Table 1: Residual intensities $I_{\rm res}$ in the observations at different distances r from the terminator or the solar limb, respectively. See text for details.
Band CN Ca II HG bandbcgcrc
$\lambda$ [nm] 388.3 396.9430.5450.5555.0668.4
Total eclipse
N 4  3  3  3  8  3 
$r = 5\hbox{$^{\prime\prime}$ }$ $2.0 \pm 0.2$[1.7, 2.3] $2.3 \pm 0.6$[2.0, 3.0] $3.4 \pm 0.9$[2.8, 4.4] $2.9 \pm 0.4$[2.4, 3.2] $4.7 \pm 1.5$[1.7, 5.9] $5.3 \pm 1.5$[3.6, 6.4]
$r = 10\hbox{$^{\prime\prime}$ }$ $1.5 \pm 0.2$[1.2, 1.7] $1.9 \pm 0.5$[1.6, 2.4] $2.9 \pm 0.7$[2.4, 3.7] $2.3 \pm 0.3$[2.0, 2.5] $4.2 \pm 1.5$[1.1, 5.3] $4.7 \pm 1.5$[3.0, 5.7]
$r = 20\hbox{$^{\prime\prime}$ }$ $0.8 \pm 0.6$[0.0, 1.3] $1.5 \pm 0.4$[1.3, 2.0] $2.6 \pm 0.6$[2.0, 3.2] $1.9 \pm 0.2$[1.7, 2.1] $3.8 \pm 1.4$[0.8, 4.8] $4.4 \pm 1.4$[2.8, 5.2]
Partial eclipse
N $\ldots$  $\ldots$  9  $\ldots$  $\ldots$  $\ldots$ 
$r = 5\hbox{$^{\prime\prime}$ }$ $\ldots$  $\ldots$  $2.0 \pm 0.8$[1.1, 3.2] $\ldots$  $\ldots$  $\ldots$ 
$r = 10\hbox{$^{\prime\prime}$ }$ $\ldots$  $\ldots$  $1.6 \pm 0.7$[0.9, 2.7] $\ldots$  $\ldots$  $\ldots$ 
$r = 20\hbox{$^{\prime\prime}$ }$ $\ldots$  $\ldots$  $1.4 \pm 0.6$[0.7, 2.2] $\ldots$  $\ldots$  $\ldots$ 
Mercury transit at solar disc-centre
N 8  5  5  5  5  4 
$r = 5\hbox{$^{\prime\prime}$ }$ $5.9 \pm 0.9$[4.9, 6.7] $ 6.2 \pm 0.3$[ 5.7, 6.5] $ 8.1 \pm 0.9$[ 7.1, 9.2] $7.0 \pm 0.7$[6.2, 8.1] $10.3 \pm 0.2$[10.2, 10.6] $11.3 \pm 0.5$[10.7, 12.0]
Mercury transit at solar limb
N $\ldots$  $\ldots$  $\ldots$  $\ldots$  39  $\ldots$ 
$r = 5\hbox{$^{\prime\prime}$ }$             $8.0 \pm 2.2$[6.3, 13.8]   
Solar limb
N $\ldots$  $\ldots$  $\ldots$  66  18  20 
$r = 5\hbox{$^{\prime\prime}$ }$ $\ldots$  $\ldots$  $\ldots$  $5.3 \pm 0.7$[4.3, 6.8] $6.9 \pm 1.1$[5.7, 10.5] $7.9 \pm 1.3$[5.5, 9.9]
$r = 10\hbox{$^{\prime\prime}$ }$ $\ldots$  $\ldots$  $\ldots$  $4.7 \pm 0.6$[3.7, 6.1] $6.4 \pm 1.2$[5.1, 9.9] $7.2 \pm 1.2$[5.0, 9.1]
$r = 20\hbox{$^{\prime\prime}$ }$ $\ldots$  $\ldots$  $\ldots$  $4.0 \pm 0.7$[2.9, 5.7] $6.0 \pm 1.3$[3.6, 9.0] $6.7 \pm 1.1$[5.0, 8.3]


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