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The excitation mechanism of [Fe XIV] 5303 å line in the inner regions of solar corona

✍ Scribed by K. P .Raju; J. N. Desai; T. Chandrasekhar; N. M. Ashok

Book ID
112828615
Publisher
Springer-Verlag
Year
1991
Tongue
English
Weight
228 KB
Volume
12
Category
Article
ISSN
0250-6335

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✍ R. R. Fisher 📂 Article 📅 1978 🏛 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