ConstantID

Shielded helion gyromagnetic ratio in MHz/T

Atomic & nuclearMeasured

γh′/2π = 32.434 100 033(28) MHz T−1

Value
32.434 100 033 MHz T−1
Standard uncertainty
2.8 × 10−8 MHz T−1
Relative uncertainty
8.6 × 10−10 (863 parts per trillion)
Status
Measured
Symbol
γh′/2π
Source
CODATA 2022 via NIST · NIST entry

Use in a calculation

# shielded helion gyromagnetic ratio in MHz/T, CODATA 2022 (NIST)
shielded_helion_gyromagnetic_ratio_in_mh = 3.2434100033e1  # MHz T^-1, standard uncertainty 2.8e-8

# SciPy: scipy.constants.physical_constants['shielded helion gyromag. ratio in MHz/T']

What it is

The precession frequency, per tesla of magnetic field, of a helion in a helium-3 gas atom (spherical sample at 25 °C), screened by the atom's two electrons: the gyromagnetic ratio divided by 2π. Magnetic resonance spectroscopists use this form.

How the value changed, 1998–2022

Each point is one CODATA adjustment, plotted as its difference from the 2022 value; the bars show one standard uncertainty (an arrowhead means the bar runs off the chart).

shielded helion gyromagnetic ratio in MHz/T: CODATA values 1998–2022 relative to the 2022 value, in parts per billion, with one-standard-uncertainty bars−150−100−500+50+100+150parts per billion1998200220062010201420182022

Relative uncertainty

shielded helion gyromagnetic ratio in MHz/T: relative standard uncertainty in each CODATA adjustment, logarithmic scale10⁻¹⁰10⁻⁹10⁻⁸10⁻⁷1998200220062010201420182022
CODATAValue (uncertainty)Relative uncertaintyChange from previous
202232.434 100 033(28)8.6 × 10−10 +1.6 σ of 2018
201832.434 099 42(38)1.2 × 10−8 −0.6 σ of 2014
201432.434 099 66(43)1.3 × 10−8 −1.5 σ of 2010
201032.434 100 84(81)2.5 × 10−8 −1.3 σ of 2006
200632.434 101 98(90)2.8 × 10−8 +0.2 σ of 2002
200232.434 1015(28)8.6 × 10−8 −0.7 σ of 1998
199832.434 1025(14)4.3 × 10−8

“Change from previous” is the shift in the value divided by the standard uncertainty of the previous adjustment. Earlier values are converted into the current unit where NIST changed it (for example J s to J Hz⁻¹).

Related constants