SOLAR IMAGES 2021
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