λ 5303 Fe XIV density models of the inne
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R. R. Fisher
📂
Article
📅
1978
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Springer
🌐
English
⚖ 580 KB
The Sacramento Peak Observatory's 40 cm coronagraph was used with an emission line photometer to observe the distribution of A5303 Fe xIv brightness as a function of position angle, height above the limb, and time. These data were used to construct models of the Volume emissivity as a function of so