Chapter 10: Problem 16
(a) Calculate the frequency shift produced by the normal Zeeman effect in the center of a sunspot that has a magnetic field strength of \(0.3 \mathrm{T}\) (b) By what fraction would the wavelength of one component of the 630.25 -nm Fe I spectral line change as a consequence of a magnetic field of \(0.3 \mathrm{T} ?\)
Short Answer
Step by step solution
Understanding the Zeeman Effect
Calculate the Frequency Shift
Convert Frequency Shift to Wavelength Change
Calculate Fractional Wavelength Change
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Key Concepts
These are the key concepts you need to understand to accurately answer the question.
Understanding Frequency Shift
The formula governing this shift is \[ \Delta f = \dfrac{e B}{4 \pi m} \]where:
- \(e\) is the electron charge, approximately \(1.6 \times 10^{-19} \ \text{C}\).
- \(B\) is the magnetic field strength.
- \(m\) is the mass of the electron, about \(9.11 \times 10^{-31} \ \text{kg}\).
Magnetic Field Strength's Role
In an exercise involving an iron spectral line in a sunspot, for instance:
- The magnetic field strength \(B = 0.3 \ \text{T}\) impacts how much the energy levels split.
- Greater magnetic field strength results in a more significant shift in frequency, readily detectable via spectral line analysis.
Understanding Spectral Line Splitting
The splitting results in:
- Multiple distinct lines observable within a spectrometer.
- The number and spacing of the lines depend on the orientation of the magnetic field relative to the observer.
Significance of Wavelength Change
For example, using the relation \[ \Delta \lambda = \dfrac{c \cdot \Delta f}{f^2}, \]we can calculate a wavelength shift from a known frequency change. With:
- \(c\) as the speed of light, \(3 \times 10^{8} \ \text{m/s}\)
- \(\Delta \lambda\) representing the wavelength alteration