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Emission_spectrum-H.png (757 × 100 piksel, fayl hajmi: 317 bayt, MIME tipi: image/png)

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

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.
Muallif Merikanto
Ruxsat
(Bu faylning takror foydalanilishi)
This work has been released into the public domain by its author, Merikanto, at the inglizcha Vikipediya 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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Faylning biror paytdagi holatini koʻrish uchun tegishli sana/vaqtga bosingiz.

Sana/VaqtMiniaturaOʻlchamlariFoydalanuvchiIzoh
joriy22:51, 2006-yil 5-may22:51, 2006-yil 5-may dagi versiya uchun tasvir757 × 100 (317 bayt)wikimediacommons>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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