The properties of velocity oscillations in vicinities of sunspot penumbra
Abstract It is suggested that the problem of the extent of the outer penumbra could be considered by investigating the range over which the influence of the penumbra on the oscillation regime of the surrounding medium extends. In summer 1998, velocity oscillations were observed in the vicinities of...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Kobanov, N.I. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
2000 |
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| Schlagwörter: |
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| Anmerkung: |
© Kluwer Academic Publishers 2000 |
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| Übergeordnetes Werk: |
Enthalten in: Solar physics - Kluwer Academic Publishers, 1967, 196(2000), 1 vom: Sept., Seite 129-135 |
|---|---|
| Übergeordnetes Werk: |
volume:196 ; year:2000 ; number:1 ; month:09 ; pages:129-135 |
| Links: |
|---|
| DOI / URN: |
10.1023/A:1005201330825 |
|---|
| Katalog-ID: |
OLC2033590070 |
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| 520 | |a Abstract It is suggested that the problem of the extent of the outer penumbra could be considered by investigating the range over which the influence of the penumbra on the oscillation regime of the surrounding medium extends. In summer 1998, velocity oscillations were observed in the vicinities of the penumbra of the NOAA 8263 sunspot. The observations were carried out in the Hβ line (chromosphere) and in the far wing of Ni i 4857.2 Å (lower photosphere) simultaneously. The oscillation regime typical for sunspot penumbrae is observed within distances of about $ 15^{′′} $ from the visible outer boundary of the penumbra. | ||
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| 650 | 4 | |a Velocity Oscillation | |
| 650 | 4 | |a Visible Outer Boundary | |
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10.1023/A:1005201330825 doi (DE-627)OLC2033590070 (DE-He213)A:1005201330825-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Kobanov, N.I. verfasserin aut The properties of velocity oscillations in vicinities of sunspot penumbra 2000 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2000 Abstract It is suggested that the problem of the extent of the outer penumbra could be considered by investigating the range over which the influence of the penumbra on the oscillation regime of the surrounding medium extends. In summer 1998, velocity oscillations were observed in the vicinities of the penumbra of the NOAA 8263 sunspot. The observations were carried out in the Hβ line (chromosphere) and in the far wing of Ni i 4857.2 Å (lower photosphere) simultaneously. The oscillation regime typical for sunspot penumbrae is observed within distances of about $ 15^{′′} $ from the visible outer boundary of the penumbra. Outer Boundary Surrounding Medium Oscillation Regime Velocity Oscillation Visible Outer Boundary Enthalten in Solar physics Kluwer Academic Publishers, 1967 196(2000), 1 vom: Sept., Seite 129-135 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:196 year:2000 number:1 month:09 pages:129-135 https://doi.org/10.1023/A:1005201330825 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_2286 AR 196 2000 1 09 129-135 |
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10.1023/A:1005201330825 doi (DE-627)OLC2033590070 (DE-He213)A:1005201330825-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Kobanov, N.I. verfasserin aut The properties of velocity oscillations in vicinities of sunspot penumbra 2000 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2000 Abstract It is suggested that the problem of the extent of the outer penumbra could be considered by investigating the range over which the influence of the penumbra on the oscillation regime of the surrounding medium extends. In summer 1998, velocity oscillations were observed in the vicinities of the penumbra of the NOAA 8263 sunspot. The observations were carried out in the Hβ line (chromosphere) and in the far wing of Ni i 4857.2 Å (lower photosphere) simultaneously. The oscillation regime typical for sunspot penumbrae is observed within distances of about $ 15^{′′} $ from the visible outer boundary of the penumbra. Outer Boundary Surrounding Medium Oscillation Regime Velocity Oscillation Visible Outer Boundary Enthalten in Solar physics Kluwer Academic Publishers, 1967 196(2000), 1 vom: Sept., Seite 129-135 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:196 year:2000 number:1 month:09 pages:129-135 https://doi.org/10.1023/A:1005201330825 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_2286 AR 196 2000 1 09 129-135 |
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10.1023/A:1005201330825 doi (DE-627)OLC2033590070 (DE-He213)A:1005201330825-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Kobanov, N.I. verfasserin aut The properties of velocity oscillations in vicinities of sunspot penumbra 2000 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2000 Abstract It is suggested that the problem of the extent of the outer penumbra could be considered by investigating the range over which the influence of the penumbra on the oscillation regime of the surrounding medium extends. In summer 1998, velocity oscillations were observed in the vicinities of the penumbra of the NOAA 8263 sunspot. The observations were carried out in the Hβ line (chromosphere) and in the far wing of Ni i 4857.2 Å (lower photosphere) simultaneously. The oscillation regime typical for sunspot penumbrae is observed within distances of about $ 15^{′′} $ from the visible outer boundary of the penumbra. Outer Boundary Surrounding Medium Oscillation Regime Velocity Oscillation Visible Outer Boundary Enthalten in Solar physics Kluwer Academic Publishers, 1967 196(2000), 1 vom: Sept., Seite 129-135 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:196 year:2000 number:1 month:09 pages:129-135 https://doi.org/10.1023/A:1005201330825 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_2286 AR 196 2000 1 09 129-135 |
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10.1023/A:1005201330825 doi (DE-627)OLC2033590070 (DE-He213)A:1005201330825-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Kobanov, N.I. verfasserin aut The properties of velocity oscillations in vicinities of sunspot penumbra 2000 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 2000 Abstract It is suggested that the problem of the extent of the outer penumbra could be considered by investigating the range over which the influence of the penumbra on the oscillation regime of the surrounding medium extends. In summer 1998, velocity oscillations were observed in the vicinities of the penumbra of the NOAA 8263 sunspot. The observations were carried out in the Hβ line (chromosphere) and in the far wing of Ni i 4857.2 Å (lower photosphere) simultaneously. The oscillation regime typical for sunspot penumbrae is observed within distances of about $ 15^{′′} $ from the visible outer boundary of the penumbra. Outer Boundary Surrounding Medium Oscillation Regime Velocity Oscillation Visible Outer Boundary Enthalten in Solar physics Kluwer Academic Publishers, 1967 196(2000), 1 vom: Sept., Seite 129-135 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:196 year:2000 number:1 month:09 pages:129-135 https://doi.org/10.1023/A:1005201330825 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_2286 AR 196 2000 1 09 129-135 |
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Abstract It is suggested that the problem of the extent of the outer penumbra could be considered by investigating the range over which the influence of the penumbra on the oscillation regime of the surrounding medium extends. In summer 1998, velocity oscillations were observed in the vicinities of the penumbra of the NOAA 8263 sunspot. The observations were carried out in the Hβ line (chromosphere) and in the far wing of Ni i 4857.2 Å (lower photosphere) simultaneously. The oscillation regime typical for sunspot penumbrae is observed within distances of about $ 15^{′′} $ from the visible outer boundary of the penumbra. © Kluwer Academic Publishers 2000 |
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Abstract It is suggested that the problem of the extent of the outer penumbra could be considered by investigating the range over which the influence of the penumbra on the oscillation regime of the surrounding medium extends. In summer 1998, velocity oscillations were observed in the vicinities of the penumbra of the NOAA 8263 sunspot. The observations were carried out in the Hβ line (chromosphere) and in the far wing of Ni i 4857.2 Å (lower photosphere) simultaneously. The oscillation regime typical for sunspot penumbrae is observed within distances of about $ 15^{′′} $ from the visible outer boundary of the penumbra. © Kluwer Academic Publishers 2000 |
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Abstract It is suggested that the problem of the extent of the outer penumbra could be considered by investigating the range over which the influence of the penumbra on the oscillation regime of the surrounding medium extends. In summer 1998, velocity oscillations were observed in the vicinities of the penumbra of the NOAA 8263 sunspot. The observations were carried out in the Hβ line (chromosphere) and in the far wing of Ni i 4857.2 Å (lower photosphere) simultaneously. The oscillation regime typical for sunspot penumbrae is observed within distances of about $ 15^{′′} $ from the visible outer boundary of the penumbra. © Kluwer Academic Publishers 2000 |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2033590070</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230504045649.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200819s2000 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1023/A:1005201330825</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2033590070</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)A:1005201330825-p</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">530</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">16,12</subfield><subfield code="2">ssgn</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Kobanov, N.I.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">The properties of velocity oscillations in vicinities of sunspot penumbra</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2000</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 2000</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract It is suggested that the problem of the extent of the outer penumbra could be considered by investigating the range over which the influence of the penumbra on the oscillation regime of the surrounding medium extends. In summer 1998, velocity oscillations were observed in the vicinities of the penumbra of the NOAA 8263 sunspot. The observations were carried out in the Hβ line (chromosphere) and in the far wing of Ni i 4857.2 Å (lower photosphere) simultaneously. 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