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Introduction
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ULTRAVIOLET CORONAGRAPH SPECTROMETER
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Flight Software
Intensities and Count Rates
Introduction
Estimates of Line Intensities in Coronal Holes
Spectral line intensities
Assumed Solar Wind Plasma Parameters
Calculated Line Intensities
Measured HI Ly-a Intensities in Coronal Holes
Measured HI Ly- intensities and estimated OVI intensities in coronal streamers
Relationships between ultraviolet intensity and count rate
Peter Smith
Fri Jan 17 12:11:15 EST 1997
