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Credit: SOHO LASCO,
EIT and MDI teams
EIT (Extreme ultraviolet
Imaging Telescope) images the solar atmosphere at several
wavelengths, and therefore, shows solar material at different
temperatures. In the images taken at 304 Angstroms the bright
material is at 60,000 to 80,000 degrees Kelvin. In those taken at
171, at 1 million degrees. 195 Angstrom images correspond to
about 1.5 million Kelvin. 284 Angstrom, to 2 million degrees. The
hotter the temperature, the higher you look in the solar
atmosphere.
Source:
NASA / ESA / SOHO / LASCO, EIT and MDI teams

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