Emission_spectrum-H.png(757 × 100 像素,檔案大細:317字節 ,MIME類型:image/png

描述
  • Suomi: Vedyn emissioviivaspektri, joka syntyy hehkuvan vetykasun säteillessä vain tiettyjä aallonpituuksia.
English: Visible lines in the hydrogen emission spectrum
來源

Created using the Balmer formula:

Where

is the wavelength.
B is a constant with the value of 3.6456×10-7 m or 364.56 nm.
n is equal to 2
m is an integer such that m > n.
The lines are plotted horizontally and coloured to match their respective wavelengths.
作者 Merikanto
許可
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This work has been released into the public domain by its author, Merikanto, at the 英文 維基百科 project. This applies worldwide.

In case this is not legally possible:
Merikanto grants anyone the right to use this work for any purpose, without any conditions, unless such conditions are required by law.

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現時2006年5月5號 (五) 21:51響2006年5月5號 (五) 21:51嘅縮圖版本757 × 100(317字節)Hautala{{PD-user-w|fi|Finnish Wikipedia|Merikanto}} * {{fi|Vedyn emissioviivaspektri, joka syntyy hehkuvan vetykasun säteillessä vain tiettyjä aallonpituuksia.}} * {{en|Emission spectrum of hydrogen.}} Category:Physics

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