K. Wood et J. Raymond, Resonant scattering of emission lines in coronal loops: Effects on image morphology and line ratios, ASTROPHYS J, 540(1), 2000, pp. 563-571
We have investigated the effects of resonant scattering of emission lines o
n the image morphology and intensity from coronal loop structures. It has p
reviously been shown that line-of-sight effects in optically thin line emis
sion can yield loop images that appear uniformly bright at one viewing angl
e but show "looptop sources" at other viewing angles. For optically thick l
oops where multiple resonant scattering is important, we use a three-dimens
ional Monte Carlo radiation transfer code. Our simulations show that the in
tensity variation across the image is more uniform than the optically thin
simulation, and depending on viewing angle the intensity may be lower or hi
gher than that predicted from optically thin simulations due to scattering
out of or into the line of sight.