Large-scale brightenings associated with flares
Flare-associated large-scale (>1010 cm) X-ray brightenings, the so-called 'giant arches' in the nomenclature of Švestka and co-workers, were discovered in images obtained by the SMM Hard X-ray Imaging Spectrometer hours after the onset of two-ribbon flares. The apparent correlation...
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Kluwer Academic Publishers
1992
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| Acceso en línea: | Registro en Scopus DOI Handle Registro en la Biblioteca Digital |
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| LEADER | 06971caa a22007697a 4500 | ||
|---|---|---|---|
| 001 | PAPER-19230 | ||
| 003 | AR-BaUEN | ||
| 005 | 20250618102919.0 | ||
| 008 | 190411s1992 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-0010230518 | |
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 100 | 1 | |a Mandrini, Cristina Hemilse | |
| 245 | 1 | 0 | |a Large-scale brightenings associated with flares |
| 260 | |b Kluwer Academic Publishers |c 1992 | ||
| 270 | 1 | 0 | |m Mandrini, C.H.; Instituto de Astronomía y Física del Espacio, CC 67, Suc 28, Buenos Aires, 1428, Argentina |
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| 504 | |a Wu, S. T., de Jager, C., Dennis, B. R., Hudson, H. S., Simnett, G. M., Strong, K. T. et al.: 1986, in M. Kundu and B. Woodgate (eds.), Energetic Phenomena on the Sun, NASA CP-2439, Ch. 5 | ||
| 506 | |2 openaire |e Política editorial | ||
| 520 | 3 | |a Flare-associated large-scale (>1010 cm) X-ray brightenings, the so-called 'giant arches' in the nomenclature of Švestka and co-workers, were discovered in images obtained by the SMM Hard X-ray Imaging Spectrometer hours after the onset of two-ribbon flares. The apparent correlation between both phenomena suggested that they could be interpreted in the framework of the same model. In this paper we show that large-scale loop brightenings, of sizes similar to the giant arches, occur also in association with confined flares in complex active regions. In these cases, the relation between the large-scale structure and the underlying flare is clearly given by the magnetic field topology. We also show that energization of these structures can be partially due to the injection of suprathermal particles that are accelerated at the separator region. We discuss the implications of these results within the framework of the interacting loops picture of flares and of the giant arch phenomenology. © 1992 Kluwer Academic Publishers. |l eng | |
| 593 | |a Instituto de Astronomía y Física del Espacio, CC 67, Suc 28, Buenos Aires, 1428, Argentina | ||
| 593 | |a Department of Physics, The University of Alabama in Huntsville, Huntsville, 35899, AL, United States | ||
| 700 | 1 | |a Machado, M.E. | |
| 773 | 0 | |d Kluwer Academic Publishers, 1992 |g v. 141 |h pp. 147-164 |k n. 1 |p Sol Phys |x 00380938 |w (AR-BaUEN)CENRE-2238 |t Solar Physics | |
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| 856 | 4 | 0 | |u https://doi.org/10.1007/BF00155909 |y DOI |
| 856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_00380938_v141_n1_p147_Mandrini |y Handle |
| 856 | 4 | 0 | |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00380938_v141_n1_p147_Mandrini |y Registro en la Biblioteca Digital |
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