Miniature loops in the solar corona | Astronomy & Astrophysics (A&A)

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Table 1

Imaging data used in this study.

	Band	Contribution	T_peak [MK]^c

Hi-C	193 Å	Fe XII	1.5

	1600 Å	continuum	<0.01
	131 Å	Fe VIII	0.4
	171 Å	Fe IX	0.7
AIA^a	193 Å	Fe XII	1.5
	211 Å	Fe XIV	2.0
	335 Å	Fe XVI	2.8
	94 Å	Fe XVIII	7.1

XRT^b	Ti-Poly	free-free emission	9

Notes.

^(a)

All listed AIA channels are used to co-align the Hi-C observations with the HMI magnetograms, and all but the 1600 Å channel are employed in the DEM analysis (Sect. 5.1).

^(b)

The XRT observations are used for thermal diagnostics.

^(c)

For the Hi-C and AIA bands, T_peak is the temperature of peak ion fraction of the main contributing ion in the respective band according to O’Dwyer et al. (2010). Most AIA bands have significant contributions from other temperatures as well. The value for XRT is taken from Golub et al. (2007).

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