observes the corona of the sun from 1.3 Ro (1.3 solar radii) out to 10.0 Ro.
Among the phenomenon observed by the instrument are
Coronal Mass Ejections (CMEs) and comet entering the corona.

To enter the comet image archive click on the comet below

To enter the CME image archive click the image below

The Latest Lyman-Alpha Synoptic Image

Click on Image for MPEG movie

The Latest O VI 1032 Angstrom Synoptic Image

Click on Image for MPEG movie

For more information about the SOHO spacecraft, the UVCS instrument, or solar physics, visit the web sites below.