| 1. | If the spectrum is flat , the star is white in color
假若光谱曲线非常平坦，那么恒星看来便是白色的。 |
| 2. | Figure 1 erythemal action spectrum
图一红班作用光谱曲线 |
| 3. | Erythemal action spectrum
红班作用光谱曲线 |
| 4. | Erythemal action spectrum
红斑作用光谱曲线 |
| 5. | Measured uv intensity across the solar uv spectrum and the erythemal action spectrum
图二太阳紫外线光谱内所量度的紫外线强度及红斑作用光谱曲线 |
| 6. | Measured uv intensity across the solar uv spectrum and the erythemal action spectrum
图一太阳紫外线光谱内所量度的紫外线强度及红班作用光谱曲线 |
| 7. | Spectral derivative is a simple and effective method to acquire the wavelengths of extremum points
光谱微分方法是一种简单而有效的确定光谱曲线极值点波长位置的方法。 |
| 8. | Evaluating factor : this is a figure indicating the match condition between the calculated and real time measured spectral
评价函数：是评价实际镀制中光谱曲线与理论曲线吻合程度的数值。 |
| 9. | Concerning the first factor , our aim is to let the desired curve " travel through " our considered wavelength domain
对于第一个因素，我们的目标是使目标光谱曲线‘移入’所考虑的波长范围。 |
| 10. | The standard way to calculate the uv index recommended by the world meteorological organization and the world health organization is
图一红斑作用光谱曲线世界气象组织及世界卫生组织所建议的计算紫外线指数标准方法为： |
