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 – Lightroom – Affinity photo