The Sun is the star at the center of the Solar System. It is a nearly perfect sphere of hot plasma, heated to incandescence by nuclear fusion reactions in its core, radiating the energy mainly as visible light and infrared radiation.
The Sun’s core fuses about 600 million tons of hydrogen into helium every second, converting 4 million tons of matter into energy every second as a result. This energy, which can take between 10,000 and 170,000 years to escape the core, is the source of the Sun’s light and heat.

Equipment for capture:

102mm f11 Fraunhofer achromat refractor,  80mm f6 refractor – Daystar Quark Chromosphere – ZWO tilt adapter – ASI 174mm – Baader 2″ ERF Filter – ZWO EAF focuser – Ioptron CEM25p mount

Capture software: Sharpcap & Firecapture

Post-processing software:  AS3! – ImPPG – PS CS5 

29-10-2021 Sunspots and filaments

28-10-2021 AR2891 Large sunspot and CME

07-09-2021 Very large prominence

22-07-2021 Sunspot and filaments

10-06-2021 Large quiescent promenences

07-07-2021 Large prominence

03-07-2021 Sunspot AR2835

28-06-2021 Active region and filament

28-06-2021  Active region and prominences

28-06-2021 Prominences

17-06-2021 Surface filaments

17-06-2021 Surface and prominences

13-06-2021 Large active region and prominences

07-06-2021 Active region

01-06-2021 Large prominences

01-06-2021 AR2827