The Coronal Helium Abundance Experiment on Spacelab 2

Details The Coronal Helium Abundance Experiment on Spacelab 2 The Coronal Helium Abundance Experiment on Spacelab 2

Dec 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ssrv...29..431p&link_type=abstract

(Schweizerische Naturforschende Gesellschaft and Eidgenoesische Technische Hochschule Zuerich, Conference on Solar Physics from

Physics

17

Abundance, Helium, Solar Corona, Solar Instruments, Spacelab Payloads, Grazing Incidence Telescopes, Solar Activity, Solar Spectrometers, Space Missions, Spaceborne Experiments, Stellar Evolution

Scientific paper

The Coronal Helium Abundance Spacelab Experiment basically consists of a grazing incidence telescope and spectrometer sensitive over the range 150-1335 A. While 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.

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