On the identification of Ar x and Ar xiv in the solar corona and the origin of the unidentified coronal lines
Abstract A study of theZ-dependence of $ the^{2} $P intervals of 2s22p and 2s22p5, aided by recent observational results, confirms the identification in the coronal spectrum of λ 4412 with Arxiv, and of λ 5533.4 with Arx. It is further shown that transitions from metastable levels in the configurati...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Edlén, Bengt [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
1969 |
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| Schlagwörter: |
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| Anmerkung: |
© D. Reidel Publishing Company 1969 |
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| Übergeordnetes Werk: |
Enthalten in: Solar physics - Kluwer Academic Publishers, 1967, 9(1969), 2 vom: Okt., Seite 439-445 |
|---|---|
| Übergeordnetes Werk: |
volume:9 ; year:1969 ; number:2 ; month:10 ; pages:439-445 |
| Links: |
|---|
| DOI / URN: |
10.1007/BF02391668 |
|---|
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OLC2033520307 |
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| 520 | |a Abstract A study of theZ-dependence of $ the^{2} $P intervals of 2s22p and 2s22p5, aided by recent observational results, confirms the identification in the coronal spectrum of λ 4412 with Arxiv, and of λ 5533.4 with Arx. It is further shown that transitions from metastable levels in the configurations 3s23pk 3d, withk=3, 4 and 5, of Fexi,x, ix, and Nixiii, xiii, xi can well account for the remaining unidentified coronal lines. | ||
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10.1007/BF02391668 doi (DE-627)OLC2033520307 (DE-He213)BF02391668-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Edlén, Bengt verfasserin aut On the identification of Ar x and Ar xiv in the solar corona and the origin of the unidentified coronal lines 1969 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1969 Abstract A study of theZ-dependence of $ the^{2} $P intervals of 2s22p and 2s22p5, aided by recent observational results, confirms the identification in the coronal spectrum of λ 4412 with Arxiv, and of λ 5533.4 with Arx. It is further shown that transitions from metastable levels in the configurations 3s23pk 3d, withk=3, 4 and 5, of Fexi,x, ix, and Nixiii, xiii, xi can well account for the remaining unidentified coronal lines. Solar Corona Observational Result Metastable Level Coronal Line Recent Observational Result Enthalten in Solar physics Kluwer Academic Publishers, 1967 9(1969), 2 vom: Okt., Seite 439-445 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:9 year:1969 number:2 month:10 pages:439-445 https://doi.org/10.1007/BF02391668 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2002 GBV_ILN_2006 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4306 AR 9 1969 2 10 439-445 |
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10.1007/BF02391668 doi (DE-627)OLC2033520307 (DE-He213)BF02391668-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Edlén, Bengt verfasserin aut On the identification of Ar x and Ar xiv in the solar corona and the origin of the unidentified coronal lines 1969 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1969 Abstract A study of theZ-dependence of $ the^{2} $P intervals of 2s22p and 2s22p5, aided by recent observational results, confirms the identification in the coronal spectrum of λ 4412 with Arxiv, and of λ 5533.4 with Arx. It is further shown that transitions from metastable levels in the configurations 3s23pk 3d, withk=3, 4 and 5, of Fexi,x, ix, and Nixiii, xiii, xi can well account for the remaining unidentified coronal lines. Solar Corona Observational Result Metastable Level Coronal Line Recent Observational Result Enthalten in Solar physics Kluwer Academic Publishers, 1967 9(1969), 2 vom: Okt., Seite 439-445 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:9 year:1969 number:2 month:10 pages:439-445 https://doi.org/10.1007/BF02391668 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2002 GBV_ILN_2006 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4306 AR 9 1969 2 10 439-445 |
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10.1007/BF02391668 doi (DE-627)OLC2033520307 (DE-He213)BF02391668-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Edlén, Bengt verfasserin aut On the identification of Ar x and Ar xiv in the solar corona and the origin of the unidentified coronal lines 1969 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1969 Abstract A study of theZ-dependence of $ the^{2} $P intervals of 2s22p and 2s22p5, aided by recent observational results, confirms the identification in the coronal spectrum of λ 4412 with Arxiv, and of λ 5533.4 with Arx. It is further shown that transitions from metastable levels in the configurations 3s23pk 3d, withk=3, 4 and 5, of Fexi,x, ix, and Nixiii, xiii, xi can well account for the remaining unidentified coronal lines. Solar Corona Observational Result Metastable Level Coronal Line Recent Observational Result Enthalten in Solar physics Kluwer Academic Publishers, 1967 9(1969), 2 vom: Okt., Seite 439-445 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:9 year:1969 number:2 month:10 pages:439-445 https://doi.org/10.1007/BF02391668 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2002 GBV_ILN_2006 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4306 AR 9 1969 2 10 439-445 |
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10.1007/BF02391668 doi (DE-627)OLC2033520307 (DE-He213)BF02391668-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Edlén, Bengt verfasserin aut On the identification of Ar x and Ar xiv in the solar corona and the origin of the unidentified coronal lines 1969 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1969 Abstract A study of theZ-dependence of $ the^{2} $P intervals of 2s22p and 2s22p5, aided by recent observational results, confirms the identification in the coronal spectrum of λ 4412 with Arxiv, and of λ 5533.4 with Arx. It is further shown that transitions from metastable levels in the configurations 3s23pk 3d, withk=3, 4 and 5, of Fexi,x, ix, and Nixiii, xiii, xi can well account for the remaining unidentified coronal lines. Solar Corona Observational Result Metastable Level Coronal Line Recent Observational Result Enthalten in Solar physics Kluwer Academic Publishers, 1967 9(1969), 2 vom: Okt., Seite 439-445 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:9 year:1969 number:2 month:10 pages:439-445 https://doi.org/10.1007/BF02391668 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2002 GBV_ILN_2006 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4306 AR 9 1969 2 10 439-445 |
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10.1007/BF02391668 doi (DE-627)OLC2033520307 (DE-He213)BF02391668-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Edlén, Bengt verfasserin aut On the identification of Ar x and Ar xiv in the solar corona and the origin of the unidentified coronal lines 1969 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1969 Abstract A study of theZ-dependence of $ the^{2} $P intervals of 2s22p and 2s22p5, aided by recent observational results, confirms the identification in the coronal spectrum of λ 4412 with Arxiv, and of λ 5533.4 with Arx. It is further shown that transitions from metastable levels in the configurations 3s23pk 3d, withk=3, 4 and 5, of Fexi,x, ix, and Nixiii, xiii, xi can well account for the remaining unidentified coronal lines. Solar Corona Observational Result Metastable Level Coronal Line Recent Observational Result Enthalten in Solar physics Kluwer Academic Publishers, 1967 9(1969), 2 vom: Okt., Seite 439-445 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:9 year:1969 number:2 month:10 pages:439-445 https://doi.org/10.1007/BF02391668 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_24 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2002 GBV_ILN_2006 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4306 AR 9 1969 2 10 439-445 |
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on the identification of ar x and ar xiv in the solar corona and the origin of the unidentified coronal lines |
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On the identification of Ar x and Ar xiv in the solar corona and the origin of the unidentified coronal lines |
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Abstract A study of theZ-dependence of $ the^{2} $P intervals of 2s22p and 2s22p5, aided by recent observational results, confirms the identification in the coronal spectrum of λ 4412 with Arxiv, and of λ 5533.4 with Arx. It is further shown that transitions from metastable levels in the configurations 3s23pk 3d, withk=3, 4 and 5, of Fexi,x, ix, and Nixiii, xiii, xi can well account for the remaining unidentified coronal lines. © D. Reidel Publishing Company 1969 |
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Abstract A study of theZ-dependence of $ the^{2} $P intervals of 2s22p and 2s22p5, aided by recent observational results, confirms the identification in the coronal spectrum of λ 4412 with Arxiv, and of λ 5533.4 with Arx. It is further shown that transitions from metastable levels in the configurations 3s23pk 3d, withk=3, 4 and 5, of Fexi,x, ix, and Nixiii, xiii, xi can well account for the remaining unidentified coronal lines. © D. Reidel Publishing Company 1969 |
| abstract_unstemmed |
Abstract A study of theZ-dependence of $ the^{2} $P intervals of 2s22p and 2s22p5, aided by recent observational results, confirms the identification in the coronal spectrum of λ 4412 with Arxiv, and of λ 5533.4 with Arx. It is further shown that transitions from metastable levels in the configurations 3s23pk 3d, withk=3, 4 and 5, of Fexi,x, ix, and Nixiii, xiii, xi can well account for the remaining unidentified coronal lines. © D. Reidel Publishing Company 1969 |
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On the identification of Ar x and Ar xiv in the solar corona and the origin of the unidentified coronal lines |
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