NASA SDO - Transit of Venus, Egress, 1700 Angstrom @LittleSDOHMI
NASA SDO - Transit of Venus, Egress, 1700 Angstrom  @LittleSDOHMI
Uploaded June 2012 | Updated September 2026, 2 weeks ago
AIA 1700: This channel (as well as AIA 1600) often shows a web-like pattern of bright areas that highlight places where bundles of magnetic fields lines are concentrated. However, small areas with a lot of field lines will appear black, usually near sunspots and active regions.

Where: Temperature minimum and photosphere
Wavelength: 1700 angstroms (0.00000017 m) = Far Ultraviolet
Primary ions seen: Continuum
Characteristic temperature: 6,000 K (11,000 ˚F)
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NASA SDO - Transit of Venus, Egress, 1700 Angstrom

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