New scientific perspectives emerge for a broad scientific community, e.g. to characterize stellar populations in our Galaxy or to characterize planetary systems by giving model-independent estimates of global properties of stars such as mass, radius, and surface gravity within several percent accuracy, as well as to constrain the age.
Seismic data become a ‘plus’ to be used in conjunction with data of various types and from various sources, e.g. space seismic archives and ground-based spectroscopic surveys, or solar seismic data to be analyzed ‘as a star’ and used as a reference in stellar studies.
The intention of the Seismic+ portal is to bridge over various data types and over different scientific communities.
You can find the Seismic+ Portal by following this link.