Active region upflows in various coronal structures and their coupling to the lower atmosphere

Open Access

Table C.1.

Parameters used in this study defining the Ne VIII 77.04 nm line PSF, in comparison to parameters reported by Plowman et al. (2023) for the C III 97.7 nm line. Note that the parameters used in this study may not be fully optimized.

Parameter	This Work	Plowman et al. (2023)
F_y₀, c^(a)	2.5″	2.0″
F_λ₀.c^(b)	1.11 Å	0.95 Å
θ_c^(c)	25°	15° or 20°
γ_c^(d)	1.8	1.5
F_y₀, w^(e)	13.0″	10.0″
F_λ₀, w^(f)	4.5 Å	2.5 Å
γ_w^(g)	1.0	1.0
w_w^(h)	0.28	0.2

Notes.

^(a)

PSF core y axis FWHM before rotation or exponentiation.

^(b)

PSF core λ axis FWHM before rotation or exponentiation.

^(c)

PSF core rotation angle.

^(d)

PSF core non-Gaussian exponentiation.

^(e)

PSF wing y axis FWHM before rotation or exponentiation.

^(f)

PSF wing λ axis FWHM before rotation or exponentiation.

^(g)

PSF wing non-Gaussian exponent.

^(h)

Wing weight.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.