Sun prominence
Taken by Valerio on June 3, 2025 @ Londa Tuscany Italy
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  Camera Used: ZWO ASI224MC
Exposure Time: Unavailable
Aperture: Unavailable
ISO: Unavailable
Date Taken: 2025:06:17 18:22:48
 
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Subject Line: "Dynamic Solar Prominence with Fine Filamentary Structures – H-alpha Observation" Body: Title: "Solar Prominence Ballet: A Magnetic Spectacle in H-alpha" Date: June 3, 2025 Location: Londa, Florence, Italy (43°51'31"N 11°34'18"E, 347m a.s.l.) Equipment & Acquisition: Telescope: Lunt LS60T H-alpha B600 Camera: ASI 224 MC + 2x Barlow Mount: Avalon Linear Fast Reverse Acquisition: 120-second capture (5.0 ms shutter, 58 fps, gain 246, gamma 49) Conditions: Sensor temperature 34°C, stable seeing Software: FireCapture, AutoStakkert, AstroSurface (wavelet sharpening), Photoshop Description: "This high-resolution H-alpha image captures a striking solar prominence extending ~92,000 km (∼7 Earth diameters) from the limb. The structure exhibits well-defined filamentary details and potential Kelvin-Helmholtz instabilities along its edges (visible at <1,000 km resolution). The plasma’s dynamic density stratification suggests active magnetic restructuring—possibly precursor to a CME or gradual dissipation. Notable Features: Distinct alternating high/low-density plasma layers Fibril structures tracing magnetic field lines (enhanced via wavelet processing) Optimal contrast between 10,000°C plasma and dark background Processing Approach: Science-optimized: Preserved intensity gradients for density analysis Selective enhancement: AstroSurface wavelet sharpening for clarity Credit: Valerio Fontani Affiliation: Società Astronomica Galileo Galilei, Londa (FI), Italy
Photographer's website:
https://http://www.elcrab.altervista.org/
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