Atomic data and spectral line intensities for O VIII and Fe XVII resonance lines as well as their O VII and Fe XVI satellite lines
- Author
- CORNILLE, M1 ; DUBAU, J1 ; FAUCHER, P2 ; BELY-DUBAU, F2 ; BLANCARD, C3
[1] CNRS, obs. Paris, 92195 Meudon, France
[2] CNRS, obs. Côte Azur, 06304 Nice, France
[3] Cent. études Limeil-Valenton, 94195 Villeneuve Saint-Georges, France - Source
Astronomy & astrophysics. Supplement Series (Print). 1994, Vol 105, Num 1, pp 77-90 ; ref : 1/2 p
- CODEN
- AAESB9
- ISSN
- 0365-0138
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- EDP Sciences, Les Ulis
- Publication country
- France
- Document type
- Article
- Language
- English
- Keyword (fr)
- Couronne solaire Donnée Fer ion Intensité raie Oxygène ion Plasma Raie satellite Soleil Spectre RX Spectre émission
- Keyword (en)
- Solar corona Data Iron ions Line intensity Oxygen ions Plasma Satellite lines Sun X-ray spectra Emission spectra
- Classification
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03A Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations / 001E03A30 Fundamental aspects of astrophysics / 001E03A30K Atomic and molecular data, spectra, and spectral parameters (opacities, rotation constants, line identification, oscillator strengths, gf values, transition probabilities, etc.)
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03B Solar system / 001E03B60 Solar physics / 001E03B60T Solar electromagnetic radiation
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 3462483
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
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