Velocity measures in the sunspot Rome no. 7490 (July 5, 1979)
Abstract Material motions on the solar surface have been deduced from the wavelength shift of Fe i λ6302.5 Å, measured over the umbra and inner penumbra of a spot for which the magnetic field configuration has already been established with some confidence. The two vector fields are considered togeth...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Adam, M. G. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
1991 |
|---|
| Schlagwörter: |
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| Anmerkung: |
© Kluwer Academic Publishers 1991 |
|---|
| Übergeordnetes Werk: |
Enthalten in: Solar physics - Kluwer Academic Publishers, 1967, 135(1991), 2 vom: Okt., Seite 319-326 |
|---|---|
| Übergeordnetes Werk: |
volume:135 ; year:1991 ; number:2 ; month:10 ; pages:319-326 |
| Links: |
|---|
| DOI / URN: |
10.1007/BF00147503 |
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OLC2033569969 |
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| 520 | |a Abstract Material motions on the solar surface have been deduced from the wavelength shift of Fe i λ6302.5 Å, measured over the umbra and inner penumbra of a spot for which the magnetic field configuration has already been established with some confidence. The two vector fields are considered together in detail and the results support the ‘convective roll’ sunspot model (Spruit, Galloway). For the magnetic field regions, both material flow along the field lines and field line motions are derived. A small upward motion only is deduced for the field free regions. | ||
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10.1007/BF00147503 doi (DE-627)OLC2033569969 (DE-He213)BF00147503-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Adam, M. G. verfasserin aut Velocity measures in the sunspot Rome no. 7490 (July 5, 1979) 1991 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1991 Abstract Material motions on the solar surface have been deduced from the wavelength shift of Fe i λ6302.5 Å, measured over the umbra and inner penumbra of a spot for which the magnetic field configuration has already been established with some confidence. The two vector fields are considered together in detail and the results support the ‘convective roll’ sunspot model (Spruit, Galloway). For the magnetic field regions, both material flow along the field lines and field line motions are derived. A small upward motion only is deduced for the field free regions. Magnetic Field Vector Field Field Line Velocity Measure Material Flow Petford, A. D. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 135(1991), 2 vom: Okt., Seite 319-326 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:135 year:1991 number:2 month:10 pages:319-326 https://doi.org/10.1007/BF00147503 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4306 AR 135 1991 2 10 319-326 |
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10.1007/BF00147503 doi (DE-627)OLC2033569969 (DE-He213)BF00147503-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Adam, M. G. verfasserin aut Velocity measures in the sunspot Rome no. 7490 (July 5, 1979) 1991 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1991 Abstract Material motions on the solar surface have been deduced from the wavelength shift of Fe i λ6302.5 Å, measured over the umbra and inner penumbra of a spot for which the magnetic field configuration has already been established with some confidence. The two vector fields are considered together in detail and the results support the ‘convective roll’ sunspot model (Spruit, Galloway). For the magnetic field regions, both material flow along the field lines and field line motions are derived. A small upward motion only is deduced for the field free regions. Magnetic Field Vector Field Field Line Velocity Measure Material Flow Petford, A. D. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 135(1991), 2 vom: Okt., Seite 319-326 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:135 year:1991 number:2 month:10 pages:319-326 https://doi.org/10.1007/BF00147503 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4306 AR 135 1991 2 10 319-326 |
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10.1007/BF00147503 doi (DE-627)OLC2033569969 (DE-He213)BF00147503-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Adam, M. G. verfasserin aut Velocity measures in the sunspot Rome no. 7490 (July 5, 1979) 1991 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1991 Abstract Material motions on the solar surface have been deduced from the wavelength shift of Fe i λ6302.5 Å, measured over the umbra and inner penumbra of a spot for which the magnetic field configuration has already been established with some confidence. The two vector fields are considered together in detail and the results support the ‘convective roll’ sunspot model (Spruit, Galloway). For the magnetic field regions, both material flow along the field lines and field line motions are derived. A small upward motion only is deduced for the field free regions. Magnetic Field Vector Field Field Line Velocity Measure Material Flow Petford, A. D. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 135(1991), 2 vom: Okt., Seite 319-326 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:135 year:1991 number:2 month:10 pages:319-326 https://doi.org/10.1007/BF00147503 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4306 AR 135 1991 2 10 319-326 |
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10.1007/BF00147503 doi (DE-627)OLC2033569969 (DE-He213)BF00147503-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Adam, M. G. verfasserin aut Velocity measures in the sunspot Rome no. 7490 (July 5, 1979) 1991 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1991 Abstract Material motions on the solar surface have been deduced from the wavelength shift of Fe i λ6302.5 Å, measured over the umbra and inner penumbra of a spot for which the magnetic field configuration has already been established with some confidence. The two vector fields are considered together in detail and the results support the ‘convective roll’ sunspot model (Spruit, Galloway). For the magnetic field regions, both material flow along the field lines and field line motions are derived. A small upward motion only is deduced for the field free regions. Magnetic Field Vector Field Field Line Velocity Measure Material Flow Petford, A. D. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 135(1991), 2 vom: Okt., Seite 319-326 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:135 year:1991 number:2 month:10 pages:319-326 https://doi.org/10.1007/BF00147503 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4306 AR 135 1991 2 10 319-326 |
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Abstract Material motions on the solar surface have been deduced from the wavelength shift of Fe i λ6302.5 Å, measured over the umbra and inner penumbra of a spot for which the magnetic field configuration has already been established with some confidence. The two vector fields are considered together in detail and the results support the ‘convective roll’ sunspot model (Spruit, Galloway). For the magnetic field regions, both material flow along the field lines and field line motions are derived. A small upward motion only is deduced for the field free regions. © Kluwer Academic Publishers 1991 |
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Abstract Material motions on the solar surface have been deduced from the wavelength shift of Fe i λ6302.5 Å, measured over the umbra and inner penumbra of a spot for which the magnetic field configuration has already been established with some confidence. The two vector fields are considered together in detail and the results support the ‘convective roll’ sunspot model (Spruit, Galloway). For the magnetic field regions, both material flow along the field lines and field line motions are derived. A small upward motion only is deduced for the field free regions. © Kluwer Academic Publishers 1991 |
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Abstract Material motions on the solar surface have been deduced from the wavelength shift of Fe i λ6302.5 Å, measured over the umbra and inner penumbra of a spot for which the magnetic field configuration has already been established with some confidence. The two vector fields are considered together in detail and the results support the ‘convective roll’ sunspot model (Spruit, Galloway). For the magnetic field regions, both material flow along the field lines and field line motions are derived. A small upward motion only is deduced for the field free regions. © Kluwer Academic Publishers 1991 |
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G.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Velocity measures in the sunspot Rome no. 7490 (July 5, 1979)</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1991</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© Kluwer Academic Publishers 1991</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract Material motions on the solar surface have been deduced from the wavelength shift of Fe i λ6302.5 Å, measured over the umbra and inner penumbra of a spot for which the magnetic field configuration has already been established with some confidence. The two vector fields are considered together in detail and the results support the ‘convective roll’ sunspot model (Spruit, Galloway). For the magnetic field regions, both material flow along the field lines and field line motions are derived. A small upward motion only is deduced for the field free regions.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Magnetic Field</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Vector Field</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Field Line</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Velocity Measure</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Material Flow</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Petford, A. 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