Service-Mode Observations for Ground-Based Solar Physics

TL;DR

This paper discusses the benefits and challenges of implementing service-mode observations at ground-based solar telescopes, highlighting initial experiments with the Dunn Solar Telescope to improve efficiency and scientific output.

Contribution

It presents initial experiences and advantages of adopting service-mode observations for ground-based solar physics, aiming to optimize operational efficiency.

Findings

Successful implementation of service-mode observations at Dunn Solar Telescope

Enhanced flexibility and data collection rates for solar observations

Potential for improved scientific output in future large telescopes

Abstract

There are significant advantages in combining Hinode observations with ground-based instruments that can observe additional spectral diagnostics at higher data rates and with greater flexibility. However, ground-based observations, because of the random effects of weather and seeing as well as the complexities data analysis due to changing instrumental configurations, have traditionally been less efficient than satellite observations in producing useful datasets. Future large ground-based telescopes will need to find new ways to optimize both their operational efficiency and scientific output. We have begun experimenting with service-mode or queue-mode observations at the Dunn Solar Telescope using the Interferometric Bidimensional Spectrometer (IBIS) as part of joint Hinode campaigns. We describe our experiences and the advantages of such an observing mode for solar physics.