Observational Evidence of S-web Source of the Slow Solar Wind

Observational Evidence of S-web Source of the Slow Solar Wind

From 2022 March 18 to 21, NOAA Active Region (AR) 12967 was tracked simultaneously by Solar Orbiter at 0.35 au and Hinode/EIS at Earth. During this period, strong blueshifted plasma upflows were observed along a thin, dark corridor of open magnetic field originating at the AR’s leading polarity and...

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Bibliographic Details
Main Authors: D. Baker, P. Démoulin, S. L. Yardley, T. Mihailescu, L. van Driel-Gesztelyi, R. D’Amicis, D. M. Long, A. S. H. To, C. J. Owen, T. S. Horbury, D. H. Brooks, D. Perrone, R. J. French, A. W. James, M. Janvier, S. Matthews, M. Stangalini, G. Valori, P. Smith, R. Aznar Cuadrado, H. Peter, U. Schuehle, L. Harra, K. Barczynski, D. Berghmans, A. N. Zhukov, L. Rodriguez, C. Verbeeck
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Slow solar wind
Online Access:https://doi.org/10.3847/1538-4357/acc653

Internet

https://doi.org/10.3847/1538-4357/acc653

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