interdinghy
- 12
- 0
Homework Statement
"The normal Zeeman effect splits a spectral line at frequency \nu_{0} and two satellite lines at \nu_{0} ± eB/(4\pi m_{e}). By what amount (in angstroms) are the satellite lines of the hydrogen Balmer \alpha line (\lambda_{0} = 6562.81 Å) split from the central component in a typical sunspot?
Given value for B in a sunspot: .1 T
Homework Equations
\lambda = c/\nu
d\lambda = c d/d\nu
The Attempt at a Solution
I've tried plugging things into eB/(4\pi m_{e}) to find the change in frequency for the satellite lines, but I'm not getting a value in hertz, so I'm not exactly sure what I'm doing wrong. I'm pretty sure that once I get an actual frequency out of this I can just use the relevant equations to find the difference in wavelength.