Doppler broadening
Phenomenon in physics
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Doppler broadening
Summary
Doppler broadening ranks in the top 2% of general entities by monthly Wikipedia readership (147 views/month).[1]
Key Facts
- Christian Doppler is named after Doppler broadening[2].
- Doppler broadening's GND ID is recorded as 4209216-4[3].
- Doppler broadening's subclass of is recorded as spectral broadening[4].
- Doppler broadening's Freebase ID is recorded as /m/06_3sq[5].
- Doppler broadening's defining formula is recorded as \Delta f_{\text{FWHM}} = \sqrt{\frac{8kT\ln 2}{mc^2}}f_{0}[6].
- Doppler broadening's defining formula is recorded as \sigma_{f} = \sqrt{\frac{kT}{mc^2}}f_0[7].
- Doppler broadening's IUPAC Gold Book ID is recorded as D01835[8].
- Doppler broadening's maintained by WikiProject is recorded as WikiProject Mathematics[9].
- Doppler broadening's Microsoft Academic ID is recorded as 62103226[10].
- Doppler broadening's OpenAlex ID is recorded as C62103226[11].
- Doppler broadening's Encyclopedia of China is recorded as 147048[12].
Why It Matters
Doppler broadening ranks in the top 2% of general entities by monthly Wikipedia readership (147 views/month).[1] It has Wikipedia articles in 15 language editions, a strong signal of global cultural recognition.[13] It is known by 3 alternative names across languages and contexts.[14]