A model for hard X-ray emission from the top of flaring loops

Citation
L. Fletcher et Pch. Martens, A model for hard X-ray emission from the top of flaring loops, ASTROPHYS J, 505(1), 1998, pp. 418-431
Citations number
37
Categorie Soggetti
Space Sciences
Journal title
ASTROPHYSICAL JOURNAL
ISSN journal
0004637X → ACNP
Volume
505
Issue
1
Year of publication
1998
Part
1
Pages
418 - 431
Database
ISI
SICI code
0004-637X(19980920)505:1<418:AMFHXE>2.0.ZU;2-7
Abstract
The frequent occurrence of hard X-ray emission from the top of flaring loop s was one of the discoveries by the Hard X-Ray Telescope on board the Japan ese Yohkoh satellite. In this paper we take a hare current-sheet geometry a nd show how the combined effect of magnetic field convergence and pitch-ang le scattering of nonthermal electrons injected at the top of the loop resul ts in the generation of a looptop source with properties akin to those obse rved by Yohkoh. We demonstrate that a looptop source can be produced in bot h impulsive and gradual phase loops. We further present a possible mechanis m for the generation of high-temperature "ridges" in the loop legs.