UVCS Team Science Working Groups

(*Note: With UVCS past its End of Mission, many of these groups are no longer active.)

1. Calibration and co-registration

2. Measurement and spectroscopic diagnostics

3. Empirical models of coronal holes, plumes, and plasmoids

4. Empirical models of helmet streamers

5. Empirical models of CME's, transients, active regions, flares, quiet corona

6. Synoptic models, tomography, morphology, long term variations

UVCS Science Working Groups

(*Note: With UVCS past its End of Mission, many of these groups are no longer active.)

S1. Theoretical models of helmet streamers

S2. Theoretical models of coronal holes, identification of heating and acceleration processes

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

S8. Coordination of white light data