Electron acceleration and transport during the November 5, 1998 solar flare at ∼13:34 UT
| dc.contributor.author | Trottet G. | |
| dc.contributor.author | Correia E. | |
| dc.contributor.author | Karlicky M. | |
| dc.contributor.author | Aulanier G. | |
| dc.contributor.author | Yan Y. | |
| dc.contributor.author | Kaufmann P. | |
| dc.date.accessioned | 2024-03-13T01:42:24Z | |
| dc.date.available | 2024-03-13T01:42:24Z | |
| dc.date.issued | 2006 | |
| dc.description.abstract | This paper deals with a detailed analysis of spectral and imaging observations of the November 5, 1998 (Hα 1B, GOES M1.5) flare obtained over a large spectral range, i.e., from hard X-rays to radiometric wavelengths. These observations allowed us to probe electron acceleration and transport over a large range of altitudes that is to say within small-scale (a few 10 3 km) and large-scale (a few 105 km) magnetic structures. The observations combined with potential and linear force-free magnetic field extrapolations allow us to show that: (i) Flare energy release and electron acceleration are basically driven by loop-loop interactions at two independent, low lying, null points of the active region magnetic field; (ii) <300 keV hard X-ray-producing electrons are accelerated by a different process (probably DC field acceleration) than relativistic electrons that radiate the microwave emission; and (iii) although there is evidence that hard X-ray and decimetric/metric radio-emitting electrons are produced by the same accelerator, the present observations and analysis did not allow us to find a clear and direct magnetic connection between the hard X-ray emitting region and the radio-emitting sources in the middle corona. © Springer 2006. | |
| dc.description.firstpage | 75 | |
| dc.description.issuenumber | 1 | |
| dc.description.lastpage | 95 | |
| dc.description.volume | 236 | |
| dc.identifier.doi | 10.1007/s11207-006-0089-2 | |
| dc.identifier.issn | 0038-0938 | |
| dc.identifier.uri | https://dspace.mackenzie.br/handle/10899/37784 | |
| dc.relation.ispartof | Solar Physics | |
| dc.rights | Acesso Restrito | |
| dc.title | Electron acceleration and transport during the November 5, 1998 solar flare at ∼13:34 UT | |
| dc.type | Artigo | |
| local.scopus.citations | 5 | |
| local.scopus.eid | 2-s2.0-33746037546 | |
| local.scopus.updated | 2024-05-01 | |
| local.scopus.url | https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=33746037546&origin=inward |