Table 6: Abundance enhancement factors (with respect to photospheric composition) for the low FIP elements in the selected segments. $\beta$ is the FIP bias deduced from the observed Mg VI (349.2 Å)/Ne VI (562.8 Å) line intensity ratio as in Young & Mason (1997). The result for Ar in segment 2(1) is not reported because the estimated error is very large.
Region Segment Enhancement factor $\beta$

Al Ca Mg Fe Si O Ar

Extended brightening 1(0) $\rm0.5_{-0.2}^{+0.2}$ $\rm 1.9_{-1.5}^{+0.9}$ $\rm 1.7_{-0.3}^{+0.3}$ $\rm 1.2_{-0.5}^{+0.6}$ $\rm 1.5_{-0.3}^{+0.2}$ $\rm0.6_{-0.2}^{+0.2}$ $\rm 2.1_{-0.9}^{+0.9}$ 3.6

2(1) $\rm 1.1_{-0.5}^{+0.6}$ $\rm 1.7_{-1.0}^{+1.9}$ $\rm 1.9_{-0.3}^{+0.3}$ $\rm 2.2_{-0.7}^{+0.7}$ $\rm 2.3_{-0.5}^{+0.5}$ $\rm0.6_{-0.1}^{+0.2}$ 3.5

Narrow brightening 3(4) $\rm 1.1_{-0.4}^{+0.4}$ $\rm 1.7_{-1.1}^{+1.5}$ $\rm 1.7_{-0.3}^{+0.3}$ $\rm 2.0_{-0.6}^{+0.8}$ $\rm 1.7_{-0.5}^{+0.4}$ $\rm0.9_{-0.1}^{+0.2}$ $\rm 1.8_{-0.8}^{+1.2}$ 3.5

5(7U) $\rm 1.0_{-0.4}^{+0.5}$ $\rm 3.7_{-1.1}^{+1.9}$ $\rm 1.5_{-0.3}^{+0.3}$ $\rm0.9_{-0.3}^{+0.3}$ $\rm 1.0_{-0.2}^{+0.2}$ $\rm0.9_{-0.1}^{+0.2}$ $\rm 1.5_{-0.7}^{+1.0}$ 3.2

7(8U) $\rm0.8_{-0.5}^{+0.4}$ $\rm 4.8_{-1.8}^{+2.8}$ $\rm 1.7_{-0.3}^{+0.3}$ $\rm 1.4_{-0.3}^{+0.5}$ $\rm 1.6_{-0.3}^{+0.4}$ $\rm 1.0_{-0.2}^{+0.2}$ $\rm0.5_{-0.3}^{+0.6}$ 3.2

8(9) $\rm0.9_{-0.6}^{+0.5}$ $\rm 2.1_{-0.6}^{+0.9}$ $\rm 1.7_{-0.3}^{+0.3}$ $\rm0.7_{-0.2}^{+0.3}$ $\rm 1.2_{-0.3}^{+0.2}$ $\rm 1.0_{-0.2}^{+0.2}$ $\rm 1.3_{-0.6}^{+0.8}$ 3.1

Dark regions 4(7L) $\rm 1.1_{-0.8}^{+0.8}$ $\rm 2.6_{-1.0}^{+1.4}$ $\rm0.8_{-0.3}^{+0.3}$ $\rm0.9_{-0.4}^{+0.4}$ $\rm 1.3_{-0.3}^{+0.3}$ $\rm0.7_{-0.1}^{+0.2}$ $\rm 2.3_{-1.3}^{+0.8}$ 1.5

6(8L) $\rm0.6_{-0.5}^{+0.4}$ $\rm 2.3_{-1.7}^{+1.4}$ $\rm 1.2_{-0.3}^{+0.3}$ $\rm0.6_{-0.2}^{+0.2}$ $\rm 1.1_{-0.2}^{+0.2}$ $\rm0.9_{-0.2}^{+0.2}$ $\rm 2.1_{-1.7}^{+1.2}$ 2.6

**Table 6:** Abundance enhancement factors (with respect to photospheric composition) for the low FIP elements in the selected segments. $\beta$ is the FIP bias deduced from the observed Mg VI (349.2 Å)/Ne VI (562.8 Å) line intensity ratio as in Young & Mason (1997). The result for Ar in segment 2(1) is not reported because the estimated error is very large.
Region	Segment	Enhancement factor	$\beta$
		Al	Ca	Mg	Fe	Si	O	Ar
Extended brightening	1(0)	$\rm0.5_{-0.2}^{+0.2}$	$\rm 1.9_{-1.5}^{+0.9}$	$\rm 1.7_{-0.3}^{+0.3}$	$\rm 1.2_{-0.5}^{+0.6}$	$\rm 1.5_{-0.3}^{+0.2}$	$\rm0.6_{-0.2}^{+0.2}$	$\rm 2.1_{-0.9}^{+0.9}$	3.6
	2(1)	$\rm 1.1_{-0.5}^{+0.6}$	$\rm 1.7_{-1.0}^{+1.9}$	$\rm 1.9_{-0.3}^{+0.3}$	$\rm 2.2_{-0.7}^{+0.7}$	$\rm 2.3_{-0.5}^{+0.5}$	$\rm0.6_{-0.1}^{+0.2}$		3.5
Narrow brightening	3(4)	$\rm 1.1_{-0.4}^{+0.4}$	$\rm 1.7_{-1.1}^{+1.5}$	$\rm 1.7_{-0.3}^{+0.3}$	$\rm 2.0_{-0.6}^{+0.8}$	$\rm 1.7_{-0.5}^{+0.4}$	$\rm0.9_{-0.1}^{+0.2}$	$\rm 1.8_{-0.8}^{+1.2}$	3.5
	5(7U)	$\rm 1.0_{-0.4}^{+0.5}$	$\rm 3.7_{-1.1}^{+1.9}$	$\rm 1.5_{-0.3}^{+0.3}$	$\rm0.9_{-0.3}^{+0.3}$	$\rm 1.0_{-0.2}^{+0.2}$	$\rm0.9_{-0.1}^{+0.2}$	$\rm 1.5_{-0.7}^{+1.0}$	3.2
	7(8U)	$\rm0.8_{-0.5}^{+0.4}$	$\rm 4.8_{-1.8}^{+2.8}$	$\rm 1.7_{-0.3}^{+0.3}$	$\rm 1.4_{-0.3}^{+0.5}$	$\rm 1.6_{-0.3}^{+0.4}$	$\rm 1.0_{-0.2}^{+0.2}$	$\rm0.5_{-0.3}^{+0.6}$	3.2
	8(9)	$\rm0.9_{-0.6}^{+0.5}$	$\rm 2.1_{-0.6}^{+0.9}$	$\rm 1.7_{-0.3}^{+0.3}$	$\rm0.7_{-0.2}^{+0.3}$	$\rm 1.2_{-0.3}^{+0.2}$	$\rm 1.0_{-0.2}^{+0.2}$	$\rm 1.3_{-0.6}^{+0.8}$	3.1
Dark regions	4(7L)	$\rm 1.1_{-0.8}^{+0.8}$	$\rm 2.6_{-1.0}^{+1.4}$	$\rm0.8_{-0.3}^{+0.3}$	$\rm0.9_{-0.4}^{+0.4}$	$\rm 1.3_{-0.3}^{+0.3}$	$\rm0.7_{-0.1}^{+0.2}$	$\rm 2.3_{-1.3}^{+0.8}$	1.5
	6(8L)	$\rm0.6_{-0.5}^{+0.4}$	$\rm 2.3_{-1.7}^{+1.4}$	$\rm 1.2_{-0.3}^{+0.3}$	$\rm0.6_{-0.2}^{+0.2}$	$\rm 1.1_{-0.2}^{+0.2}$	$\rm0.9_{-0.2}^{+0.2}$	$\rm 2.1_{-1.7}^{+1.2}$	2.6

Source LaTeX | All tables | In the text

	1 Introduction
	2 Overview of the CDS observing sequence
	3 Data handling
	4 DEM analysis
	5 Conclusions
	References