PPT Slide
- Perform:
- EUV Spectroscopy with High Spectral and Spatial Resolution
- Monochromatic EUV Imaging
- Imaging and Spectroscopy with High Temporal Resolution
- Obtain:
- Imaging and Spectral Measurements from Lines in Transition Region, Coronal and Solar Flare Plasma
- Accurate Coronal Density Measurements
- Respond to Highly Dynamic Phenomena
- Locate and Change the Observing Mode to a Region of Brighter Intensity
- Observe a Range of Sizes of Solar Phenomena
Summary of Science Requirements