Table 2: Imaging instruments. Spatial resolution is given in arcseconds per pixel, temporal cadence in minutes. Note that the Hida and NoRH data are available at much higher cadences, and that the cadence for SXT applies to each specific combination of filters and exposure times.
Instrument/ Wavelength Spatial Temporal Reference Events

Observatory resolution cadence

DHC/KSO H $\alpha$ 2.3 $\approx$ 1 Messerotti et al. (1999) E3, 5, 10

Singer/BBSO H $\alpha$ 1.1 0.5-1 Denker et al. (1999) E7-9, 12

FMT/Hida H $\alpha$ , H $\alpha\pm0.8$ Å 4.2 1 Kurokawa et al. (1995) E2, 4, 6, 11

CHIP/MLSO He I 10 830 Å 2.3 3 MacQueen et al. (1998) E8, 9, 12

EIT/SOHO Fe XII 195 Å 2.6 $\approx$ 15 Delaboudinière et al. (1995) E1-5, 10-12

SXT/Yohkoh 3-45 Å 4.9/9.8 0.5-2 Tsuneta et al. (1991) E2-4, 11

NoRH/Nobeyama 17 GHz 10 0.5 Nakajima et al. (1994) E1, 2, 6, 8

**Table 2:** Imaging instruments. Spatial resolution is given in arcseconds per pixel, temporal cadence in minutes. Note that the Hida and NoRH data are available at much higher cadences, and that the cadence for SXT applies to each specific combination of filters and exposure times.
Instrument/	Wavelength	Spatial	Temporal	Reference	Events
Observatory		resolution	cadence
DHC/KSO	H $\alpha$	2.3	$\approx$ 1	Messerotti et al. (1999)	E3, 5, 10
Singer/BBSO	H $\alpha$	1.1	0.5-1	Denker et al. (1999)	E7-9, 12
FMT/Hida	H $\alpha$ , H $\alpha\pm0.8$ Å	4.2	1	Kurokawa et al. (1995)	E2, 4, 6, 11
CHIP/MLSO	He I 10 830 Å	2.3	3	MacQueen et al. (1998)	E8, 9, 12
EIT/SOHO	Fe XII 195 Å	2.6	$\approx$ 15	Delaboudinière et al. (1995)	E1-5, 10-12
SXT/Yohkoh	3-45 Å	4.9/9.8	0.5-2	Tsuneta et al. (1991)	E2-4, 11
NoRH/Nobeyama	17 GHz	10	0.5	Nakajima et al. (1994)	E1, 2, 6, 8

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