Line asymmetries in $ Ca^{+} $-active regions
Abstract Spatially-resolved Fei line bisectors were studied in magnetically active and non-active regions. In active regions, small-scale velocities which are of convective origin, were reduced by a factor of 1.9 and individual bisectors originating in granular-intergranular regions showed a differe...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Hanslmeier, A. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
1990 |
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| Schlagwörter: |
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| Anmerkung: |
© Kluwer Academic Publishers 1990 |
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| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 170(1990), 1-2 vom: Aug., Seite 51-53 |
|---|---|
| Übergeordnetes Werk: |
volume:170 ; year:1990 ; number:1-2 ; month:08 ; pages:51-53 |
| Links: |
|---|
| DOI / URN: |
10.1007/BF00652644 |
|---|
| Katalog-ID: |
OLC2066181471 |
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| 520 | |a Abstract Spatially-resolved Fei line bisectors were studied in magnetically active and non-active regions. In active regions, small-scale velocities which are of convective origin, were reduced by a factor of 1.9 and individual bisectors originating in granular-intergranular regions showed a different behaviour. | ||
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Abstract Spatially-resolved Fei line bisectors were studied in magnetically active and non-active regions. In active regions, small-scale velocities which are of convective origin, were reduced by a factor of 1.9 and individual bisectors originating in granular-intergranular regions showed a different behaviour. © Kluwer Academic Publishers 1990 |
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Abstract Spatially-resolved Fei line bisectors were studied in magnetically active and non-active regions. In active regions, small-scale velocities which are of convective origin, were reduced by a factor of 1.9 and individual bisectors originating in granular-intergranular regions showed a different behaviour. © Kluwer Academic Publishers 1990 |
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Abstract Spatially-resolved Fei line bisectors were studied in magnetically active and non-active regions. In active regions, small-scale velocities which are of convective origin, were reduced by a factor of 1.9 and individual bisectors originating in granular-intergranular regions showed a different behaviour. © Kluwer Academic Publishers 1990 |
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