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
The population of excited levels of the ground terms of ions Fe X, XI and XIV in the solar corona
β Scribed by C. Jordan
- Publisher
- Elsevier Science
- Year
- 1965
- Weight
- 156 KB
- Volume
- 18
- Category
- Article
- ISSN
- 0031-9163
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
A theoretical analysis is given for the excitation transfer of Xe('P,) +N, (X IX ,') + Xe ( 'SO) + N, (B 'Qy). The analysis is based on (i} pure Coulomb interaction coupled with electron exchange and (ii) spin-dependent interaction between the collision partners. Both mechanisms can account for the
Experimental data on ground-and excited-state properties for all nuclei with mass number A=144 have been compiled and evaluated. States populated in radioactive decay as well as in nuclear reactions have been considered. For these nuclei, level and decay schemes have been built, as well as tables of