SOLAR IMAGES

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.


Active region 26-4-21

TS80mm f6 refractor
Daystar Quark Chromosphere H-alpha filter
ASI 174mm camera
TS UV/IR blocking filter
TS tilt adapter
Ioptron CEM25p mount

Firecapture – AS3! – ImPPG – Affinity



Large promenance 23-4-21

TS80mm f6 refractor
Daystar Quark Chromosphere H-alpha filter
ASI 174mm camera
TS UV/IR blocking filter
TS tilt adapter
Ioptron CEM25p mount

Firecapture – AS3! – ImPPG – Affinity



Solar activity 20-4-21

TS80mm f6 refractor
Daystar Quark Chromosphere H-alpha filter
ASI 174mm camera
TS UV/IR blocking filter
TS tilt adapter
Ioptron CEM25p mount

Firecapture – AS3! – ImPPG – Affinity



Three large promenances and activity on the chromosphere 29-3-21

TS80mm f6 refractor
Daystar Quark Chromosphere H-alpha filter
ASI 174mm camera
TS UV/IR blocking filter
TS tilt adapter
Ioptron CEM25p mount

Firecapture – AS3! – ImPPG – Affinity



Large promenance and activity on the chromosphere 30-3-21

TS80mm f6 refractor
Daystar Quark Chromosphere H-alpha filter
ASI 174mm camera
TS UV/IR blocking filter
TS tilt adapter
Ioptron CEM25p mount

Firecapture – AS3! – ImPPG – Affinity