Large-scale component of dynamics of the local solar sources of cm-radiation
Abstract The large-scale component of the dynamics of local solar source radiation was found according to observations with the radio telescope RATAN-600 by the ‘relay’ method at wavelengths 2.3 cm and 4.5 cm on 17 July and 29 July, 1981. The local solar sources were identified with groups of spots...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Golubchina, O. A. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
1995 |
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| Schlagwörter: |
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| Anmerkung: |
© Kluwer Academic Publishers 1995 |
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| Übergeordnetes Werk: |
Enthalten in: Solar physics - Kluwer Academic Publishers, 1967, 160(1995), 1 vom: Aug., Seite 199-206 |
|---|---|
| Übergeordnetes Werk: |
volume:160 ; year:1995 ; number:1 ; month:08 ; pages:199-206 |
| Links: |
|---|
| DOI / URN: |
10.1007/BF00679105 |
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| Katalog-ID: |
OLC2033578178 |
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10.1007/BF00679105 doi (DE-627)OLC2033578178 (DE-He213)BF00679105-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Golubchina, O. A. verfasserin aut Large-scale component of dynamics of the local solar sources of cm-radiation 1995 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1995 Abstract The large-scale component of the dynamics of local solar source radiation was found according to observations with the radio telescope RATAN-600 by the ‘relay’ method at wavelengths 2.3 cm and 4.5 cm on 17 July and 29 July, 1981. The local solar sources were identified with groups of spots on the Sun widely separated from each other. Radiation Source Radiation Solar Source Radio Telescope Local Solar Source Enthalten in Solar physics Kluwer Academic Publishers, 1967 160(1995), 1 vom: Aug., Seite 199-206 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:160 year:1995 number:1 month:08 pages:199-206 https://doi.org/10.1007/BF00679105 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_4306 AR 160 1995 1 08 199-206 |
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10.1007/BF00679105 doi (DE-627)OLC2033578178 (DE-He213)BF00679105-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Golubchina, O. A. verfasserin aut Large-scale component of dynamics of the local solar sources of cm-radiation 1995 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1995 Abstract The large-scale component of the dynamics of local solar source radiation was found according to observations with the radio telescope RATAN-600 by the ‘relay’ method at wavelengths 2.3 cm and 4.5 cm on 17 July and 29 July, 1981. The local solar sources were identified with groups of spots on the Sun widely separated from each other. Radiation Source Radiation Solar Source Radio Telescope Local Solar Source Enthalten in Solar physics Kluwer Academic Publishers, 1967 160(1995), 1 vom: Aug., Seite 199-206 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:160 year:1995 number:1 month:08 pages:199-206 https://doi.org/10.1007/BF00679105 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_4306 AR 160 1995 1 08 199-206 |
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10.1007/BF00679105 doi (DE-627)OLC2033578178 (DE-He213)BF00679105-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Golubchina, O. A. verfasserin aut Large-scale component of dynamics of the local solar sources of cm-radiation 1995 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1995 Abstract The large-scale component of the dynamics of local solar source radiation was found according to observations with the radio telescope RATAN-600 by the ‘relay’ method at wavelengths 2.3 cm and 4.5 cm on 17 July and 29 July, 1981. The local solar sources were identified with groups of spots on the Sun widely separated from each other. Radiation Source Radiation Solar Source Radio Telescope Local Solar Source Enthalten in Solar physics Kluwer Academic Publishers, 1967 160(1995), 1 vom: Aug., Seite 199-206 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:160 year:1995 number:1 month:08 pages:199-206 https://doi.org/10.1007/BF00679105 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_4306 AR 160 1995 1 08 199-206 |
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Abstract The large-scale component of the dynamics of local solar source radiation was found according to observations with the radio telescope RATAN-600 by the ‘relay’ method at wavelengths 2.3 cm and 4.5 cm on 17 July and 29 July, 1981. The local solar sources were identified with groups of spots on the Sun widely separated from each other. © Kluwer Academic Publishers 1995 |
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Abstract The large-scale component of the dynamics of local solar source radiation was found according to observations with the radio telescope RATAN-600 by the ‘relay’ method at wavelengths 2.3 cm and 4.5 cm on 17 July and 29 July, 1981. The local solar sources were identified with groups of spots on the Sun widely separated from each other. © Kluwer Academic Publishers 1995 |
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Abstract The large-scale component of the dynamics of local solar source radiation was found according to observations with the radio telescope RATAN-600 by the ‘relay’ method at wavelengths 2.3 cm and 4.5 cm on 17 July and 29 July, 1981. The local solar sources were identified with groups of spots on the Sun widely separated from each other. © Kluwer Academic Publishers 1995 |
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A.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Large-scale component of dynamics of the local solar sources of cm-radiation</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1995</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 1995</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract The large-scale component of the dynamics of local solar source radiation was found according to observations with the radio telescope RATAN-600 by the ‘relay’ method at wavelengths 2.3 cm and 4.5 cm on 17 July and 29 July, 1981. 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