Height of Tracers and the Correction of the Measured Solar Synodic Rotation Rate: Demonstration of the Method
Abstract Two large stable solar filaments were used as test tracers to determine the apparent synodic rotation rate as a function of the central meridian distance for several filaments' segments at different heights. An analytic fitting procedure was applied to determine simultaneously the real...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Vršnak, B. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
1999 |
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| Schlagwörter: |
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| Anmerkung: |
© Kluwer Academic Publishers 1999 |
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| Übergeordnetes Werk: |
Enthalten in: Solar physics - Kluwer Academic Publishers, 1967, 185(1999), 2 vom: Apr., Seite 207-225 |
|---|---|
| Übergeordnetes Werk: |
volume:185 ; year:1999 ; number:2 ; month:04 ; pages:207-225 |
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| DOI / URN: |
10.1023/A:1005107424355 |
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OLC2033587029 |
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| 520 | |a Abstract Two large stable solar filaments were used as test tracers to determine the apparent synodic rotation rate as a function of the central meridian distance for several filaments' segments at different heights. An analytic fitting procedure was applied to determine simultaneously the real synodic rotation rate and the height of the traced filament segments. The determined heights were compared with the values obtained from the widths of filament contours on the solar disk and with the values obtained by direct measurements at the solar limb. Furthermore, the obtained rotation rates and heights of the filaments' segments close to the filaments' pivot points were compared with the values obtained using two successive central meridian passages. Finally, sources and scales of errors were investigated and possible implications on the previous studies of the solar differential rotation were considered. | ||
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| 700 | 1 | |a Roša, D. |4 aut | |
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| 700 | 1 | |a Ruždjak, V. |4 aut | |
| 700 | 1 | |a Schroll, A. |4 aut | |
| 700 | 1 | |a Wöhl, H. |4 aut | |
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10.1023/A:1005107424355 doi (DE-627)OLC2033587029 (DE-He213)A:1005107424355-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Vršnak, B. verfasserin aut Height of Tracers and the Correction of the Measured Solar Synodic Rotation Rate: Demonstration of the Method 1999 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1999 Abstract Two large stable solar filaments were used as test tracers to determine the apparent synodic rotation rate as a function of the central meridian distance for several filaments' segments at different heights. An analytic fitting procedure was applied to determine simultaneously the real synodic rotation rate and the height of the traced filament segments. The determined heights were compared with the values obtained from the widths of filament contours on the solar disk and with the values obtained by direct measurements at the solar limb. Furthermore, the obtained rotation rates and heights of the filaments' segments close to the filaments' pivot points were compared with the values obtained using two successive central meridian passages. Finally, sources and scales of errors were investigated and possible implications on the previous studies of the solar differential rotation were considered. Direct Measurement Rotation Rate Solar Disk Test Tracer Differential Rotation Roša, D. aut Božić, H. aut Brajša, R. aut Ruždjak, V. aut Schroll, A. aut Wöhl, H. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 185(1999), 2 vom: Apr., Seite 207-225 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:185 year:1999 number:2 month:04 pages:207-225 https://doi.org/10.1023/A:1005107424355 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_2279 GBV_ILN_2286 GBV_ILN_4306 AR 185 1999 2 04 207-225 |
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10.1023/A:1005107424355 doi (DE-627)OLC2033587029 (DE-He213)A:1005107424355-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Vršnak, B. verfasserin aut Height of Tracers and the Correction of the Measured Solar Synodic Rotation Rate: Demonstration of the Method 1999 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1999 Abstract Two large stable solar filaments were used as test tracers to determine the apparent synodic rotation rate as a function of the central meridian distance for several filaments' segments at different heights. An analytic fitting procedure was applied to determine simultaneously the real synodic rotation rate and the height of the traced filament segments. The determined heights were compared with the values obtained from the widths of filament contours on the solar disk and with the values obtained by direct measurements at the solar limb. Furthermore, the obtained rotation rates and heights of the filaments' segments close to the filaments' pivot points were compared with the values obtained using two successive central meridian passages. Finally, sources and scales of errors were investigated and possible implications on the previous studies of the solar differential rotation were considered. Direct Measurement Rotation Rate Solar Disk Test Tracer Differential Rotation Roša, D. aut Božić, H. aut Brajša, R. aut Ruždjak, V. aut Schroll, A. aut Wöhl, H. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 185(1999), 2 vom: Apr., Seite 207-225 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:185 year:1999 number:2 month:04 pages:207-225 https://doi.org/10.1023/A:1005107424355 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_2279 GBV_ILN_2286 GBV_ILN_4306 AR 185 1999 2 04 207-225 |
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10.1023/A:1005107424355 doi (DE-627)OLC2033587029 (DE-He213)A:1005107424355-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Vršnak, B. verfasserin aut Height of Tracers and the Correction of the Measured Solar Synodic Rotation Rate: Demonstration of the Method 1999 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1999 Abstract Two large stable solar filaments were used as test tracers to determine the apparent synodic rotation rate as a function of the central meridian distance for several filaments' segments at different heights. An analytic fitting procedure was applied to determine simultaneously the real synodic rotation rate and the height of the traced filament segments. The determined heights were compared with the values obtained from the widths of filament contours on the solar disk and with the values obtained by direct measurements at the solar limb. Furthermore, the obtained rotation rates and heights of the filaments' segments close to the filaments' pivot points were compared with the values obtained using two successive central meridian passages. Finally, sources and scales of errors were investigated and possible implications on the previous studies of the solar differential rotation were considered. Direct Measurement Rotation Rate Solar Disk Test Tracer Differential Rotation Roša, D. aut Božić, H. aut Brajša, R. aut Ruždjak, V. aut Schroll, A. aut Wöhl, H. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 185(1999), 2 vom: Apr., Seite 207-225 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:185 year:1999 number:2 month:04 pages:207-225 https://doi.org/10.1023/A:1005107424355 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_2279 GBV_ILN_2286 GBV_ILN_4306 AR 185 1999 2 04 207-225 |
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10.1023/A:1005107424355 doi (DE-627)OLC2033587029 (DE-He213)A:1005107424355-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Vršnak, B. verfasserin aut Height of Tracers and the Correction of the Measured Solar Synodic Rotation Rate: Demonstration of the Method 1999 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1999 Abstract Two large stable solar filaments were used as test tracers to determine the apparent synodic rotation rate as a function of the central meridian distance for several filaments' segments at different heights. An analytic fitting procedure was applied to determine simultaneously the real synodic rotation rate and the height of the traced filament segments. The determined heights were compared with the values obtained from the widths of filament contours on the solar disk and with the values obtained by direct measurements at the solar limb. Furthermore, the obtained rotation rates and heights of the filaments' segments close to the filaments' pivot points were compared with the values obtained using two successive central meridian passages. Finally, sources and scales of errors were investigated and possible implications on the previous studies of the solar differential rotation were considered. Direct Measurement Rotation Rate Solar Disk Test Tracer Differential Rotation Roša, D. aut Božić, H. aut Brajša, R. aut Ruždjak, V. aut Schroll, A. aut Wöhl, H. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 185(1999), 2 vom: Apr., Seite 207-225 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:185 year:1999 number:2 month:04 pages:207-225 https://doi.org/10.1023/A:1005107424355 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_2279 GBV_ILN_2286 GBV_ILN_4306 AR 185 1999 2 04 207-225 |
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Height of Tracers and the Correction of the Measured Solar Synodic Rotation Rate: Demonstration of the Method |
| abstract |
Abstract Two large stable solar filaments were used as test tracers to determine the apparent synodic rotation rate as a function of the central meridian distance for several filaments' segments at different heights. An analytic fitting procedure was applied to determine simultaneously the real synodic rotation rate and the height of the traced filament segments. The determined heights were compared with the values obtained from the widths of filament contours on the solar disk and with the values obtained by direct measurements at the solar limb. Furthermore, the obtained rotation rates and heights of the filaments' segments close to the filaments' pivot points were compared with the values obtained using two successive central meridian passages. Finally, sources and scales of errors were investigated and possible implications on the previous studies of the solar differential rotation were considered. © Kluwer Academic Publishers 1999 |
| abstractGer |
Abstract Two large stable solar filaments were used as test tracers to determine the apparent synodic rotation rate as a function of the central meridian distance for several filaments' segments at different heights. An analytic fitting procedure was applied to determine simultaneously the real synodic rotation rate and the height of the traced filament segments. The determined heights were compared with the values obtained from the widths of filament contours on the solar disk and with the values obtained by direct measurements at the solar limb. Furthermore, the obtained rotation rates and heights of the filaments' segments close to the filaments' pivot points were compared with the values obtained using two successive central meridian passages. Finally, sources and scales of errors were investigated and possible implications on the previous studies of the solar differential rotation were considered. © Kluwer Academic Publishers 1999 |
| abstract_unstemmed |
Abstract Two large stable solar filaments were used as test tracers to determine the apparent synodic rotation rate as a function of the central meridian distance for several filaments' segments at different heights. An analytic fitting procedure was applied to determine simultaneously the real synodic rotation rate and the height of the traced filament segments. The determined heights were compared with the values obtained from the widths of filament contours on the solar disk and with the values obtained by direct measurements at the solar limb. Furthermore, the obtained rotation rates and heights of the filaments' segments close to the filaments' pivot points were compared with the values obtained using two successive central meridian passages. Finally, sources and scales of errors were investigated and possible implications on the previous studies of the solar differential rotation were considered. © Kluwer Academic Publishers 1999 |
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| title_short |
Height of Tracers and the Correction of the Measured Solar Synodic Rotation Rate: Demonstration of the Method |
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https://doi.org/10.1023/A:1005107424355 |
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Roša, D. Božić, H. Brajša, R. Ruždjak, V. Schroll, A. Wöhl, H. |
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Roša, D. Božić, H. Brajša, R. Ruždjak, V. Schroll, A. Wöhl, H. |
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10.1023/A:1005107424355 |
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2024-07-03T17:34:56.680Z |
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