| Autor: |
Byard, Paul L., Kissell, Kenneth E. |
| Zdroj: |
Solar Physics; December 1971, Vol. 21 Issue: 2 p351-359, 9p |
| Abstrakt: |
The purpose of this paper is to report on some intensity measurements of the Fe xiii lines at 10 747 Å and 10 798 Å made during the total eclipse of 12 November, 1966. Infrared spectra were taken of the solar corona at a dispersion of 90 Å per mm, using an RCA image converter and spectrograph aboard the NASA CV 990 aircraft off the coast of southern Brazil. The spectra have been reduced to equivalent width in terms of the coronal continuum and values derived for different points in the corona. |
| Databáze: |
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