Interpretation of Ti I lines of excitation energy 0.0-0.05 eV in the solar spectrum; use of new oscillator strengths of accuracy 0.5 per cent

Autor:	M. J. Shallis, D. E. Blackwell, G. J. Simmons
Rok vydání:	1982
Předmět:	Physics Space and Planetary Science Solar spectra Astronomy and Astrophysics Atomic physics Solar atmosphere Solar physics Spectral line Excitation Energy (signal processing) Interpretation (model theory)
Zdroj:	Monthly Notices of the Royal Astronomical Society. 199:37-42
ISSN:	1365-2966 0035-8711
DOI:	10.1093/mnras/199.1.37
Databáze:	OpenAIRE
Externí odkaz:	https://explore.openaire.eu/search/publication?articleId=doi_________::114d8f46a887c6a3f5f67964c4a5e787 https://doi.org/10.1093/mnras/199.1.37 Zobrazit plný text záznamu