SUNSPOT MONITORING – NOVEMBER 29, 2018

SUNSPOT MONITORING – NOVEMBER 29, 2018

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Here are today’s solar images taken from Al Sadeem Observatory, November 29, 2018.

The sky was clear with light air turbulence making the seeing and transparency good at the time these images were taken.

Generally very low solar activity has persisted over the past 24 hours.  The Sun remains spotless and relatively inactive, without any significant flaring activity recorded. The latest sunspot number (based on visual count and Wolf number calculation) is 0.

Space weather agencies* forecast solar activity to remain at very low levels with chances of weak X-ray fluxes or flares ranging up to B-class intensity. Close monitoring is being conducted by numerous space weather agencies for any significant development. Some huge eruptive prominences at the limbs, and tiny filaments across the disk were distinctively captured in H-alpha imagery.

Equipment used are Skywatcher 120mm refractor telescope with Baader filter and unmodified Canon EOS 1D Mark IV DSLR camera for visible imagery and Lunt H-alpha solar telescope and ZWO120MM CMOS camera for H-alpha imagery, mounted on Skywatcher EQ6 Pro. Pre-processing of visible solar images was performed in PIPP, stacking in Autostakkert, slight wavelet adjustments in Registax 6 and post-processing in Adobe Photoshop CC.

*Technical reports courtesy of Solar Influence Data Center (SIDC), NOAA-Space Weather Prediction Center (NOAA-SWPC)

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