2-D radiative transfer simulations with angle-dependent partial frequency redistribution
被引:0
作者:
Gorshkov, AB
论文数: 0引用数: 0
h-index: 0
机构:
Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119899, RussiaMoscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119899, Russia
Gorshkov, AB
[1
]
Heinzel, P
论文数: 0引用数: 0
h-index: 0
机构:
Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119899, RussiaMoscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119899, Russia
Heinzel, P
[1
]
机构:
[1] Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119899, Russia
来源:
NEW PERSPECTIVES ON SOLAR PROMINENCES
|
1998年
/
150卷
关键词:
D O I:
暂无
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
We demonstrate how the angle-dependent redistribution function can be incorporated into the 2-D transfer modelling of solar prominences. Some preliminary numerical simulations have been performed and we present their results by comparing the emergent hydrogen L alpha line profiles computed with the angle-averaged and angle-dependent redistributions.