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  J/A+A/552/A114
 Sun chromospheric CaII-HK emission (Shapiro+, 2013)
model
  
    J/A+A/552/A114/table1Variability long-term VLT=0%, V11=0.00044mag, no secular changes of the chromospheric activity (upper-left panel in Fig. 3); [model](plot) (9354 rows)
    J/A+A/552/A114/table2Variability long-term VLT=0.044%, V11=0.00044mag, strong changes of the chromospheric activity (upper-right panel in Fig. 3); [model](plot) (9354 rows)
    J/A+A/552/A114/table3Variability long-term VLT=0.17%, V11=0.00044mag, strong changes of the chromospheric activity (middle-left panel in Fig. 3); [model](plot) (9354 rows)
    J/A+A/552/A114/table4Variability long-term VLT=0.17%, V11=0.00044mag, no secular changes of the chromospheric activity (middle-right panel in Fig. 3); [model](plot) (9354 rows)
    J/A+A/552/A114/table5Variability long-term VLT=0.5%, V11=0.00044mag, strong changes of the chromospheric activity (lower-left panel in Fig. 3); [model](plot) (9354 rows)
    J/A+A/552/A114/table6Variability long-term VLT=0.5%, V11=0.0002mag, no secular changes of the chromospheric activity (lower-right panel in Fig. 3). [model](plot) (9354 rows)

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