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.

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 AR2835



28-06-2021 Active region and filament



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



10-06-2021 Large quiescent prominences

 



07-06-2021 Large active region and sunspots

 



02-06-2021 Active region and large prominences

 



12-05-2021 Sunspot and plage

 



26-04-2021 – active region (inverse)

 



23-04-2021

 



22-04-2021 – active region & prominences

 



20-04-2021 Active region and prominences

 



18-04-2021
active region, filaments and prominences

 


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30-03-2021 – Large flame prominence