  We present in this reference paper an instrumental project dedicated to the
monitoring of solar activity during solar cycle 25. It concerns the survey of
fast evolving chromospheric events implied in Space Weather, such as flares,
coronal mass ejections, filament instabilities and Moreton waves. Coronal waves
are produced by large flares around the solar maximum and propagate with
chromospheric counterparts; they are rare, faint, difficult to observe, and for
that reason, challenging. They require systematic observations with automatic,
fast and multi-channel optical instruments. MeteoSpace is a high cadence
telescope assembly specially designed for that purpose. The large amount of
data will be freely available to the solar community. We describe in details
the optical design, the qualification tests and capabilities of the telescopes,
and show how waves can be detected. MeteoSpace will be installed at Calern
observatory (C{\^o}te d'Azur, 1270 m) and will be in full operation in 2023.
