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Science Acrylic Print featuring the photograph Sun Emits M6.5 Class Solar Flare, 2013 by Science Source

The watermark in the lower right corner of the image will not appear on the final print.

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Sun Emits M6.5 Class Solar Flare, 2013 Acrylic Print

Science Source

by Science Source

$109.00

Product Details

Sun Emits M6.5 Class Solar Flare, 2013 acrylic print by Science Source.   Bring your artwork to life with the stylish lines and added depth of an acrylic print. Your image gets printed directly onto the back of a 1/4" thick sheet of clear acrylic. The high gloss of the acrylic sheet complements the rich colors of any image to produce stunning results. Two different mounting options are available, see below.

Design Details

NASA's Solar Dynamics Observatory captured this image of an M6.5 class flare at 316 EDT on April 11, 2013. This image shows a combination of light in... more

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3 - 4 business days

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Sun Emits M6.5 Class Solar Flare, 2013 Photograph by Science Source

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Acrylic Print Tags

acrylic prints science acrylic prints astronomy acrylic prints astronomical acrylic prints astrophysics acrylic prints astrophysical acrylic prints celestial body acrylic prints celestial object acrylic prints heavenly body acrylic prints deep space acrylic prints deep sky acrylic prints sun acrylic prints g-type main-sequence star acrylic prints g2v acrylic prints yellow dwarf acrylic prints star acrylic prints

Photograph Tags

photographs science photos astronomy photos astronomical photos astrophysics photos astrophysical photos celestial body photos celestial object photos heavenly body photos deep space photos deep sky photos sun photos g-type main-sequence star photos g2v photos yellow dwarf photos star photos

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Artist's Description

NASA's Solar Dynamics Observatory captured this image of an M6.5 class flare at 316 EDT on April 11, 2013. This image shows a combination of light in wavelengths of 131 and 171 Angstroms. The Sun is the star at the center of the Solar System. It is almost perfectly spherical and consists of hot plasma interwoven with magnetic fields. The Sun is classified as a G-type main-sequence star (G2V) based on spectral class and it is informally designated as a yellow dwarf because its visible radiation is most intense in the yellow-green portion of the spectrum, and although it is actually white in color, from the surface of the Earth it may appear yellow because of atmospheric scattering of blue light. A coronal mass ejection (CME) is a massive burst of solar wind and magnetic fields rising above the solar corona or being released into space. Coronal mass ejections are often associated with other forms of solar activity, most notably solar flares, but a causal relationship has not been establi...

 

$109.00

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