Abstract
The Zeeman effect on lines in the (0, 0) A 2Π-X 2Σ+ band system of a cold molecular beam sample of magnesium hydride, MgH, has been recorded at high resolution (FWHM ≅60 MHz) and analyzed. The lines associated with the lowest rotational levels are detected for the first time. The field-free spectrum was analyzed to produce spectroscopic parameters for the A 2Π (v = 0) state. The experimentally observed magnetic tuning of the low-rotational spectral features at field strengths comparable to those found in sunspots is accurately modeled by assuming that the electronic spin and orbital magnetic g-factors, g S and gL, of the A 2Π and X 2Σ+ states are 2.002 and 1.000, respectively, and gl is-0.0023 for the X 2Σ+.
Original language | English (US) |
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Article number | 51 (7pp) |
Journal | Astrophysical Journal |
Volume | 781 |
Issue number | 1 |
DOIs | |
State | Published - 2014 |
Keywords
- Sun: magnetic fields
- methods: laboratory: molecular
- molecular data
- stars: magnetic field
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science