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Multi-spacecraft study of the solar wind at solar minimum: Dependence on latitude and transient outflows

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Title: Multi-spacecraft study of the solar wind at solar minimum: Dependence on latitude and transient outflows
Authors: Laker, R
Horbury, TS
Bale, SD
Matteini, L
Woolley, T
Woodham, LD
Stawarz, JE
Davies, EE
Eastwood, JP
Owens, MJ
O'Brien, H
Evans, V
Angelini, V
Richter, I
Heyner, D
Owen, CJ
Louarn, P
Fedorov, A
Item Type: Journal Article
Abstract: Context. The recent launches of Parker Solar Probe, Solar Orbiter (SO), and BepiColombo, along with several older spacecraft, have provided the opportunity to study the solar wind at multiple latitudes and distances from the Sun simultaneously. Aims. We take advantage of this unique spacecraft constellation, along with low solar activity across two solar rotations between May and July 2020, to investigate how the solar wind structure, including the heliospheric current sheet (HCS), varies with latitude. Methods. We visualise the sector structure of the inner heliosphere by ballistically mapping the polarity and solar wind speed from several spacecraft onto the Sun’s source surface. We then assess the HCS morphology and orientation with the in situ data and compare this with a predicted HCS shape. Results. We resolve ripples in the HCS on scales of a few degrees in longitude and latitude, finding that the local orientations of sector boundaries were broadly consistent with the shape of the HCS but were steepened with respect to a modelled HCS at the Sun. We investigate how several CIRs varied with latitude, finding evidence for the compression region affecting slow solar wind outside the latitude extent of the faster stream. We also identified several transient structures associated with HCS crossings and speculate that one such transient may have disrupted the local HCS orientation up to five days after its passage. Conclusions. We have shown that the solar wind structure varies significantly with latitude, with this constellation providing context for solar wind measurements that would not be possible with a single spacecraft. These measurements provide an accurate representation of the solar wind within ±10° latitude, which could be used as a more rigorous constraint on solar wind models and space weather predictions. In the future, this range of latitudes will increase as SO’s orbit becomes more inclined.
Issue Date: 19-Aug-2021
Date of Acceptance: 1-Aug-2021
URI: http://hdl.handle.net/10044/1/91882
DOI: 10.1051/0004-6361/202140679
ISSN: 0004-6361
Publisher: EDP Sciences
Start Page: 1
End Page: 10
Journal / Book Title: Astronomy and Astrophysics: a European journal
Volume: 652
Copyright Statement: © ESO 2021
Sponsor/Funder: Science and Technology Facilities Council (STFC)
Science and Technology Facilities Council (STFC)
Imperial College London
Funder's Grant Number: ST/S000364/1
ST/T001062/1
Keywords: Science & Technology
Physical Sciences
Astronomy & Astrophysics
Sun
coronal mass ejections (CMEs)
solar wind
heliosphere
HELIOSPHERIC CURRENT SHEET
COROTATING INTERACTION REGIONS
CORONAL MASS EJECTIONS
SOURCE-SURFACE
MAGNETIC RECONNECTION
INTERPLANETARY
PLASMA
MODEL
STREAM
AU
Science & Technology
Physical Sciences
Astronomy & Astrophysics
Sun
coronal mass ejections (CMEs)
solar wind
heliosphere
HELIOSPHERIC CURRENT SHEET
COROTATING INTERACTION REGIONS
CORONAL MASS EJECTIONS
SOURCE-SURFACE
MAGNETIC RECONNECTION
INTERPLANETARY
PLASMA
MODEL
STREAM
AU
physics.space-ph
physics.space-ph
astro-ph.SR
Astronomy & Astrophysics
0201 Astronomical and Space Sciences
Publication Status: Published
Article Number: ARTN A105
Online Publication Date: 2021-08-19
Appears in Collections:Space and Atmospheric Physics
Physics