Advanced Methods for Analyzing in-Situ Observations of Magnetic Reconnection

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dc.citation.articleNumber68en_US
dc.citation.journalTitleSpace Science Reviewsen_US
dc.citation.volumeNumber220en_US
dc.contributor.authorHasegawa, H.en_US
dc.contributor.authorArgall, M. R.en_US
dc.contributor.authorAunai, N.en_US
dc.contributor.authorBandyopadhyay, R.en_US
dc.contributor.authorBessho, N.en_US
dc.contributor.authorCohen, I. J.en_US
dc.contributor.authorDenton, R. E.en_US
dc.contributor.authorDorelli, J. C.en_US
dc.contributor.authorEgedal, J.en_US
dc.contributor.authorFuselier, S. A.en_US
dc.contributor.authorGarnier, P.en_US
dc.contributor.authorGénot, V.en_US
dc.contributor.authorGraham, D. B.en_US
dc.contributor.authorHwang, K. J.en_US
dc.contributor.authorKhotyaintsev, Y. V.en_US
dc.contributor.authorKorovinskiy, D. B.en_US
dc.contributor.authorLavraud, B.en_US
dc.contributor.authorLenouvel, Q.en_US
dc.contributor.authorLi, T. C.en_US
dc.contributor.authorLiu, Y.-H.en_US
dc.contributor.authorMichotte de Welle, B.en_US
dc.contributor.authorNakamura, T. K. M.en_US
dc.contributor.authorPayne, D. S.en_US
dc.contributor.authorPetrinec, S. M.en_US
dc.contributor.authorQi, Y.en_US
dc.contributor.authorRager, A. C.en_US
dc.contributor.authorReiff, P. H.en_US
dc.contributor.authorSchroeder, J. M.en_US
dc.contributor.authorShuster, J. R.en_US
dc.contributor.authorSitnov, M. I.en_US
dc.contributor.authorStephens, G. K.en_US
dc.contributor.authorSwisdak, M.en_US
dc.contributor.authorTian, A. M.en_US
dc.contributor.authorTorbert, R. B.en_US
dc.contributor.authorTrattner, K. J.en_US
dc.contributor.authorZenitani, S.en_US
dc.contributor.orgRice Space Instituteen_US
dc.date.accessioned2024-10-01T14:03:58Zen_US
dc.date.available2024-10-01T14:03:58Zen_US
dc.date.issued2024en_US
dc.description.abstractThere is ample evidence for magnetic reconnection in the solar system, but it is a nontrivial task to visualize, to determine the proper approaches and frames to study, and in turn to elucidate the physical processes at work in reconnection regions from in-situ measurements of plasma particles and electromagnetic fields. Here an overview is given of a variety of single- and multi-spacecraft data analysis techniques that are key to revealing the context of in-situ observations of magnetic reconnection in space and for detecting and analyzing the diffusion regions where ions and/or electrons are demagnetized. We focus on recent advances in the era of the Magnetospheric Multiscale mission, which has made electron-scale, multi-point measurements of magnetic reconnection in and around Earth’s magnetosphere.en_US
dc.identifier.citationHasegawa, H., Argall, M. R., Aunai, N., Bandyopadhyay, R., Bessho, N., Cohen, I. J., Denton, R. E., Dorelli, J. C., Egedal, J., Fuselier, S. A., Garnier, P., Génot, V., Graham, D. B., Hwang, K. J., Khotyaintsev, Y. V., Korovinskiy, D. B., Lavraud, B., Lenouvel, Q., Li, T. C., … Zenitani, S. (2024). Advanced Methods for Analyzing in-Situ Observations of Magnetic Reconnection. Space Science Reviews, 220(6), 68. https://doi.org/10.1007/s11214-024-01095-wen_US
dc.identifier.digitals11214-024-01095-wen_US
dc.identifier.doihttps://doi.org/10.1007/s11214-024-01095-wen_US
dc.identifier.urihttps://hdl.handle.net/1911/117900en_US
dc.language.isoengen_US
dc.publisherSpringer Natureen_US
dc.rightsExcept where otherwise noted, this work is licensed under a Creative Commons Attribution (CC BY) license.  Permission to reuse, publish, or reproduce the work beyond the terms of the license or beyond the bounds of fair use or other exemptions to copyright law must be obtained from the copyright holder.en_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_US
dc.titleAdvanced Methods for Analyzing in-Situ Observations of Magnetic Reconnectionen_US
dc.typeJournal articleen_US
dc.type.dcmiTexten_US
dc.type.publicationpublisher versionen_US
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