𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Structure of the inner corona derived from observations of the eclipse of 16 February 1980

✍ Scribed by O. G. Badalyan; M. A. Livshits; J. Sýkora

Publisher
Springer
Year
1984
Tongue
English
Weight
949 KB
Volume
93
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

The spectrum of the inner corona observe
The spectrum of the inner corona observed during the total solar eclipse of 30 May 1965
✍ John T. Jefferies; Frank Q. Orrall; J. B. Zirker 📂 Article 📅 1971 🏛 Springer 🌐 English ⚖ 444 KB

A series of spectrograms of the inner solar corona were obtained at the total solar eclipse of 30 May 1965 using a fast spectrograph with a circular slit that recorded the spectrum from 23000 to 29000 at all position angles around the limb simultaneously. In this paper absolute intensity is given as

The physical conditions in inner corona
The physical conditions in inner corona derived from spectral data of the solar eclipse on 7 March, 1970
✍ E. A. Gurtovenko; K. V. Alikayeva 📂 Article 📅 1971 🏛 Springer 🌐 English ⚖ 442 KB

The spectrum of the solar corona obtained during the eclipse of 7 March, 1970 has been studied. From the analysis of the line halfwidths it is concluded that the emission of coronal lines of various groups arises in different volumes of the corona. The lines 15303 and 14231 are analyzed in detail an

Clues to the mode of excitation of Fe x
Clues to the mode of excitation of Fe x ions in the solar corona from the 1980 eclipse observations
✍ Jagdev Singh 📂 Article 📅 1985 🏛 Springer 🌐 English ⚖ 353 KB

The line and continuum intensities deduced from the multislit spectra of the (Fex) coronal emission line taken at the 1980 eclipse are used to discuss the relative roles of radiative and collisional excitation mechanisms. It is shown that for R/R o < 1.2, collisional excitation is the predominant mo