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- W2100072484 abstract "A vector magnetometer has been built utilizing the <tex xmlns:mml=http://www.w3.org/1998/Math/MathML xmlns:xlink=http://www.w3.org/1999/xlink>n = 0, p = 1</tex> parametric resonance associated with zero-field level crossings in the optically pumped 2 <sup xmlns:mml=http://www.w3.org/1998/Math/MathML xmlns:xlink=http://www.w3.org/1999/xlink>3</sup> S <inf xmlns:mml=http://www.w3.org/1998/Math/MathML xmlns:xlink=http://www.w3.org/1999/xlink>1</inf> level of He <sup xmlns:mml=http://www.w3.org/1998/Math/MathML xmlns:xlink=http://www.w3.org/1999/xlink>4</sup> . The principles of operation are discussed and performance is described. The parametric resonance signal-to-noise ratio is 3.5 × 10 <sup xmlns:mml=http://www.w3.org/1998/Math/MathML xmlns:xlink=http://www.w3.org/1999/xlink>4</sup> in a 0.5 Hz noise bandwidth. The linewidth is 9.7 × 10 <sup xmlns:mml=http://www.w3.org/1998/Math/MathML xmlns:xlink=http://www.w3.org/1999/xlink>-4</sup> G. Techniques for optimizing the sensitivity are discussed, and the sensitivity of the instrument is demonstrated by placing the sensor inside a superconducting magnetic shield and applying calibration signals, The peak-to-peak noise level is 1 × 10 <sup xmlns:mml=http://www.w3.org/1998/Math/MathML xmlns:xlink=http://www.w3.org/1999/xlink>-8</sup> G. The use of parametric resonance instruments to measure interplanetary and geomagnetic fields is discussed." @default.
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- W2100072484 date "1973-09-01" @default.
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- W2100072484 title "Measurement of weak magnetic fields using zero-field parametric resonance in optically pumped He<sup>4</sup>" @default.
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- W2100072484 doi "https://doi.org/10.1109/tmag.1973.1067647" @default.
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