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Switch-off slow shock/rotational discontinuity structures in collisionless magnetic reconnection: What to look for in satellite observations
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2017 (engelsk)Inngår i: Geophysical Research Letters, ISSN 0094-8276, E-ISSN 1944-8007, Vol. 44, nr 8, s. 3447-3455Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

In Innocenti et al. (2015) we have observed and characterized for the first time Petschek-like switch-off slow shock/rotational discontinuity (SO-SS/RD) compound structures in a 2-D fully kinetic simulation of collisionless magnetic reconnection. Observing these structures in the solar wind or in the magnetotail would corroborate the possibility that Petschek exhausts develop in collisionless media as a result of single X point collisionless reconnection. Here we highlight their signatures in simulations with the aim of easing their identification in observations. The most notable signatures include a four-peaked ion current profile in the out-of-plane direction, associated ion distribution functions, increased electron and ion anisotropy downstream the SS, and increased electron agyrotropy downstream the RDs.

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American Geophysical Union (AGU), 2017. Vol. 44, nr 8, s. 3447-3455
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URN: urn:nbn:se:kth:diva-208844DOI: 10.1002/2017GL073092ISI: 000401847500003OAI: oai:DiVA.org:kth-208844DiVA, id: diva2:1108393
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QC 20170612

Tilgjengelig fra: 2017-06-12 Laget: 2017-06-12 Sist oppdatert: 2017-06-12bibliografisk kontrollert

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