Depicted on the right is the additional Zeeman splitting, which occurs in the presence of magnetic fields.
2.
The Zeeman splitting is caused by the fact that individual atoms are magnetized due to the circulating motion of electrons bound to them.
3.
If Zeeman splitting is included, each Landau level splits into a pair, one for spin up electrons and the other for spin down electrons.
4.
Zeeman splitting has a significant effect on the Landau levels because their energy scales are the same, "'? " } }.
5.
On June 25, 1908, Hale would record Zeeman splitting in the spectrum of a sunspot, showing for the first time that magnetic fields existed somewhere besides the earth.
6.
Zeeman splitting has been detected in five hydroxyl megamasers, and the typical strength of a detected field is of order a few milligauss, similar to the field strengths measured in galactic hydroxyl masers.
7.
In the presence of a magnetic field, the levels with different values of magnetic spin quantum number ( M S = 0, ? ) are separated and the Zeeman splitting dictates their separation.
8.
Zeeman splitting of hydroxyl megamaser lines may be used to measure magnetic fields in the masing regions, and this application represents the first detection of Zeeman splitting in a galaxy other than the Milky Way.
9.
Zeeman splitting of hydroxyl megamaser lines may be used to measure magnetic fields in the masing regions, and this application represents the first detection of Zeeman splitting in a galaxy other than the Milky Way.
10.
By the Stark effect and Zeeman splitting, the base absorption lines may be " split " into finer lines . " Stark and Zeeman tuning . . . can be used to tune the detector ."
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