Dr Adam J. Finley
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adamfinley.bsky.social
Dr Adam J. Finley
@adamfinley.bsky.social
ESA Research Fellow at ESTEC in the Netherlands. Investigating the Sun's magnetic activity, solar wind connection science, and the spin-down of Sun-like stars. Previously a postdoc at CEA Paris-Saclay and PhD at Uni of Exeter.
Towards maximum activity, the heliospheric current sheet became complex and the solar wind sources moved towards the active latitudes. So, for example, an encounter of PSP that spends more time in the solar wind near current sheets will have a smaller Alfvén radii on average. (7/8)
September 10, 2025 at 10:43 AM
A very dipolar magnetic field became inclined to the rotation axis. (6/8)
September 10, 2025 at 10:43 AM
The heliospheric current sheet became warped by the emergence of active regions. (5/8)
September 10, 2025 at 10:43 AM
The evolution of the coronal magnetic field during the solar cycle, strongly influenced the magnetic connectivity of PSP. Each encounter is different, which obscures our perception of the average Alfvén radius. Near minimum, the wind measured by PSP originated closer to the Sun's poles. (4/8)
September 10, 2025 at 10:43 AM
3D view of this plot:
September 2, 2025 at 11:43 AM
Here's the same process applied to the Autumn 2025 remote-sensing window:
July 28, 2025 at 8:56 AM
Here's a comparison of the coronal magnetic field from solar minimum (Dec 2019) and now at solar maximum. The dipole component of the Sun's magnetic field is visibly inclined to the rotation axis.
July 27, 2025 at 2:52 PM