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2023 |
Magnetic reconnection as an erosion mechanism for magnetic switchbacks Context. Magnetic switchbacks are localised polarity reversals in the radial component of the heliospheric magnetic field. Observations from Parker Solar Probe (PSP) have shown that they are a prevalent feature of the near-Sun solar wind. However, observations of switchbacks at 1 au and beyond are less frequent, suggesting that these structures evolve and potentially erode as they propagate away from the Sun. The specific mechanisms at play have not been identified thus far. \ Aims: We search for magnetic switchbacks undergo ... Suen, G.~H.~H.; Owen, C.~J.; Verscharen, D.; Horbury, T.~S.; Louarn, P.; De Marco, R.; Published by: \aap Published on: jul YEAR: 2023   DOI: 10.1051/0004-6361/202345922 Parker Data Used; Solar wind; Sun: heliosphere; plasmas; magnetic reconnection; Physics - Space Physics; Astrophysics - Solar and Stellar Astrophysics; Physics - Plasma Physics |
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