Abstract. — Using a newly proposed method of analysis of the solar photometric spectrum in the range λ 6105 - λ 6150, with the spectral data published by Delbouille, Neven and Roland, all lines mentioned in the S.R.R.T. are confirmed with the exception of the eight weak lines mentioned in table I. Eleven weak lines quoted in the R.R.T. but rejected in the S.R.R.T., reappear in our analysis (column λ0 of Table II). Tentative identifications are proposed for five new lines while two identifications given in the R.R.T. are confirmed.Baeck Nicole. Remarks on the presence of some weak lines in the solar photometric spectral range λ 6105 - λ 6150. In: Bulletin de la Classe des sciences, tome 61, 1975. pp. 706-710
Context. Present knowledge of the solar spectrum is limited because it is very difficult to observe ...
We present here the solar LOG GF values obtained using the Liege solar at las and the standard solar...
Individual spectral line parameters including line positions, strengths, and intensities were genera...
Abstract. — Using a newly proposed method of analysis of the solar photometric spectrum in the range...
Abstract. — A new very general (computer) method is proposed for decomposing the solar photometric s...
Abstract. — The results obtained with our newly proposed method for analyzing the solar photospheric...
Abstract. — Applying a newly proposed method for decomposing the solar spectrum into Gaussian compon...
Kramida and Buchet-Poulizac [Eur. Phys. J. D 39, 173 (2006)] provide a comprehensive compilation of ...
Context. Both the quality and amount of astrophysical data are steadily increasing over time owing t...
SUMMARY: Taking into account effects of hyperfine structure, we calculated the synthetic solar spect...
At head of title: Solar physics committee.I. The spectra of the sun (Fraunhoferic) chromosphere, and...
We present an analysis of the second solar spectrum, as plotted in graphical form in the three volu...
SUMER – Solar Ultraviolet Measurements of Emitted Radiation – onboard of SOHO – Solar and Heliospher...
L. Becker — The solar spectrum at medium and low altitudes (Transactions of the Royal Society of Edi...
Synthetic stellar spectra are extensively used for many different applications in astronomy, from st...
Context. Present knowledge of the solar spectrum is limited because it is very difficult to observe ...
We present here the solar LOG GF values obtained using the Liege solar at las and the standard solar...
Individual spectral line parameters including line positions, strengths, and intensities were genera...
Abstract. — Using a newly proposed method of analysis of the solar photometric spectrum in the range...
Abstract. — A new very general (computer) method is proposed for decomposing the solar photometric s...
Abstract. — The results obtained with our newly proposed method for analyzing the solar photospheric...
Abstract. — Applying a newly proposed method for decomposing the solar spectrum into Gaussian compon...
Kramida and Buchet-Poulizac [Eur. Phys. J. D 39, 173 (2006)] provide a comprehensive compilation of ...
Context. Both the quality and amount of astrophysical data are steadily increasing over time owing t...
SUMMARY: Taking into account effects of hyperfine structure, we calculated the synthetic solar spect...
At head of title: Solar physics committee.I. The spectra of the sun (Fraunhoferic) chromosphere, and...
We present an analysis of the second solar spectrum, as plotted in graphical form in the three volu...
SUMER – Solar Ultraviolet Measurements of Emitted Radiation – onboard of SOHO – Solar and Heliospher...
L. Becker — The solar spectrum at medium and low altitudes (Transactions of the Royal Society of Edi...
Synthetic stellar spectra are extensively used for many different applications in astronomy, from st...
Context. Present knowledge of the solar spectrum is limited because it is very difficult to observe ...
We present here the solar LOG GF values obtained using the Liege solar at las and the standard solar...
Individual spectral line parameters including line positions, strengths, and intensities were genera...