Chromospheric Flashes in a Solar Pore: Insights from Multiline Spectropolarimetric Diagnostics
Solar pores are strongly magnetized regions without a photospheric penumbra, with predominantly vertical magnetic fields. We present a multiline investigation of flashes in a pore using high-resolution Swedish Solar Telescope observations in Fe I 6302, Ca II (λ8542 and K), and Hβ, complemented with (extreme-)UV observations from the Interface
Dubey, Sandeep et al.
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2026