The Coronal Helium Abundance Spacelab Experiment, (CHASE), basically consists of a grazing incidence telescope and spectrometer sensitive over the range 150–1335 Å. Whilst aimed primarily at deriving the solar helium abundance from measurements of coronal resonance scattering, its specification has been extended in order to provide a more general purpose solar XUV facility. The instrument will be flown on the Spacelab 2 Mission, currently scheduled for launch in November 1984.
Spacelab-2
The Coronal Helium Abundance Spacelab Experiment, (CHASE) aimed primarily at deriving the solar helium abundance from measurements of coronal resonance scattering - 1984
