Reconnection properties in Kelvin-Helmholtz instabilities

Autor: Vernisse, Y., Lavraud, B., Eriksson, S., Gershman, D. J., Dorelli, J. C., Pollock, C. J., Giles, B. L., Aunai, N., Avanov, L. A., Burch, J. L., Chandler, Michael O., Coffey, V. N., Dargent, Jérémy, Ergun, R., Farrugia, C. J., Genot, V. N., Graham, Daniel B., Hasegawa, H., Jacquey, C., Kacem, I., Khotyaintsev, Y. V., Li, W., Magnes, W., Marchaudon, A., Moore, T. E., Paterson, W. R., Penou, E., Phan, T., Retinò, Alessandro, Schwartz, S. J., Saito, Y., Sauvaud, J.-A., Schiff, C., Torbert, R. B., Wilder, F. D., Yokota, S.
Přispěvatelé: Institut de recherche en astrophysique et planétologie (IRAP), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique des Plasmas (LPP), Université Paris-Saclay-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11)-École polytechnique (X)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL), Swedish Institute of Space Physics [Uppsala] (IRF)
Jazyk: angličtina
Rok vydání: 2017
Předmět:
Zdroj: 2017 AGU Fall Meeting
2017 AGU Fall Meeting, Dec 2017, New Orleans, Louisiane, United States. pp.SM13B-2377
Popis: International audience; Kelvin-Helmholtz instabilities are particular laboratories to study strong guide field reconnection processes. In particular, unlike the usual dayside magnetopause, the conditions across the magnetopause in KH vortices are quasi-symmetric, with low differences in beta and magnetic shear angle. We study these properties by means of statistical analysis of the high-resolution data of the Magnetospheric Multiscale mission. Several events of Kelvin-Helmholtz instabilities pas the terminator plane and a long lasting dayside instabilities event where used in order to produce this statistical analysis. Early results present a consistency between the data and the theory. In addition, the results emphasize the importance of the thickness of the magnetopause as a driver of magnetic reconnection in low magnetic shear events.
Databáze: OpenAIRE