Artículo
Machado, M.E.; Mandrini, C.H. "Use of RHESSI observations to determine the origin and fate of non-thermal flare electrons" (2004) Advances in Space Research. 34(2):451-455
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Abstract:
Most analyses of the characteristics of hard X-ray emission from solar flares have relied on observations of the spectral, temporal and spatial intensity distribution obtained by different instruments and, in the majority of cases, different events. The Reuven Ramaty High Energy Spectroscopic Imager gives us the possibility of combining all three fundamental parameters in a single set of observations from the same instrument. In this paper, we describe a method to compute the distribution of hard X-ray emission in flare loops, which can be used to determine the characteristics of electron energization, transport and thermalization during short lived impulsive peaks. © 2004 COSPAR. Published by Elsevier Ltd. All rights reserved.
Registro:
| Documento: | Artículo |
| Título: | Use of RHESSI observations to determine the origin and fate of non-thermal flare electrons |
| Autor: | Machado, M.E.; Mandrini, C.H. |
| Filiación: | Com Natl de Actividades Espaciales, Paseo Colón 751, Buenos Aires C1063ACH, Argentina Inst. de Astron./Fisica del Espacio, IAFE, Buenos Aires 1428, Argentina |
| Palabras clave: | Hard X-rays; Particle acceleration; Solar flares; Electron emission; Image processing; Spectroscopic analysis; X rays; Electron energization; Flare loops; Thermalization; X-ray emission; Space research; solar activity |
| Año: | 2004 |
| Volumen: | 34 |
| Número: | 2 |
| Página de inicio: | 451 |
| Página de fin: | 455 |
| DOI: | http://dx.doi.org/10.1016/j.asr.2004.01.007 |
| Título revista: | Advances in Space Research |
| Título revista abreviado: | Adv. Space Res. |
| ISSN: | 02731177 |
| CODEN: | ASRSD |
| Registro: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_02731177_v34_n2_p451_Machado |
Referencias:
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Citas:
---------- APA ----------
Machado, M.E. & Mandrini, C.H. (2004) . Use of RHESSI observations to determine the origin and fate of non-thermal flare electrons. Advances in Space Research, 34(2), 451-455.http://dx.doi.org/10.1016/j.asr.2004.01.007
---------- CHICAGO ----------
Machado, M.E., Mandrini, C.H. "Use of RHESSI observations to determine the origin and fate of non-thermal flare electrons" . Advances in Space Research 34, no. 2 (2004) : 451-455.http://dx.doi.org/10.1016/j.asr.2004.01.007
---------- MLA ----------
Machado, M.E., Mandrini, C.H. "Use of RHESSI observations to determine the origin and fate of non-thermal flare electrons" . Advances in Space Research, vol. 34, no. 2, 2004, pp. 451-455.http://dx.doi.org/10.1016/j.asr.2004.01.007
---------- VANCOUVER ----------
Machado, M.E., Mandrini, C.H. Use of RHESSI observations to determine the origin and fate of non-thermal flare electrons. Adv. Space Res. 2004;34(2):451-455.http://dx.doi.org/10.1016/j.asr.2004.01.007
