  The Tunka-Grande experiment is a scintillation array with about 0.5 sq.km
sensitive area at Tunka Valley, Siberia, for measuring charged particles and
muons in extensive air showers (EASs). Tunka-Grande is optimized for cosmic ray
studies in the energy range 10 PeV to about 1 EeV, where exploring the
composition is of fundamental importance for understanding the transition from
galactic to extragalactic origin of cosmic rays. This paper attempts to provide
a synopsis of the current results of the experiment. In particular, the
reconstruction of the all-particle energy spectrum in the range of 10 PeV to 1
EeV based on experimental data from four observation seasons is presented.
