摘要
通过建立吸积盘Eddington近似下的辐射转移方程,局域能量守恒方程以及流体静力学平衡方程,对轴向求解温度分布,发现由于大气中粘滞能量耗散,吸积盘上有冕形成。
By equations of radiative trasfer in Eddington approximation,local energy conservation and hydrostatic established,the temperature distribution in vertical direction is studied. It is found that a corona forms above disc.
出处
《湖北大学学报(自然科学版)》
CAS
1992年第3期213-217,共5页
Journal of Hubei University:Natural Science
关键词
吸积盘
温度分层
冕
辐射转移
Accretion disc Temperature Distribution Radiatice trasfer Corona