Zeeman effect - significado y definición. Qué es Zeeman effect
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  3. Zeeman effect

Qué (quién) es Zeeman effect - definición


Zeeman effect         
  • 2}}).
  • This animation shows what happens as a sunspot (or starspot) forms and the magnetic field increases in strength. The light emerging from the spot starts to demonstrate the Zeeman effect. The dark spectra lines in the spectrum of the emitted light split into three components and the strength of the circular polarisation in parts of the spectrum increases significantly. This polarisation effect is a powerful tool for astronomers to detect and measure stellar magnetic fields.
  • Zeeman effect on a sunspot spectral line
EFFECT OF SPLITTING A SPECTRAL LINE INTO SEVERAL COMPONENTS IN THE PRESENCE OF A STATIC MAGNETIC FIELD
Zeeman Effect; Zeeman Splitting; Paschen–Back effect; Paschen-back effect; Paschen-Back Effect; Paschen-Bach effect; Anomalous zeeman effect; Zeeman splitting; Anomalous Zeeman Effect; Anomalous Zeeman effect; Normal zeeman effect; Paschen-Back effect; Inverse Zeeman effect; Breit-Rabi equation; Breit-Rabi formula; Breit–Rabi equation
The Zeeman effect (; ) is the effect of splitting of a spectral line into several components in the presence of a static magnetic field. It is named after the Dutch physicist Pieter Zeeman, who discovered it in 1896 and received a Nobel prize for this discovery.
https://en.wikipedia.org/wiki/Zeeman_effect
Zeeman effect         
  • 2}}).
  • This animation shows what happens as a sunspot (or starspot) forms and the magnetic field increases in strength. The light emerging from the spot starts to demonstrate the Zeeman effect. The dark spectra lines in the spectrum of the emitted light split into three components and the strength of the circular polarisation in parts of the spectrum increases significantly. This polarisation effect is a powerful tool for astronomers to detect and measure stellar magnetic fields.
  • Zeeman effect on a sunspot spectral line
EFFECT OF SPLITTING A SPECTRAL LINE INTO SEVERAL COMPONENTS IN THE PRESENCE OF A STATIC MAGNETIC FIELD
Zeeman Effect; Zeeman Splitting; Paschen–Back effect; Paschen-back effect; Paschen-Back Effect; Paschen-Bach effect; Anomalous zeeman effect; Zeeman splitting; Anomalous Zeeman Effect; Anomalous Zeeman effect; Normal zeeman effect; Paschen-Back effect; Inverse Zeeman effect; Breit-Rabi equation; Breit-Rabi formula; Breit–Rabi equation
·add. ·- The widening and duplication, triplication, ·etc., of spectral lines when the radiations emanate in a strong magnetic field, first observed in 1896 by P. Zeeman, a Dutch physicist, and regarded as an important confirmation of the electromagnetic theory of light.
Zeeman effect         
  • 2}}).
  • This animation shows what happens as a sunspot (or starspot) forms and the magnetic field increases in strength. The light emerging from the spot starts to demonstrate the Zeeman effect. The dark spectra lines in the spectrum of the emitted light split into three components and the strength of the circular polarisation in parts of the spectrum increases significantly. This polarisation effect is a powerful tool for astronomers to detect and measure stellar magnetic fields.
  • Zeeman effect on a sunspot spectral line
EFFECT OF SPLITTING A SPECTRAL LINE INTO SEVERAL COMPONENTS IN THE PRESENCE OF A STATIC MAGNETIC FIELD
Zeeman Effect; Zeeman Splitting; Paschen–Back effect; Paschen-back effect; Paschen-Back Effect; Paschen-Bach effect; Anomalous zeeman effect; Zeeman splitting; Anomalous Zeeman Effect; Anomalous Zeeman effect; Normal zeeman effect; Paschen-Back effect; Inverse Zeeman effect; Breit-Rabi equation; Breit-Rabi formula; Breit–Rabi equation
['zi:m?n, 'ze?-]
¦ noun Physics the splitting of a spectrum line into several components by a magnetic field.
Origin
C19: named after the Dutch physicist Pieter Zeeman.
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