AR2832  has completely decayed into plage as it approaches the NW limb. The lone visible sunspot group, AR2833 (Hsx/alpha) exhibited very little to no noticeable change in its large unipolar sunspot structure. Both sunspot regions are currently quiet with no significant flaring activity recorded over the past 24 hours. The latest sunspot number (based on visual count and Wolf number calculation) is 11. 

Enhanced plages associated with the upper-mentioned sunspot groups, few short stable filaments across the Sun’s disk, and some huge eruptive prominences at the opposite (SW and NE) limbs, were the other noteworthy solar features distinctively captured in H-alpha imagery.

Space weather agencies* forecast solar activity to remain at very low levels with chances of solar flares of mostly B-class to possibly isolated C-class intensity, mainly from AR2833 in the next few 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. For H-alpha imagery, the equipment used are Lunt 60mm H-alpha solar telescope, and QHYCCD 290III mono camera; all mounted on Skywatcher EQ6 pro mount 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.