On the asymmetry of selected Fraunhofer lines
Abstract An analysis is made of the asymmetry of Fraunhofer lines observed with the double-pass monochromator of the horizontal solar telescope ASU-5 of the Main Astronomical Observatory of the Ukrainian Academy of Sciences. The conclusion is that the character of macromotion in the radial direction...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1977 |
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| Umfang: |
6 |
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| Reproduktion: |
Springer Online Journal Archives 1860-2002 |
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| Übergeordnetes Werk: |
in: Solar physics - 1967, 53(1977) vom: Feb., Seite 353-358 |
| Übergeordnetes Werk: |
volume:53 ; year:1977 ; month:02 ; pages:353-358 ; extent:6 |
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| 520 | |a Abstract An analysis is made of the asymmetry of Fraunhofer lines observed with the double-pass monochromator of the horizontal solar telescope ASU-5 of the Main Astronomical Observatory of the Ukrainian Academy of Sciences. The conclusion is that the character of macromotion in the radial direction varies with height; in a tangential direction the motions at different depths are homogeneous. The asymmetry of weak lines is due to convection rather than to wave motions. | ||
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| 700 | 1 | |a Orlova, T. V. |4 oth | |
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(DE-627)NLEJ195889665 DE-627 ger DE-627 rakwb eng On the asymmetry of selected Fraunhofer lines 1977 6 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract An analysis is made of the asymmetry of Fraunhofer lines observed with the double-pass monochromator of the horizontal solar telescope ASU-5 of the Main Astronomical Observatory of the Ukrainian Academy of Sciences. The conclusion is that the character of macromotion in the radial direction varies with height; in a tangential direction the motions at different depths are homogeneous. The asymmetry of weak lines is due to convection rather than to wave motions. Springer Online Journal Archives 1860-2002 Kostik, R. I. oth Orlova, T. V. oth in Solar physics 1967 53(1977) vom: Feb., Seite 353-358 (DE-627)NLEJ188983465 (DE-600)1473830-2 1573-093X nnns volume:53 year:1977 month:02 pages:353-358 extent:6 http://dx.doi.org/10.1007/BF00160278 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 53 1977 2 353-358 6 |
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(DE-627)NLEJ195889665 DE-627 ger DE-627 rakwb eng On the asymmetry of selected Fraunhofer lines 1977 6 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract An analysis is made of the asymmetry of Fraunhofer lines observed with the double-pass monochromator of the horizontal solar telescope ASU-5 of the Main Astronomical Observatory of the Ukrainian Academy of Sciences. The conclusion is that the character of macromotion in the radial direction varies with height; in a tangential direction the motions at different depths are homogeneous. The asymmetry of weak lines is due to convection rather than to wave motions. Springer Online Journal Archives 1860-2002 Kostik, R. I. oth Orlova, T. V. oth in Solar physics 1967 53(1977) vom: Feb., Seite 353-358 (DE-627)NLEJ188983465 (DE-600)1473830-2 1573-093X nnns volume:53 year:1977 month:02 pages:353-358 extent:6 http://dx.doi.org/10.1007/BF00160278 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 53 1977 2 353-358 6 |
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(DE-627)NLEJ195889665 DE-627 ger DE-627 rakwb eng On the asymmetry of selected Fraunhofer lines 1977 6 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract An analysis is made of the asymmetry of Fraunhofer lines observed with the double-pass monochromator of the horizontal solar telescope ASU-5 of the Main Astronomical Observatory of the Ukrainian Academy of Sciences. The conclusion is that the character of macromotion in the radial direction varies with height; in a tangential direction the motions at different depths are homogeneous. The asymmetry of weak lines is due to convection rather than to wave motions. Springer Online Journal Archives 1860-2002 Kostik, R. I. oth Orlova, T. V. oth in Solar physics 1967 53(1977) vom: Feb., Seite 353-358 (DE-627)NLEJ188983465 (DE-600)1473830-2 1573-093X nnns volume:53 year:1977 month:02 pages:353-358 extent:6 http://dx.doi.org/10.1007/BF00160278 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 53 1977 2 353-358 6 |
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(DE-627)NLEJ195889665 DE-627 ger DE-627 rakwb eng On the asymmetry of selected Fraunhofer lines 1977 6 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract An analysis is made of the asymmetry of Fraunhofer lines observed with the double-pass monochromator of the horizontal solar telescope ASU-5 of the Main Astronomical Observatory of the Ukrainian Academy of Sciences. The conclusion is that the character of macromotion in the radial direction varies with height; in a tangential direction the motions at different depths are homogeneous. The asymmetry of weak lines is due to convection rather than to wave motions. Springer Online Journal Archives 1860-2002 Kostik, R. I. oth Orlova, T. V. oth in Solar physics 1967 53(1977) vom: Feb., Seite 353-358 (DE-627)NLEJ188983465 (DE-600)1473830-2 1573-093X nnns volume:53 year:1977 month:02 pages:353-358 extent:6 http://dx.doi.org/10.1007/BF00160278 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 53 1977 2 353-358 6 |
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(DE-627)NLEJ195889665 DE-627 ger DE-627 rakwb eng On the asymmetry of selected Fraunhofer lines 1977 6 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract An analysis is made of the asymmetry of Fraunhofer lines observed with the double-pass monochromator of the horizontal solar telescope ASU-5 of the Main Astronomical Observatory of the Ukrainian Academy of Sciences. The conclusion is that the character of macromotion in the radial direction varies with height; in a tangential direction the motions at different depths are homogeneous. The asymmetry of weak lines is due to convection rather than to wave motions. Springer Online Journal Archives 1860-2002 Kostik, R. I. oth Orlova, T. V. oth in Solar physics 1967 53(1977) vom: Feb., Seite 353-358 (DE-627)NLEJ188983465 (DE-600)1473830-2 1573-093X nnns volume:53 year:1977 month:02 pages:353-358 extent:6 http://dx.doi.org/10.1007/BF00160278 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 53 1977 2 353-358 6 |
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in Solar physics 53(1977) vom: Feb., Seite 353-358 volume:53 year:1977 month:02 pages:353-358 extent:6 |
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Abstract An analysis is made of the asymmetry of Fraunhofer lines observed with the double-pass monochromator of the horizontal solar telescope ASU-5 of the Main Astronomical Observatory of the Ukrainian Academy of Sciences. The conclusion is that the character of macromotion in the radial direction varies with height; in a tangential direction the motions at different depths are homogeneous. The asymmetry of weak lines is due to convection rather than to wave motions. |
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Abstract An analysis is made of the asymmetry of Fraunhofer lines observed with the double-pass monochromator of the horizontal solar telescope ASU-5 of the Main Astronomical Observatory of the Ukrainian Academy of Sciences. The conclusion is that the character of macromotion in the radial direction varies with height; in a tangential direction the motions at different depths are homogeneous. The asymmetry of weak lines is due to convection rather than to wave motions. |
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Abstract An analysis is made of the asymmetry of Fraunhofer lines observed with the double-pass monochromator of the horizontal solar telescope ASU-5 of the Main Astronomical Observatory of the Ukrainian Academy of Sciences. The conclusion is that the character of macromotion in the radial direction varies with height; in a tangential direction the motions at different depths are homogeneous. The asymmetry of weak lines is due to convection rather than to wave motions. |
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