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Photographer:

a.carrozzi

Location of Photo:

Casalgrande, Italy

Date/Time of photo:

March 8th, 2025. 11:00 UTC

Equipment:

H-Alpha Tecnosky Acro 152/900 mm Daystar Quark Chromosphere ZWO ASI 174MM CaK Coronado PST (40/400 mm) Basler ace 1300

Description:

Multiwavelength Sun The solar chromosphere is a dynamic layer of the Sun’s atmosphere, and its appearance changes depending on the observed wavelength—meaning the element being visualized in that layer. H-Alpha (656.3 nm - red): Highlights active regions and plasma dynamics. Best reveals filaments and prominences. CaK (393.4 nm - near-ultraviolet): Better shows the interaction between the magnetic field and the chromosphere. Displays a more granular structure compared to H-Alpha. In this panel, from the top left: prominences in H-Alpha, full disk in CaK, active region AR4012 in CaK and H-Alpha.

Website:

https://www.instagram.com/alessandro.carrozzi/