Solar activity was at very low levels over the past 24 hours. AR2829 has recently decayed while approaching the SW limb, away from Earth-view. AR2832 (Bxo/beta) exhibited continuous gradual disintegration of its sunspot structure. Only a few B-class solar enhancements mainly from AR2832 was recorded by space weather agencies throughout the monitoring period. Meanwhile, AR2826 from the previous rotation is returning into Earth-view from the NE limb. The latest sunspot number (based on visual count and Wolf number calculation) is 23. 

Enhanced plages associated with the upper-mentioned sunspot groups, few short stable filaments across the Sun’s disk, and some 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 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.