Nonuniform target ionization and fitting thick target electron injection spectra to RHESSI data

被引:47
作者
Kontar, EP [1 ]
Brown, JC
McArthur, GK
机构
[1] Univ Glasgow, Dept Phys & Astron, Astron & Astrophys Grp, Glasgow G12 8QQ, Lanark, Scotland
[2] Catholic Univ Amer, Goddard Space Flight Ctr, Washington, DC 20064 USA
关键词
D O I
10.1023/A:1022494318540
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Past analyses of flare hard X-ray (HXR) spectra have largely ignored the effect of nonuniform ionization along the electron paths in the thick-target model, though it is very significant for well-resolved spectra. The inverse problem (photon spectrum to electron injection spectrum F-o(E-o)) is disturbingly non-unique. However, we show that it is relatively simple to allow for the effect in forward fitting of parametric models of F-o (E-0) and provide an expression to evaluate it for the usual single power-law form of F-o(E-o). The expression involves the column depth N* of the transition region in the flare loop as one of the parameters so data fitting can enable derivation of N* (and its evaporative evolution) as part of the fitting procedure. The fit to RHESSI data on four flares for a single power law F-o(E-o) is much improved when ionization structure is included compared to when the usual fully ionized approximation is used. This removes the need, in these events at least, to invoke broken power laws, or other forms, of the acceleration spectrum F-o(E-o) to explain the observed photon spectrum.
引用
收藏
页码:419 / 429
页数:11
相关论文
共 11 条
[1]  
ASCHWANDEN MJ, 2002, IN PRESS SPACE SCI R
[2]  
BROWN JC, 1973, SOL PHYS, V31, P143, DOI 10.1007/BF00156080
[4]   THICK TARGET X-RAY BREMSSTRAHLUNG FROM PARTIALLY IONIZED TARGETS IN SOLAR-FLARES [J].
BROWN, JC .
SOLAR PHYSICS, 1973, 28 (01) :151-158
[5]   Inversion of thick-target bremsstrahlung spectra from nonuniformly ionised plasmas [J].
Brown, JC ;
McArthur, GK ;
Barrett, RK ;
McIntosh, SW ;
Emslie, AG .
SOLAR PHYSICS, 1998, 179 (02) :379-404
[6]   ANALYTIC LIMITS ON THE FORMS OF SPECTRA POSSIBLE FROM OPTICALLY THIN COLLISIONAL BREMSSTRAHLUNG SOURCE MODELS [J].
BROWN, JC ;
EMSLIE, AG .
ASTROPHYSICAL JOURNAL, 1988, 331 (01) :554-564
[7]  
CRAIG IJD, 1986, INVERSE PROBLEMS AST
[8]   An empirical method to determine electron energy modification rates from spatially resolved hard X-ray data [J].
Emslie, AG ;
Barrett, RK ;
Brown, JC .
ASTROPHYSICAL JOURNAL, 2001, 557 (02) :921-929
[9]   2 ACCELERATED ELECTRON POPULATIONS IN THE 1980 JUNE 27 SOLAR-FLARE [J].
LIN, RP ;
JOHNS, CM .
ASTROPHYSICAL JOURNAL, 1993, 417 (01) :L53-L56
[10]  
MCARTHUR GK, 2000, THESIS U GLASGOW