI1tXZGUsdMYA== [fileUNF]</biblCit></citation></docDscr><stdyDscr><citation><titlStmt><titl>The mechanism of plasma electron hole transverse instability</titl><IDNo agency="DOI">doi:10.7910/DVN/X6XQTM</IDNo></titlStmt><rspStmt><AuthEnty>I. H. Hutchinson</AuthEnty></rspStmt><prodStmt/><distStmt><distrbtr source="archive">Harvard Dataverse</distrbtr></distStmt><holdings URI="https://doi.org/10.7910/DVN/X6XQTM"/></citation><stdyInfo><subject><keyword xml:lang="en">Physics</keyword><keyword>holes</keyword><keyword>instability</keyword><keyword>nonlinear theory</keyword><keyword>PIC</keyword><keyword>space plasmas</keyword></subject><abstract>It is shown through multidimensional particle-in-cell simulation that the transverse instability of plasma electron holes is caused   not by the previously proposed focusing of trapped particles, but   instead by kinematic jetting of marginally passing electrons. The   mechanism is explained and heuristic analytic estimates obtained   which agree with the growth rates and transverse wave-numbers   observed in the simulations.</abstract><sumDscr/><notes>&lt;a href="http://library.psfc.mit.edu/catalog/reports/2010/18ja/18ja003/abstract.php">PSFC REPORT PSFC/JA-18-3&lt;/a>&lt;br />&lt;br />This work was partially supported by NASA grant NNX16AG82G. Computer simulations were carried out on the MIT PSFC parallel AMD Opteron/Infiniband cluster Loki, and on the MIT-PSFC partition of the Engaging cluster at the MGHPCC facility (www.mghpcc.org) which was funded by DoE grant number DE-FG02-91-ER54109.</notes></stdyInfo><method><dataColl><sources/></dataColl><anlyInfo/></method><dataAccs><setAvail/><useStmt/><notes type="DVN:TOU" level="dv">This dataset is made available without information on how it can be used. 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