Evidence for interacting loop process in a phase of the May 16, 1981 flare

Abstract The behaviour of the flare in the period of enhancement and maximum of hard X-ray, microwave and decimetric type IV continuum is analysed. The elongation of the Hα ribbons and microwave source disclose that the energy release site was shifting through a system of loops with a velocity less...
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Autor*in:	Vršnak, B. [verfasserIn] Ruždjak, V. Messerotti, M. Zlobec, P.

Format:	Artikel
Sprache:	Englisch

Erschienen:	1987

Schlagwörter:	Microwave Thermal Conduction Flare Energy Release Field Line

Anmerkung:	© D. Reidel Publishing Company 1987

Übergeordnetes Werk:	Enthalten in: Solar physics - Kluwer Academic Publishers, 1967, 111(1987), 1 vom: März, Seite 23-29
Übergeordnetes Werk:	volume:111 ; year:1987 ; number:1 ; month:03 ; pages:23-29

Links:	Volltext

DOI / URN:	10.1007/BF00145437

Katalog-ID:	OLC2033562107

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allfields	10.1007/BF00145437 doi (DE-627)OLC2033562107 (DE-He213)BF00145437-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Vršnak, B. verfasserin aut Evidence for interacting loop process in a phase of the May 16, 1981 flare 1987 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1987 Abstract The behaviour of the flare in the period of enhancement and maximum of hard X-ray, microwave and decimetric type IV continuum is analysed. The elongation of the Hα ribbons and microwave source disclose that the energy release site was shifting through a system of loops with a velocity less than 200 km $ s^{-1} $, and that the energy was carried down the field lines with a velocity of about 1000 km $ s^{-1} $, implying the thermal conduction front mechanism of energy transport. Several processes of energy release are considered and it is concluded that an explanation in terms of succeeding interactions of neighbouring loops, involving fast reconnection of their poloidal components is in best agreement with the observations. Microwave Thermal Conduction Flare Energy Release Field Line Ruždjak, V. aut Messerotti, M. aut Zlobec, P. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 111(1987), 1 vom: März, Seite 23-29 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:111 year:1987 number:1 month:03 pages:23-29 https://doi.org/10.1007/BF00145437 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_4046 GBV_ILN_4306 AR 111 1987 1 03 23-29
spelling	10.1007/BF00145437 doi (DE-627)OLC2033562107 (DE-He213)BF00145437-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Vršnak, B. verfasserin aut Evidence for interacting loop process in a phase of the May 16, 1981 flare 1987 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1987 Abstract The behaviour of the flare in the period of enhancement and maximum of hard X-ray, microwave and decimetric type IV continuum is analysed. The elongation of the Hα ribbons and microwave source disclose that the energy release site was shifting through a system of loops with a velocity less than 200 km $ s^{-1} $, and that the energy was carried down the field lines with a velocity of about 1000 km $ s^{-1} $, implying the thermal conduction front mechanism of energy transport. Several processes of energy release are considered and it is concluded that an explanation in terms of succeeding interactions of neighbouring loops, involving fast reconnection of their poloidal components is in best agreement with the observations. Microwave Thermal Conduction Flare Energy Release Field Line Ruždjak, V. aut Messerotti, M. aut Zlobec, P. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 111(1987), 1 vom: März, Seite 23-29 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:111 year:1987 number:1 month:03 pages:23-29 https://doi.org/10.1007/BF00145437 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_4046 GBV_ILN_4306 AR 111 1987 1 03 23-29
allfields_unstemmed	10.1007/BF00145437 doi (DE-627)OLC2033562107 (DE-He213)BF00145437-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Vršnak, B. verfasserin aut Evidence for interacting loop process in a phase of the May 16, 1981 flare 1987 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1987 Abstract The behaviour of the flare in the period of enhancement and maximum of hard X-ray, microwave and decimetric type IV continuum is analysed. The elongation of the Hα ribbons and microwave source disclose that the energy release site was shifting through a system of loops with a velocity less than 200 km $ s^{-1} $, and that the energy was carried down the field lines with a velocity of about 1000 km $ s^{-1} $, implying the thermal conduction front mechanism of energy transport. Several processes of energy release are considered and it is concluded that an explanation in terms of succeeding interactions of neighbouring loops, involving fast reconnection of their poloidal components is in best agreement with the observations. Microwave Thermal Conduction Flare Energy Release Field Line Ruždjak, V. aut Messerotti, M. aut Zlobec, P. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 111(1987), 1 vom: März, Seite 23-29 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:111 year:1987 number:1 month:03 pages:23-29 https://doi.org/10.1007/BF00145437 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_4046 GBV_ILN_4306 AR 111 1987 1 03 23-29
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allfieldsSound	10.1007/BF00145437 doi (DE-627)OLC2033562107 (DE-He213)BF00145437-p DE-627 ger DE-627 rakwb eng 530 VZ 16,12 ssgn Vršnak, B. verfasserin aut Evidence for interacting loop process in a phase of the May 16, 1981 flare 1987 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1987 Abstract The behaviour of the flare in the period of enhancement and maximum of hard X-ray, microwave and decimetric type IV continuum is analysed. The elongation of the Hα ribbons and microwave source disclose that the energy release site was shifting through a system of loops with a velocity less than 200 km $ s^{-1} $, and that the energy was carried down the field lines with a velocity of about 1000 km $ s^{-1} $, implying the thermal conduction front mechanism of energy transport. Several processes of energy release are considered and it is concluded that an explanation in terms of succeeding interactions of neighbouring loops, involving fast reconnection of their poloidal components is in best agreement with the observations. Microwave Thermal Conduction Flare Energy Release Field Line Ruždjak, V. aut Messerotti, M. aut Zlobec, P. aut Enthalten in Solar physics Kluwer Academic Publishers, 1967 111(1987), 1 vom: März, Seite 23-29 (DE-627)129856010 (DE-600)281593-X (DE-576)015160033 0038-0938 nnns volume:111 year:1987 number:1 month:03 pages:23-29 https://doi.org/10.1007/BF00145437 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_4046 GBV_ILN_4306 AR 111 1987 1 03 23-29
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title_sort	evidence for interacting loop process in a phase of the may 16, 1981 flare
title_auth	Evidence for interacting loop process in a phase of the May 16, 1981 flare
abstract	Abstract The behaviour of the flare in the period of enhancement and maximum of hard X-ray, microwave and decimetric type IV continuum is analysed. The elongation of the Hα ribbons and microwave source disclose that the energy release site was shifting through a system of loops with a velocity less than 200 km $ s^{-1} $, and that the energy was carried down the field lines with a velocity of about 1000 km $ s^{-1} $, implying the thermal conduction front mechanism of energy transport. Several processes of energy release are considered and it is concluded that an explanation in terms of succeeding interactions of neighbouring loops, involving fast reconnection of their poloidal components is in best agreement with the observations. © D. Reidel Publishing Company 1987
abstractGer	Abstract The behaviour of the flare in the period of enhancement and maximum of hard X-ray, microwave and decimetric type IV continuum is analysed. The elongation of the Hα ribbons and microwave source disclose that the energy release site was shifting through a system of loops with a velocity less than 200 km $ s^{-1} $, and that the energy was carried down the field lines with a velocity of about 1000 km $ s^{-1} $, implying the thermal conduction front mechanism of energy transport. Several processes of energy release are considered and it is concluded that an explanation in terms of succeeding interactions of neighbouring loops, involving fast reconnection of their poloidal components is in best agreement with the observations. © D. Reidel Publishing Company 1987
abstract_unstemmed	Abstract The behaviour of the flare in the period of enhancement and maximum of hard X-ray, microwave and decimetric type IV continuum is analysed. The elongation of the Hα ribbons and microwave source disclose that the energy release site was shifting through a system of loops with a velocity less than 200 km $ s^{-1} $, and that the energy was carried down the field lines with a velocity of about 1000 km $ s^{-1} $, implying the thermal conduction front mechanism of energy transport. Several processes of energy release are considered and it is concluded that an explanation in terms of succeeding interactions of neighbouring loops, involving fast reconnection of their poloidal components is in best agreement with the observations. © D. Reidel Publishing Company 1987
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up_date	2024-07-03T17:28:53.027Z
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Reidel Publishing Company 1987</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract The behaviour of the flare in the period of enhancement and maximum of hard X-ray, microwave and decimetric type IV continuum is analysed. The elongation of the Hα ribbons and microwave source disclose that the energy release site was shifting through a system of loops with a velocity less than 200 km $ s^{-1} $, and that the energy was carried down the field lines with a velocity of about 1000 km $ s^{-1} $, implying the thermal conduction front mechanism of energy transport. Several processes of energy release are considered and it is concluded that an explanation in terms of succeeding interactions of neighbouring loops, involving fast reconnection of their poloidal components is in best agreement with the observations.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Microwave</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Thermal Conduction</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Flare</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Energy Release</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Field Line</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ruždjak, V.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Messerotti, M.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Zlobec, P.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Solar physics</subfield><subfield code="d">Kluwer Academic Publishers, 1967</subfield><subfield code="g">111(1987), 1 vom: März, Seite 23-29</subfield><subfield code="w">(DE-627)129856010</subfield><subfield code="w">(DE-600)281593-X</subfield><subfield code="w">(DE-576)015160033</subfield><subfield code="x">0038-0938</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:111</subfield><subfield code="g">year:1987</subfield><subfield code="g">number:1</subfield><subfield code="g">month:03</subfield><subfield code="g">pages:23-29</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1007/BF00145437</subfield><subfield code="z">lizenzpflichtig</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_11</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_22</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_47</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2002</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2279</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2286</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4012</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4046</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4306</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">111</subfield><subfield code="j">1987</subfield><subfield code="e">1</subfield><subfield code="c">03</subfield><subfield code="h">23-29</subfield></datafield></record></collection>
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Evidence for interacting loop process in a phase of the May 16, 1981 flare

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