Markus Roth, Frank Hill, Michael Thompson

SPRING is an evolving concept for next generation solar synoptic observations network. It is envisaged that the new network will cater to the needs of (i) Helioseismology community, by providing improved resolution Doppler observations at multiple heights in solar atmosphere, (ii) Space weather research community, by providing full disk vector magnetograms at a cadence of few minutes and in multiple heights in the solar atmosphere, and (iii) Large solar telescopes, such as DKIST and EAST, by providing high resolution fulldisk context imaging in multiple wavelengths. We will present the conceptual designs currently being explored for SPRING.