|
Determination of the acceleration region size in a loop-structured solar flare
|
|
Jingnan Guo Submitted: 2012-06-03 11:26
In order to study the acceleration and propagation of bremsstrahlung-producing electrons in solar flares, we analyze the evolution of the flare loop size with respect to energy at a variety of times. A GOES M3.7 loop-structured flare starting around 23:55 on 2002 April 14 is studied in detail using Ramaty High Energy Solar Spectroscopic Imager (RHESSI) observations. We construct photon and mean-electron-flux maps in 2-keV energy bins by processing observationally-deduced photon and electron visibilities, respectively, through several image-processing methods: a visibility-based forward-fit (FWD) algorithm, a maximum entropy (MEM) procedure and the uv-smooth (UVS) approach. We estimate the sizes of elongated
ares (i.e., the length and width of flaring loops) by calculating the second normalized moments of the intensity in any given map. Employing a collisional model with an extended acceleration region, we fit the loop lengths as a function of energy in both the photon and electron domains.
The consistency of the estimates from these methods provides strong support that the model can reliably
determine geometric parameters of the acceleration region. The acceleration region is estimated to be a substantial
fraction (~ 1/2) of the loop extent, indicating that this dense flaring loop incorporates both acceleration and transport of electrons, with concurrent thick-target bremsstrahlung emission.
Authors: Jingnan Guo, A. Gordon Emslie, Eduard P. Kontar, Federico Benvenuto, Anna Maria Massone, Michele Piana
Projects: RHESSI
|
Publication Status: Accepted by A&A
Last Modified: 2012-06-08 07:28
|
 
 
 
 
|
|