“星系中的射电辐射”的版本间差异

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无编辑摘要
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星系中的射电辐射主要有三种
星系中的射电辐射主要有三种


#同步辐射 (低频,幂律谱)
*同步辐射 (低频,幂律谱)
#自由-自由散射 (HII区:低频是接近于热谱,光学厚,高频光学薄,平谱)
*自由-自由散射 (HII区:低频是接近于热谱,光学厚,高频光学薄,平谱)
:https://www.cv.nrao.edu/course/astr534/FreeFreeEmission.html
:https://www.cv.nrao.edu/course/astr534/FreeFreeEmission.html
#AME
*AME
:Anomalous Microwave Emission (AME) is a component of diffuse Galactic radiation observed at frequencies in the range ≈ 10–60 GHz. AME was first detected in 1996 and recognised as an additional component of emission in 1997
:Anomalous Microwave Emission (AME) is a component of diffuse Galactic radiation observed at frequencies in the range ≈ 10–60 GHz. AME was first detected in 1996 and recognised as an additional component of emission in 1997

2018年11月15日 (四) 05:58的版本

星系中的射电辐射主要有三种

  • 同步辐射 (低频,幂律谱)
  • 自由-自由散射 (HII区:低频是接近于热谱,光学厚,高频光学薄,平谱)
https://www.cv.nrao.edu/course/astr534/FreeFreeEmission.html
  • AME
Anomalous Microwave Emission (AME) is a component of diffuse Galactic radiation observed at frequencies in the range ≈ 10–60 GHz. AME was first detected in 1996 and recognised as an additional component of emission in 1997