In Situ Measurements of the Variable Slow Solar Wind near Sector Boundaries

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http://hdl.handle.net/10138/308458

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Sanchez-Diaz , E , Rouillard , A P , Lavraud , B , Kilpua , E & Davies , J A 2019 , ' In Situ Measurements of the Variable Slow Solar Wind near Sector Boundaries ' , Astrophysical Journal , vol. 882 , no. 1 , 51 . https://doi.org/10.3847/1538-4357/ab341c

Title: In Situ Measurements of the Variable Slow Solar Wind near Sector Boundaries
Author: Sanchez-Diaz, E.; Rouillard, A. P.; Lavraud, B.; Kilpua, E.; Davies, J. A.
Contributor organization: Space Physics Research Group
Particle Physics and Astrophysics
Department of Physics
Date: 2019-09-01
Language: eng
Number of pages: 12
Belongs to series: Astrophysical Journal
ISSN: 0004-637X
DOI: https://doi.org/10.3847/1538-4357/ab341c
URI: http://hdl.handle.net/10138/308458
Abstract: The release of density structures at the tip of the coronal helmet streamers, likely as a consequence of magnetic reconnection, contributes to the mass flux of the slow solar wind (SSW). In situ measurements in the vicinity of the heliospheric plasma sheet of the magnetic field, protons, and suprathermal electrons reveal details of the processes at play during the formation of density structures near the Sun. In a previous article, we exploited remote-sensing observations to derive a 3D picture of the dynamic evolution of a streamer. We found evidence of the recurrent and continual release of dense blobs from the tip of the streamers. In the present paper, we interpret in situ measurements of the SSW during solar maximum. Through both case and statistical analysis, we show that in situ signatures (magnetic field magnitude, smoothness and rotation, proton density, and suprathermal electrons, in the first place) are consistent with the helmet streamers producing, in alternation, high-density regions (mostly disconnected) separated by magnetic flux ropes (mostly connected to the Sun). This sequence of emission of dense blobs and flux ropes also seems repeated at smaller scales inside each of the high-density regions. These properties are further confirmed with in situ measurements much closer to the Sun using Helios observations. We conclude on a model for the formation of dense blobs and flux ropes that explains both the in situ measurements and the remote-sensing observations presented in our previous studies.
Subject: MAGNETIC RECONNECTION
DENSITY STRUCTURES
CONNECTION
ELECTRONS
MISSION
AU
115 Astronomy, Space science
Peer reviewed: Yes
Rights: unspecified
Usage restriction: openAccess
Self-archived version: acceptedVersion


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