As part of our on-going commitment to observing solar oscillations over several magnetic cycles, we are developing a new version of the instrumentation to allow us to have a smaller and more versatile footprint and to update the technology. This work forms part of the PhD project of Steve Hale and is nearing completion. I will report on the successes and some of the issues still to be solved.

I will also note potential synergies with the SONG helioseismic data.