Conveners
Day 1: Session 1
- Ivan Milic (KIS)
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Hardi Peter (MPS), Sami Solanki (MPS)02/06/2026, 09:00Science Meeting
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02/06/2026, 09:05Science Meeting
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02/06/2026, 09:20Science Meeting
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02/06/2026, 09:35Science Meeting
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Johannes Hoelken (MPS)02/06/2026, 09:50Science Meeting
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Jose Carlos del Toro Iniesta (Instituto de Astrofísica de Andalucía (IAA-CSIC))02/06/2026, 10:05Science MeetingContributed
Studies of image formation in astronomical instruments are often conducted under the assumption that light polarization has no significant influence. When diffraction effects are considered, they are typically treated using scalar point spread functions. This contribution aims to address the general problem by highlighting the potential impact of polarization and assessing it for a specific...
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Francisco Javier Bailen (IAA-CSIC)02/06/2026, 10:20Science Meeting
Solar magnetographs are often equipped with Fabry–Pérot etalons to sample spectral lines that are sensitive to the magnetic field. Typically, two etalons with different optical thicknesses and reflectivities are used to reduce unwanted light from secondary orders while improving the spectral resolution. However, using two etalons in spaceborne or balloon-borne applications is usually...
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