Imagery of the Sun in both White Light and Hydrogen-Alpha. Do not point your telescope at the sun without proper filtering!

White Light: the full visible light spectrum reduced to safe levels. This shows the Sun’s Photosphere, or the lowest visible altitude of the star

Hydrogen-Alpha: a deep red 656.28nm wavelength which is emitted by energized Hydrogen atoms. On the Sun this reveals the Chromosphere, or the Sun’s lower atmosphere

 

AR3576 captured in White Light on February 9, 2024

 

Solar ISS Transit from the morning of October 31st, 2023 in 0.7A

Capture of AA2593 transiting the Sun (0.7A) on the morning of October 17th

Full Disk capture of AR 3448-3459 in 0.7Å from October 7, 2023

Full Disk capture of AR 3440-3451 in 0.7Å from October 1, 2023

AR3571-3584 in in 0.7A Hα captured on February 12, 2024

AR3256, 3257 in Hydrogen Light from March 19, 2023

AR3256, 3257 in White Light from March 19, 2023

AR3190-3192 in 0.5Å Hα from January 16, 2023

Active Regions 3182, 3184, 3193 in 0.5Å Hα from January 16, 2023

Solar Disc and several Active Regions (3181 through 3192) captured January 13, 2023 in White Light using a Canon RP and 8” SCT

Solar activity in Hydrogen-Alpha, captured July 24, 2021 using a Coronado 60mm and an ASI178MM camera

Solar activity in Hydrogen-Alpha, captured July 24, 2021 using a Coronado 60mm and an ASI178MM camera

A transit of the ISS across the Sun from February 2, 2020 in Hα

A transit of the ISS across the Sun from February 2, 2020 in Hα

A transit of the ISS across the Sun from February 2, 2020 in White Light

A transit of the ISS across the Sun from February 2, 2020 in White Light

Sunspot Group AR2765 from June 2020 in White Light, 2000mm Focal Length

Sunspot Group AR2765 from June 2020 in White Light, 2000mm Focal Length

Sunspot Group AR2765 from June 2020 in White Light, 4000mm Focal Length

Sunspot Group AR2765 from June 2020 in White Light, 4000mm Focal Length

The Full Disk of the Sun in 0.5Å Hα taken on 26 January, 2020, shown in double exposure / false color. AR 2757 can be seen near the meridian with the Sun’s North Pole oriented upCoronado SolarMax III 70 Double Stack, ZWO ASI1600MM-P

The Full Disk of the Sun in 0.5Å Hα taken on 26 January, 2020, shown in double exposure / false color. AR 2757 can be seen near the meridian with the Sun’s North Pole oriented up

Coronado SolarMax III 70 Double Stack, ZWO ASI1600MM-P

Sunspot / AR 2738 taken in false color White Light from April 2019 at 2000mm. ZWO ASI290MC, Celestron C8, AstroZap Mylar filter

Sunspot / AR 2738 taken in false color White Light from April 2019 at 2000mm. ZWO ASI290MC, Celestron C8, AstroZap Mylar filter

Sunspot / AR 2738 taken in false color White Light from April 2019 at 6000mm. ZWO ASI290MC, Celestron C8, AstroZap Mylar filter

Sunspot / AR 2738 taken in false color White Light from April 2019 at 6000mm. ZWO ASI290MC, Celestron C8, AstroZap Mylar filter

A Solar ISS Transit captured on 11 October 2020 in White Light. Sunspot group AR2775 can be seen near one of the transit captures

A Solar ISS Transit captured on 11 October 2020 in White Light. Sunspot group AR2775 can be seen near one of the transit captures

Sunspots AR2673 & AR2674 from September 2017, taken with a Canon T3i and a C8 with a White Light solar filter

A pair of Prominences on the edge of the Sun from May 2019, shown in false color with double exposure. AR2714 is the cause of the Prominence seen in the upper-left as it nears the edge of the Sun. North is to the leftCoronado SolarMax II 90 Double S…

A pair of Prominences on the edge of the Sun from May 2019, shown in false color with double exposure. AR2714 is the cause of the Prominence seen in the upper-left as it nears the edge of the Sun. North is to the left

Coronado SolarMax II 90 Double Stack, ZWO ASI290MC