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What Happens Before a Southward IMF Turning Reaches the Magnetopause?

Samsonov, AA; Sibeck, DG; Dmitrieva, NP; Semenov, VS; (2017) What Happens Before a Southward IMF Turning Reaches the Magnetopause? Geophysical Research Letters , 44 (18) pp. 9159-9166. 10.1002/2017GL075020. Green open access

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Abstract

Previous observations have shown a ∼10–15 min time delay in the ionospheric response to solar wind directional discontinuities marked by either southward or northward interplanetary magnetic field (IMF) turnings. We have studied one southward IMF turning observed by Time History of Events and Macroscale Interactions during Substorms (THEMIS) and GOES in the dayside magnetosphere. Using a global MHD model, we have reproduced the magnetopause motion in this event. We find that the observed delay in the ground response can be completely explained by deceleration of the directional discontinuity in the subsolar magnetosheath. We show that the speed of the discontinuity significantly decreases in the vicinity of the magnetopause where the magnetic barrier formed during the previous northward IMF interval. The southward turning can reach the magnetopause only after complete disruption of the magnetic barrier. The disruption or dissipation occurs via magnetosheath reconnection, as confirmed by high‐speed jets in the magnetosheath. The magnetopause moves sunward as the directional discontinuity transits the magnetosheath. This sunward motion is followed by the earthward motion when the discontinuity strikes the magnetopause and magnetopause reconnection begins.

Type: Article
Title: What Happens Before a Southward IMF Turning Reaches the Magnetopause?
Open access status: An open access version is available from UCL Discovery
DOI: 10.1002/2017GL075020
Publisher version: http://doi.org/10.1002/2017GL075020
Language: English
Additional information: This version is the version of record. For information on re-use, please refer to the publisher’s terms and conditions.
Keywords: southward IMF turning, magnetosheath reconnection
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
URI: https://discovery-pp.ucl.ac.uk/id/eprint/10048453
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