2019
DOI: 10.1103/physreva.99.013420
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Sources of heading errors in optically pumped magnetometers operated in the Earth's magnetic field

Abstract: When optically pumped magnetometers are aimed for the use in Earth's magnetic field, the orientation of the sensor to the field direction is of special importance to achieve accurate measurement result. Measurement errors and inaccuracies related to the heading of the sensor can be an even more severe problem in the case of special operational configurations, such as for example the use of strong off-resonant pumping. We systematically study the main contributions to the heading error in systems that promise h… Show more

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Cited by 36 publications
(42 citation statements)
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“…The solid lines in Figure a are the fitted sinusoidal curves of the measured results that write lefttrueω1,1θ/2π=1,124.8043.35Sin1.99θ+0.28,ω0,0θ/2π=28.163.14Cos4.01θ+18.92,ω1,1θ/2π=+1082.69+43.92Sin1.96θ+3.76, where ωmF,mF()θ/2π ( m F = − 1,0,1) is in the unit of Hz, whereas θ is in the unit of rad. Based on the fitted results in Equation , the absolute magnetic field is extracted as B eff = 78.84 nT using the method proposed by Oelsner et al and Hu et al; thus the Zeeman frequency shift of the ω 1, 1 ( ω −1, − 1 ) transition peak is δ Zeeman = 1,103.74 Hz (−1,103.74 Hz). The Doppler shifts are calculated as δ D = 6.15 Hz for the three resonant frequencies using the Raman laser's effective wave vector kfalse→eff and the atomic velocity vfalse→atom at 0.4 s after launch, and the angles θ k and α 0 of the effective magnetic field vector Bfalse→eff are extracted as 3.4° and 80.54° by comparing Equation with Equation .…”
Section: Resultsmentioning
confidence: 99%
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“…The solid lines in Figure a are the fitted sinusoidal curves of the measured results that write lefttrueω1,1θ/2π=1,124.8043.35Sin1.99θ+0.28,ω0,0θ/2π=28.163.14Cos4.01θ+18.92,ω1,1θ/2π=+1082.69+43.92Sin1.96θ+3.76, where ωmF,mF()θ/2π ( m F = − 1,0,1) is in the unit of Hz, whereas θ is in the unit of rad. Based on the fitted results in Equation , the absolute magnetic field is extracted as B eff = 78.84 nT using the method proposed by Oelsner et al and Hu et al; thus the Zeeman frequency shift of the ω 1, 1 ( ω −1, − 1 ) transition peak is δ Zeeman = 1,103.74 Hz (−1,103.74 Hz). The Doppler shifts are calculated as δ D = 6.15 Hz for the three resonant frequencies using the Raman laser's effective wave vector kfalse→eff and the atomic velocity vfalse→atom at 0.4 s after launch, and the angles θ k and α 0 of the effective magnetic field vector Bfalse→eff are extracted as 3.4° and 80.54° by comparing Equation with Equation .…”
Section: Resultsmentioning
confidence: 99%
“…In our previous study, we presented the frequency‐dependent SVT dynamical polarizabilities and measured the vector and tensor dynamical polarizabilities between the 5s ground‐state sublevels interacting with a pair of circularly polarized lasers. A recent study had demonstrated that the major heading error sources of the optically pumped magnetometers are the nonlinear Zeeman splitting and the orientation‐dependent LS.…”
Section: Introductionmentioning
confidence: 99%
“…On the one hand, the measured resonance frequencies are strongly modified by the light shift due to the intense off-resonant pumping. This effect has been extensively studied [6,7,9,24] and we use the method presented in Ref. [6] for a description of our data.…”
Section: Iib Theoretical Descriptionmentioning
confidence: 99%
“…Ref. [6]) as well as an additional factor of |cos α|. Also, we did not include the linear polarized component scaling with sin α that, in principle, can also contribute to a population difference.…”
Section: Iib Theoretical Descriptionmentioning
confidence: 99%
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