Characterization of horizontal flows around solar pores from high-resolution time series of images

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Table 1:

Characteristics of the time series of solar pores observed from ground-based and satellite facilities.
Telescope	Date 2007	Series	Time, UT	Duration [min]	N. images	Cadence [s]	FOV [ $\hbox{$^{\prime\prime}$ }$ ]
SST	Sep. 30	1	08:43-09:31	48	286	10	$64.3\times 65.0$
SST	Sep. 30	2	09:36-09:56	20	118	10	$64.3\times 65.0$
Hinode	Jun. 1	1	21:35-21:55	20	40	30	$27.9\times 55.7$
	Jun. 1	2	22:26-23:33	67	134	30	$27.9\times 55.7$
	Sep. 30	1	00:14-17:59	960	1030	60	$55.7\times 111.4$

Source LaTeX | All tables | In the text

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