Detector Development for the Advanced Technology Solar telescope

In recent years, a wealth of observational data from a range of (highly successful) ground- and satellite-based solar facilities has revealed the perplexing and complex nature of the Sun's atmospheric structure and dynamics. This tremendous complexity is a result of the continuous interaction of the plasma motions with the magnetic field. To understand these interactions, we need to observe, model and interpret solar phenomena over a wide range of spatial and temporal scales, and in particular establish the links between the small-scale processes and the large-scale phenomena.

Solar physics research is very strong in the UK and an area of high priority in the STFC Roadmap. The commissioning of the Rapid Oscillations in Solar Atmosphere imager in 2009 allowed the UK community to expand both its user base of ground-based solar facilities and its exploitation of data from such facilities, which can provide higher spatial and temporal resolution that their satellite-based counterparts. For the future, the Advanced Technology Solar Telescope (ATST), under construction by the US National Solar Observatory with first-light expected in 2019, will be a truly revolutionary facility for ground-based solar physics. It will operate in the optical and near-infrared and be the pre-eminent ground-based solar telescope for the foreseeable future. Key advances in its instrumentation over that currently available include ultra-high spatial (25 km on the solar surface) and temporal (millisecond) resolution, high resolution imaging spectroscopy and coronal magnetometry. The first-light science objectives of the ATST are at the core of UK solar physics research programmes, and it is clearly important for the UK community to have access to the facility to remain competitive.

Current UK-led technology has been highlighted as the best option for detectors meeting the science requirements of the ATST. In this proposal we aim to secure UK participation in the ATST and maximise the science return for the UK community at the time of first-light. This will be achieved by a joint programme, funded by STFC, a consortium of UK universities/research institute and industry (Andor Technology plc), on the development of new state-of-the-art detectors for the ATST, plus a set of software tools that will allow the optimal planning of ATST observations and the processing of the resultant datasets.

The main academic benefit for the UK will be dedicated observing time on the world-leading ATST facility, which our solar physics community will be in an excellent position to exploit. In terms of non-academic benefit, the proposed detector development will have a significant socio-economic impact and is therefore in line with the STFC strategy for economic growth through innovation. It will open new technological markets and provide growth and diversity in existing detector markets.

We refer to the Impact Summary to the full PRPP proposal submission coordinated by the lead Institute (Queen Mary Belfast).