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- UVCS
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- CME Ultraviolet Spectra vs. time and space
- ∑ UVCS has measured coronal plasma parameters (at large coronal radii) in several CMEs in 1996 and 1997.
- ∑ UVCS can isolate spectral lines from both hot (coronal) and cool (chromospheric) material, and measure intensities,
- Doppler shifts, and line shapes.
- ∑ Observed ``knots'' of emission are strongly Doppler shifted, exhibiting a complex 3D velocity structure.
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