Innovative Telescopes and Instrumentation for Solar Astrophysics

By S. Keil, S. Avakyan. 2003

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The Polarimetric and Helioseismic Imager on Solar Orbiter (2019, methodology): “…with an instrument in near-Earth orbit (such as SDO/HMI) or on the ground, for instance by telescopes such as the Swedish 1 m Solar Telescope (SST; Scharmer et al. 2003), Gregor (Schmidt et al. 2012), the Goode Solar Telescope (GST; Cao et al. 2010), or the Daniel K. Inouye Solar Telescope…”
CRISPRED: A data pipeline for the CRISP imaging spectropolarimeter (2014, result): “This system (Scharmer et al., in preparation) is similar to the previous system by Scharmer et al. (2003), although it is an upgrade in both hardware and software.”
The Daniel K. Inouye Solar Telescope – Observatory Overview (2020, methodology): “To achieve the telescope scattered-light performance required for sensitive coronal magnetometry, DKIST uses an unobstructed, fast, off-axis optical configuration that recent solar telescopes have adopted (Kuhn et al., 2003; Goode and Cao, 2012a).”
The magnetic field in the solar atmosphere (2014, background): “…(Wilhelm et al., 1995) SOLIS Solar Optical Long-term Investigations of the Sun (Keller et al., 2003a) SOLIS/VSM SOLIS Vector SpectroMagnetograph (Keller et al., 2003b) Solar Orbiter (Müller et al., 2013) STEREO Solar-TErrestrial RElations Observatory (Kaiser et al., 2008) STEREO/SECCHI STEREO…”