TL;DR
The paper discusses how large-aperture ground-based solar telescopes will enhance our understanding of solar phenomena across atmospheric layers through advanced imaging, polarimetry, and spectroscopy, emphasizing multi-wavelength observations.
Contribution
It highlights the scientific potential of next-generation large solar telescopes and outlines key observational strategies for studying solar atmospheric coupling.
Findings
Enhanced imaging, polarimetry, and spectroscopy capabilities with new telescopes
Multi-wavelength observations are essential for understanding atmospheric coupling
Potential to study sunspot penumbrae in greater detail
Abstract
The new generation of ground-based, large-aperture solar telescopes promises to significantly increase our capabilities to understand the many basic phenomena taking place in the Sun at all atmospheric layers and how they relate to each other. A (non-exaustive) summary of the main scientific arguments we have to pursue these impressive technological goals is presented. We illustrate how imaging, polarimetry, and spectroscopy can benefit from the new telescopes and how several wavelength bands should be observed to study the atmospheric coupling from the upper convection zone all the way to the corona. The particular science case of sunspot penumbrae is barely discussed as a specific example.
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