70 citations · 401 across the 11 of their papers we have counts for
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astro-ph.SR2022★ 29 cited
Direct observations of a complex coronal web driving highly structured slow solar wind
L. P. Chitta, D. B. Seaton, C. Downs +2
The solar wind consists of continuous streams of charged particles that escape into the heliosphere from the Sun, and is split into fast and slow components, with the fast wind eme…
astro-ph.SR2022★ 56 cited
Defining the Middle Corona
Matthew J. West, Daniel B. Seaton, David B. Wexler +31
The middle corona, the region roughly spanning heliocentric altitudes from to , encompasses almost all of the influential physical transitions and processes that…
astro-ph.SR2022★ 8 cited
The Dynamic Coupling of Streamers and Pseudostreamers to the Heliosphere
V. Aslanyan, D. I. Pontin, A. K. Higginson +3
The slow solar wind is generally believed to result from the interaction of open and closed coronal magnetic flux at streamers and pseudostreamers. We use 3-dimensional magnetohydr…