英文の和訳を教えてください
以下の文なのですが、訳せる方いらっしゃいましたらお願いします。
Stars, including our own sun, emit energies covering a range of wavelengths of the EM spectrum.
However, different types of stars produce differing amounts of energy in each region of the spectrum.
Our sun emits more photons in the visible light and surrounding regions than in any other part of the EM spectrum.
This phenomenon may be why our eyes have evolved to see that part of the EM spectrum and not microwaves, gamma rays, or any of the other wavelengths that are emitted at lower intensities by our sun.
Figure 9 includes a spectrum of the sun’s light that reaches Earth’s upper atmosphere.
Notice the peak region is from 400 to 700 nanometers (nm), which is the visible range of the spectrum.
Also note that there is a large number of photons through most of the infrared region of the spectrum (700 to 10,000 nm). At the higher-energy, shorter-wavelength end of the spectrum, the number of photons drops off dramatically.
The sun’s spectrum contains very little light with wavelengths shorter than about 300 nm (i.e., photon energy greater than about 4 eV).
The Earth’s atmosphere protects us from the higher-energy forms of light, such as ultraviolet rays. In fact, the existence of life on Earth would be far less likely if these more damaging forms of energy were more abundant.
The terrestrial spectrum in Fig. 9 describes the light that actually reaches the Earth’s surface after passing through the atmosphere.
Notice that there are various wavelengths in which the number of photons is greatly reduced as compared to the space solar spectrum.
This difference is due to photons being absorbed by atmospheric gases, the best known being ozone (O3), which absorbs higher-energy (lower-wavelength) ultraviolet light below 400 nm.
Photons with wavelengths near 900, 1100, and 1400 nm are absorbed by water vapor in the atmosphere.
以上です。自分でできれば良いのですが・・・
お礼
ご丁寧にありがとうございます。 大変助かりました！