k Solar activity, SDO ultraviolet image Solar activity, Solar Dynamics Observatory SDO combined ultraviolet image. The SDO is an Earthorbiting spacecraft launched in 2010 by NASA and used to observe the Sun. Here, the Sun is seen at three wavelengths 304 orange, 211 pink, and 171 yellow angstroms all extreme ultraviolet. Channel 304 shows filaments and prominences in the upper chromosphere and lower transition region. Channel 211 shows the Suns corona outer atmosphere. Channel 171 shows coronal loops and the upper transition region. Image obtained on 23 January 2012, during a period of solar activity. Stock Photo - Afloimages
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Solar activity, SDO ultraviolet image Solar activity, Solar Dynamics Observatory  SDO  combined ultraviolet image. The SDO is an Earth orbiting spacecraft launched in 2010 by NASA and used to observe the Sun. Here, the Sun is seen at three wavelengths: 304  orange , 211  pink , and 171  yellow  angstroms  all extreme ultraviolet . Channel 304 shows filaments and prominences in the upper chromosphere and lower transition region. Channel 211 shows the Sun s corona  outer atmosphere . Channel 171 shows coronal loops and the upper transition region. Image obtained on 23 January 2012, during a period of solar activity.
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Solar activity, SDO ultraviolet image

Solar activity, Solar Dynamics Observatory (SDO) combined ultraviolet image. The SDO is an Earth-orbiting spacecraft launched in 2010 by NASA and used to observe the Sun. Here, the Sun is seen at three wavelengths: 304 (orange), 211 (pink), and 171 (yellow) angstroms (all extreme ultraviolet). Channel 304 shows filaments and prominences in the upper chromosphere and lower transition region. Channel 211 shows the Sun's corona (outer atmosphere). Channel 171 shows coronal loops and the upper transition region. Image obtained on 23 January 2012, during a period of solar activity.

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