Table 2: Exemplary flare distribution properties for the black hole/disk system seen at a moderate inclination, $i=30{\hbox {$^\circ $ }}$. Parameters above the double line are assumed while the parameters below the double line are calculated as described in Sect. 2.2.
\begin{displaymath}{\begin{tabular}{llcrrrrrrrrrrrrr} \hline\hline &\multicolum... ...& 36 & 17 & 25 & 32 & 7.0 & 15 & 28 \\ \hline \end{tabular}} \end{displaymath}
M is the black hole mass in $M_{\odot}$; $R_{\rm {}in}$, $R_{\rm {}out}$ and $R_{\rm {}X}^{\cdots}$ are the disk and the spot characteristic radii in $R_{\rm {}g}=GM/c^2$(radius $R_{\rm {}X}^{\rm {}a}$ of the spot orbit follows from Eq. (11), while $R_{\rm {}X}^{\rm {}b}$ includes correction on finite size of spots); luminosity $L_{\rm {}X}$ is in units of 1044 erg s-1 cm-2; time intervals $t_{\rm {}life}$, $T_{\rm {}obs}$ are in seconds; variances $F_{\rm {}var}^{\cdots}$ are in percent; ( $F_{\rm {}var}^{\rm {}a}$ follows from Eq. (23), $F_{\rm {}var}^{\rm {}b}$ includes the effect of the spot finite size and $F_{\rm {}var}^{\rm {}}$ was obtained numerically at 1 keV with relativistic corrections and finite size of the spots taken into account).

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