Abstract
The limb event of 13 August 1973, observed by Skylab in soft X-rays, exhibited typical characteristics of the giant post-flare arches observed by HXIS and FCS on board SMM in the 1980s. We present here examples of the processed Skylab images which yield 4 times better angular resolution than the SMM experiments and thus, for the first time, make it possible to distinguish the real fine structure of a giant post-flare arch.
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