The Fine Scale Structure of the Solar Limb in a Coronal Hole

Physics

Scientific paper

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Scientific paper

Using simultaneous multiwavelength observations made with the Extreme
Ultraviolet Spectrometer of the Harvard experiment on Skylab, and an
image enhancement algorithm we explore the fine scale structure of the
solar limb in a coronal hole at temperatures ranging from 10^3 to 10^6
K.

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