Sunspots and a detached prominence photographed on July 11, 2014. (© Alan Friedman, All Rights Reserved.)
Captured in hydrogen-alpha wavelengths, the image above has been colored by Alan, rotated 90 degrees counterclockwise, and inverted from the original. The sunspots and standing prominence are cooler in Ha than the surrounding chromosphere and corona, and so actually photograph darker.
A view of sunspot 2109 in visible light can be seen below:
Sunspots are the result of magnetic fields rising up from deep within the Sun, preventing convection from occurring in large areas on the Sun’s surface and thereby creating relatively cooler regions we see as dark spots. They can often be many times the size of Earth and can be sources of powerful solar flares.
See these and more images by Alan on his blog here.
Images © Alan Friedman. All rights reserved.
Tagged as:
Alan Friedman,
astrophotography,
hydrogen alpha,
prominence,
Star,
sun,
sunspot
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