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Autor:
V. V. Ivanov, R. C. Mancini, N. A. Huerta, K. J. Swanson, D. E. Winget, M. H. Montgomery, I. E. Golovkin, H. K. Hariharan, Z. S. Berbel
Publikováno v:
Physical Review E. 106
The Zeeman effect is used for measurement of magnetic fields in astrophysical and laboratory plasmas. Magnetic fields in atmospheres of magnetic white dwarf stars are in the range 40 kG-1 GG. The quadratic Zeeman effect results in the additional spli
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::55ef1f1958c72a1ed4c0dbf19a68ec75
https://doi.org/10.1103/physreve.106.045206
https://doi.org/10.1103/physreve.106.045206
