Overview of the HeSP FOV at 246 s after the start of the observations. First row (a–d): magnetic field in the photosphere as determined from a Milne-Eddington inversion of the Fe I 617.3 nm recorded by CRISP. Second row: magnetic field in the chromosphere as determined from the weak-field approximation in the Ca II 854.2 nm (also CRISP data). Bottom two rows: intensity images at various wavelengths. The Hα red wing image is at Δλ = +45 km s⁻¹ from the nominal line core, the Ca II K red wing image at Δλ = +36 km s⁻¹. Panel j shows the intensity normalized to the local continuum intensity I(x, y, λ)/I_cont(x, y), the other panels show the unscaled intensity I(x, y, λ). A movie of this figure showing the entire time series is available online.