  Sun-as-a star observations put our star as a reference for stellar
observations. Here, I review the activities in which the SPACEINN global
seismology team (Working Package WP4.1) has worked during the past 3 years. In
particular, we will explain the new deliverables available on the SPACEINN
seismic+ portal. Moreover, special attention will be given to surface dynamics
(rotation and magnetic fields). After characterizing the rotation and the
magnetic properties of around 300 solar-like stars and defining proper metrics
for that, we use their seismic properties to characterize 18 solar analogues
for which we study their surface magnetic and seismic properties. This allows
us to put the Sun into context compared to its siblings.
