Three-dimensional temperature mapping of solar photospheric fine structure using Ca ii H filtergrams

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Table 3

rms of the observational intensity versus the HD synthetics.

Pos.	Obs.	Obs.	HD	HD
(i)	MOMFBD	filtered		degraded

(1)	27%	18%	38%	19%
(2)	18%	13%	34%	16%
(3)	15%	11%	27%	13%
(4)	12%	10%	20%	11%
(5)	11%	10%	22%	12%
(6)	11%	10%	25%	13%
(7)	12%	12%	30%	14%

Notes. Columns in order: filter position, rms of the quiet Sun patches shown in Fig. 1, rms of the same patches after the most aggressive filtering (Sect. 3.2), rms of the synthesized HD images, and rms of the degraded HD synthetics, including straylight as described in Sect. 4.4.

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