A Possible Origin of Faint Fraunhofer Lines
β Scribed by KOTHARI, DAULAT SINGE
- Book ID
- 109491948
- Publisher
- Nature Publishing Group
- Year
- 1929
- Tongue
- English
- Weight
- 256 KB
- Volume
- 124
- Category
- Article
- ISSN
- 0028-0836
- DOI
- 10.1038/124090b0
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
From observations made at Kitt Peak the true central intensities of 40 Fraunhofer lines distributed between ,~2 3083-7699, for the center of the solar disk, are derived and given in tabular form. The paper includes a description of the optical system -telescope and spectrograph. The methods of obser
Solar differential rotation for 1982-83 obtained at the double pass spectrograph of the McMath telescope at Kitt Peak, are presented for lines of Fe, Mg, Na, K, Si, and O in the wavelength interval 223820-10827. The results are analyzed by representations in Legendre polynominals and a power series.