%0 Journal Article
%@holdercode {isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S}
%@nexthigherunit 8JMKD3MGPCW/3ETR8EH
%@archivingpolicy denypublisher denyfinaldraft12
%@resumeid
%@resumeid 8JMKD3MGP5W/3C9JH2C
%@usergroup administrator
%@usergroup simone
%3 Electron acceleration and transport.pdf
%@dissemination WEBSCI; PORTALCAPES.
%D 2006
%2 sid.inpe.br/mtc-m16@80/2006/08.03.14.12.52
%4 sid.inpe.br/mtc-m16@80/2006/08.03.14.12
%X This paper deals with a detailed analysis of spectral and imaging observations of the November 5, 1998 (H alpha 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 10(5) 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.
%8 June
%N 1
%T Electron acceleration and transport during the November 5, 1998 solar flare at similar to 13 : 34 UT
%@secondarytype PRE PI
%K HARD X-RAY, RECONNECTING CURRENT SHEETS, DOUBLE-LOOP CONFIGURATION, GAMMA-RAY, MAGNETIC-FIELD, GYROSYNCHROTRON RADIATION, TIME STRUCTURES, MICROWAVE, RADIO, MILLIMETER.
%@group
%@group DAS-INPE-MCT-BR
%@secondarykey INPE-13952--PRE/9128
%@copyholder SID/SCD
%@issn 0038-0938
%@issn 1573-093X
%@affiliation Observatoire de Paris, Section de Meudon,
%@affiliation Instituto Nacional de Pesquisas Espaciais, Divisão de Astrofísica (INPE.DAS),
%@affiliation Observatoire de Paris, Section de Meudon,
%@affiliation National Astronomical Observatories, Chinese Academy of Sciences,
%@affiliation CRAAM, Universidade Presbiteriana Mackenzie,
%B Solar Physics
%P 75-95
%V 236
%A Trottet, G.,
%A Correia, Emilia,
%A Aulanier, G.,
%A Yan, Y.,
%A Kaufmann, P.,
%@area CEA