Soft X-ray emission from active regions shortly before solar flares
Abstract Detailed examination of the variations in the intensity of soft X-ray emission prior to many solar flares are presented. In addition, these preflare intensity variations are contrasted with the variations typically observed for the same active regions in the absence of a flare. It is shown...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Wolfson, C. J. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
1982 |
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| Schlagwörter: |
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| Anmerkung: |
© D. Reidel Publishing Co. 1982 |
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| Übergeordnetes Werk: |
Enthalten in: Solar physics - Kluwer Academic Publishers, 1967, 76(1982), 2 vom: März, Seite 377-386 |
|---|---|
| Übergeordnetes Werk: |
volume:76 ; year:1982 ; number:2 ; month:03 ; pages:377-386 |
| Links: |
|---|
| DOI / URN: |
10.1007/BF00170992 |
|---|
| Katalog-ID: |
OLC2033550567 |
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| 520 | |a Abstract Detailed examination of the variations in the intensity of soft X-ray emission prior to many solar flares are presented. In addition, these preflare intensity variations are contrasted with the variations typically observed for the same active regions in the absence of a flare. It is shown that a 5–20 min preflare brightening phase is not typically observed. These observations are discussed in context with other complimentary investigations and theoretical models. | ||
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10.1007/BF00170992 doi (DE-627)OLC2033550567 (DE-He213)BF00170992-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Wolfson, C. J. verfasserin aut Soft X-ray emission from active regions shortly before solar flares 1982 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Co. 1982 Abstract Detailed examination of the variations in the intensity of soft X-ray emission prior to many solar flares are presented. In addition, these preflare intensity variations are contrasted with the variations typically observed for the same active regions in the absence of a flare. It is shown that a 5–20 min preflare brightening phase is not typically observed. These observations are discussed in context with other complimentary investigations and theoretical models. Theoretical Model Flare Active Region Intensity Variation Solar Flare Enthalten in Solar physics Kluwer Academic Publishers, 1967 76(1982), 2 vom: März, Seite 377-386 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:76 year:1982 number:2 month:03 pages:377-386 https://doi.org/10.1007/BF00170992 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 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_4082 GBV_ILN_4305 GBV_ILN_4306 AR 76 1982 2 03 377-386 |
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10.1007/BF00170992 doi (DE-627)OLC2033550567 (DE-He213)BF00170992-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Wolfson, C. J. verfasserin aut Soft X-ray emission from active regions shortly before solar flares 1982 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Co. 1982 Abstract Detailed examination of the variations in the intensity of soft X-ray emission prior to many solar flares are presented. In addition, these preflare intensity variations are contrasted with the variations typically observed for the same active regions in the absence of a flare. It is shown that a 5–20 min preflare brightening phase is not typically observed. These observations are discussed in context with other complimentary investigations and theoretical models. Theoretical Model Flare Active Region Intensity Variation Solar Flare Enthalten in Solar physics Kluwer Academic Publishers, 1967 76(1982), 2 vom: März, Seite 377-386 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:76 year:1982 number:2 month:03 pages:377-386 https://doi.org/10.1007/BF00170992 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 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_4082 GBV_ILN_4305 GBV_ILN_4306 AR 76 1982 2 03 377-386 |
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10.1007/BF00170992 doi (DE-627)OLC2033550567 (DE-He213)BF00170992-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Wolfson, C. J. verfasserin aut Soft X-ray emission from active regions shortly before solar flares 1982 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Co. 1982 Abstract Detailed examination of the variations in the intensity of soft X-ray emission prior to many solar flares are presented. In addition, these preflare intensity variations are contrasted with the variations typically observed for the same active regions in the absence of a flare. It is shown that a 5–20 min preflare brightening phase is not typically observed. These observations are discussed in context with other complimentary investigations and theoretical models. Theoretical Model Flare Active Region Intensity Variation Solar Flare Enthalten in Solar physics Kluwer Academic Publishers, 1967 76(1982), 2 vom: März, Seite 377-386 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:76 year:1982 number:2 month:03 pages:377-386 https://doi.org/10.1007/BF00170992 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 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_4082 GBV_ILN_4305 GBV_ILN_4306 AR 76 1982 2 03 377-386 |
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10.1007/BF00170992 doi (DE-627)OLC2033550567 (DE-He213)BF00170992-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Wolfson, C. J. verfasserin aut Soft X-ray emission from active regions shortly before solar flares 1982 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Co. 1982 Abstract Detailed examination of the variations in the intensity of soft X-ray emission prior to many solar flares are presented. In addition, these preflare intensity variations are contrasted with the variations typically observed for the same active regions in the absence of a flare. It is shown that a 5–20 min preflare brightening phase is not typically observed. These observations are discussed in context with other complimentary investigations and theoretical models. Theoretical Model Flare Active Region Intensity Variation Solar Flare Enthalten in Solar physics Kluwer Academic Publishers, 1967 76(1982), 2 vom: März, Seite 377-386 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:76 year:1982 number:2 month:03 pages:377-386 https://doi.org/10.1007/BF00170992 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_20 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_4082 GBV_ILN_4305 GBV_ILN_4306 AR 76 1982 2 03 377-386 |
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Abstract Detailed examination of the variations in the intensity of soft X-ray emission prior to many solar flares are presented. In addition, these preflare intensity variations are contrasted with the variations typically observed for the same active regions in the absence of a flare. It is shown that a 5–20 min preflare brightening phase is not typically observed. These observations are discussed in context with other complimentary investigations and theoretical models. © D. Reidel Publishing Co. 1982 |
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Abstract Detailed examination of the variations in the intensity of soft X-ray emission prior to many solar flares are presented. In addition, these preflare intensity variations are contrasted with the variations typically observed for the same active regions in the absence of a flare. It is shown that a 5–20 min preflare brightening phase is not typically observed. These observations are discussed in context with other complimentary investigations and theoretical models. © D. Reidel Publishing Co. 1982 |
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Abstract Detailed examination of the variations in the intensity of soft X-ray emission prior to many solar flares are presented. In addition, these preflare intensity variations are contrasted with the variations typically observed for the same active regions in the absence of a flare. It is shown that a 5–20 min preflare brightening phase is not typically observed. These observations are discussed in context with other complimentary investigations and theoretical models. © D. Reidel Publishing Co. 1982 |
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J.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Soft X-ray emission from active regions shortly before solar flares</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1982</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">© D. Reidel Publishing Co. 1982</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract Detailed examination of the variations in the intensity of soft X-ray emission prior to many solar flares are presented. In addition, these preflare intensity variations are contrasted with the variations typically observed for the same active regions in the absence of a flare. It is shown that a 5–20 min preflare brightening phase is not typically observed. 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