  We present the solar S-index record of cycle 24, obtained by the TIGRE
robotic telescope facility and its high-resolution spectrograph HEROS
(R$\approx$20,000), which measures the solar chromospheric Ca II H&K line
emission by using moonlight. Our calibration process uses the same set of
standard stars as introduced by the Mt. Wilson team, thus giving us a direct
comparison with their huge body of observations taken between 1966 and 1992, as
well as with other cool stars. Carrington cycle 24 activity started from the
unusually deep and long minimum 2008/09, with an S-index average of only 0.154,
by 0.015 deeper than the one of 1986 (<S>=0.169). In this respect,the
chromospheric radiative losses differ remarkably from the variation of the
coronal radio flux F10.7cm and the sunspot numbers. In addition, the cycle 24
S-amplitude remained small, 0.022 (cycles 21 and 22 averaged: 0.024), and so
resulted a very low 2014 maximum of <S>=0.176 (cycles 21 and 22 averaged:
0.193). We argue that this find is significant, since the Ca II H&K line
emission is a good proxy for the solar far-UV flux, which plays an important
role in the heating of the Earth's stratosphere, and we further argue that the
solar far-UV flux changes change s with solar activity much more strongly than
the total solar output.
