SUNSPOT MONITORING – OCTOBER 16, 2018

SUNSPOT MONITORING – OCTOBER 16, 2018

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Here are today’s solar images taken from Al Sadeem Observatory, October 16, 2018.

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

AR2724 has recently decayed completely into plage. The other visible sunspot group AR2725 was also in dissipating stage, barely seen in visible imagery. Both mentioned active regions were inactie; did not produce any significant flaring activity. The latest sunspot number (based on visual count and Wolf number calculation) is 10.  Some huge eruptive prominences at the opposite sides (southeast and northwestern limb) and associated remnant plages and filaments associated with former AR2724 and the decaying AR2725 were distinctively captured in H-alpha imagery.

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. The extent of the frequency and intensity of the Sun’s activity will highly depend on the magnetic flux fluctuations happening in the visible ARs in the coming days. Close monitoring is being conducted by numerous space weather agencies for any significant development.

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 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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