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Table 3:

The details of the filling factor calculations, for the O V emission of the sunspot plume observed in 2006.

Line (${\AA}$)
I $\rm {log}$  $N_{\rm {e}}$ $G(T_{\rm {max}},N_{\rm {e}})$ $L~\rm {(Mm)}$ f

758.68
190.77 10.12 $2.81\times10^{-25}$ 0.5 0.096
        7.0 0.007
759.43 154.72 10.09 $2.15\times10^{-25}$ 0.5 0.120
        7.0 0.009
761.99 202.43 10.03 $2.61\times10^{-25}$ 0.5 0.160
        7.0 0.012
774.51 44.19 10.03 $5.54\times10^{-26}$ 0.5 0.170
        7.0 0.012
The units of I, $N_{\rm {e}}$ and $G(T_{\rm {max}},N_{\rm {e}})$ are $\rm {erg~cm^{-2}~s^{-1}~sr^{-1}}$, $\rm {cm}^{-3}$
and $\rm {erg~cm^{-3}~s^{-1}~sr^{-1}}$, respectively.

Source LaTeX | All tables | In the text

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