Speaker
Jorrit Leenaarts
(Stockholm University)
Description
Instrumentation for solar observations always represents a trade-off between spatial resolution, spectral resolution, field-of-view, time-coherence, calibration, and available money. The current state-of-the art for optical and near-infrared wavelengths consists of Fabry-Perot interferometers, and various types of imaging spectrographs.
In this talk I will discuss some aspects of these considerations, and review current and upcoming instrumentation at DKIST, SST, and other observatories.
Primary author
Jorrit Leenaarts
(Stockholm University)
