
Check here for the description of the current synoptic sequences.
For detailed time/date for past synoptic observations, check the UVCS mission logs.
The current UVCS OVI synoptic program is a 14-hour observation at 1.6, 1.75, 1.9 Ro (coronal hole, mostly for N and S), and at 1.6, 1.75, 1.9, 2.1, 3.0 Ro (streamer, mostly for W, NW, NE, E, SE, SW).

The current UVCS LyA synoptic program is a 7-hour observation at 1.6, 1.75, 1.9, 2.1 Ro (coronal hole, mostly for N and S), and at 1.6, 1.75, 1.9, 2.1 , 2.5, 3.0 Ro (streamer, mostly for W, NW, NE, E, SE, SW).

The current UVCS mini-synoptic program is a 5-hour observation at 1.6, 1.75, 1.9 Ro (coronal hole, mostly for N and S), and at 1.6, 1.75, 2.1 Ro (streamer, mostly for W, NW, NE, E, SE, SW).

These directories contain the complete pointing information for the SOHO/UVCS synoptic observations
since April 11, 2000 (View the synoptic program sequences).
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This page is created by Yuan-Kuen Ko, Silvio Giordano, and Rai Wu, and is maintained by Yuan-Kuen Ko at SOHO EOF.
Last updated: Feb.27, 2006