Calculating Satellite Line Splitting in a Sunspot using the Zeeman Effect

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Homework Help Overview

The discussion revolves around calculating the splitting of satellite lines in the hydrogen Balmer alpha line due to the normal Zeeman effect, specifically in the context of sunspots. The original poster presents a problem involving the frequency and wavelength changes resulting from a magnetic field in a sunspot.

Discussion Character

  • Exploratory, Assumption checking, Mathematical reasoning

Approaches and Questions Raised

  • Participants discuss the calculation of frequency changes and their conversion to wavelength differences. The original poster attempts to compute the frequency shift but encounters issues with unit compatibility. Others suggest checking the units of various components involved in the calculations.

Discussion Status

The discussion is ongoing, with participants exploring different aspects of the calculations and clarifying unit conversions. Some guidance has been offered regarding unit analysis, and the original poster has made progress in understanding the role of the electron charge in the calculations.

Contextual Notes

Participants are working within the constraints of the problem statement and the specific values provided for the magnetic field and the wavelength of the hydrogen Balmer alpha line. There is an emphasis on ensuring that units are compatible throughout the calculations.

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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.
 
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Did you calculate the individual wavelengths and take their difference? or did you calculate the difference in frequency and calculate a wavelength with that?
 
If I calculate the frequency based off the given wavelength, I get 4.56*10^14 hertz, but that doesn't get me any further I don't think.

The problem is the difference between the initial frequency and the satellite lines. I can't add or subtract the difference because the difference isn't a frequency, it's some nonsense units (seconds^-2 ampere^-1).
 
Try writing out the units of each piece in the SI base units. See what happens.
 
frogjg2003 said:
Try writing out the units of each piece in the SI base units. See what happens.

I think this is maybe where I'm missing something?

A tesla divided by an electron mass is giving me 1 per second per ampere, and wolfram seems to agree with this.

\nu_{0} + s^{-1}A^{-1} = Hz + s^{-1}A^{-1} is adding incompatible units, so I'm pretty sure I can't do it.
 
What about the electron charge?
 
Also, I'm getting per second squared in Wolfram.
 
Oh okay I see now. I was so sure e was the base of the natural log. I actually tried looking around for other things it could stand for, but putting it in as the electron charge on wolfram made it work.

Thanks!
 

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