UVCS Team Science Working Groups
(*Note: With UVCS past its End of Mission, many of these groups are no longer active.)
UVCS Science Working Groups
(*Note: With UVCS past its End of Mission, many of these groups are no longer active.)
S3. Theoretical models of CME's
S4. Determination of coronal elemental abundances and minor ion densities
S5. Unassigned
S6. Studies of stars, comets, planets, and the F corona
S7. Determination of electron coronal density irregularities from K Corona
H I Lyman lines