k Sun observed at different wavelengths Sun observed at different wavelengths. Collage of solar images from NASAs Solar Dynamics Observatory SDO. Observing the Sun in different wavelengths helps highlight different aspects of the suns surface and atmosphere. The wavelengths in nanometres nm from the Atmospheric Imaging Assembly AIA are 450nm light green, 170nm pink, 160nm dark green, 33.5nm blue, 30.4nm orange, 21.1nm violet, 19.3nm bronze, 17.1nm gold, 13.1nm aqua and 9.4nm bright green. From the Helioseismic and Magnetic Imager HMI are visible light at 617.3nm orangeyellow, and dopplergram and magnetogram observations both grey. For a key for the colours, see C0223724. Stock Photo - Afloimages
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Sun observed at different wavelengths Sun observed at different wavelengths. Collage of solar images from NASA s Solar Dynamics Observatory  SDO . Observing the Sun in different wavelengths helps highlight different aspects of the sun s surface and atmosphere. The wavelengths in nanometres  nm  from the Atmospheric Imaging Assembly  AIA  are: 450nm  light green , 170nm  pink , 160nm  dark green , 33.5nm  blue , 30.4nm  orange , 21.1nm  violet , 19.3nm  bronze , 17.1nm  gold , 13.1nm  aqua  and 9.4nm  bright green . From the Helioseismic and Magnetic Imager  HMI  are visible light at 617.3nm  orange yellow , and dopplergram and magnetogram observations  both grey . For a key for the colours, see C022 3724.
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Sun observed at different wavelengths

Sun observed at different wavelengths. Collage of solar images from NASA's Solar Dynamics Observatory (SDO). Observing the Sun in different wavelengths helps highlight different aspects of the sun's surface and atmosphere. The wavelengths in nanometres (nm) from the Atmospheric Imaging Assembly (AIA) are: 450nm (light green), 170nm (pink), 160nm (dark green), 33.5nm (blue), 30.4nm (orange), 21.1nm (violet), 19.3nm (bronze), 17.1nm (gold), 13.1nm (aqua) and 9.4nm (bright green). From the Helioseismic and Magnetic Imager (HMI) are visible light at 617.3nm (orange/yellow), and dopplergram and magnetogram observations (both grey). For a key for the colours, see C022/3724.

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