Table 3.

Observed Stokes coefficients (no units) of gravity variations of degree 2 and contribution from core processes

	$\Delta C_{20}$		$\Delta C_{21}$, $\Delta S_{21}$		$\Delta C_{22}$, $\Delta S_{22}$
	Decadal	6 year	Decadal	6 year	Decadal	6 year
Observed	1	0.5	0.5	0.2	0.5	0.2
CMB pressure	0.1	0.01	0.05	0.005	0.05	0.005
Density ${\text{anomalies}}^{†}$	0.05	0.005	0.025	0.0025	0.025	0.0025
Inner core rotation					0.2	0.006
Inner core ${\text{tilt}}^{‡}$			0.025	0.0025

All numerical values are multiplied by a factor ${10}^{-10}$. To retrieve amplitudes in units of nGal, numerical values for $m=0$, 1 and 2 should be multiplied by $6.59\times {10}^{12}$ (for the amplitude at the poles), $1.14\times {10}^{13}$ and $5.70\times {10}^{12}$, respectively

^†Set to half of the contribution from CMB pressure based on the results in Dumberry (2010)

^‡Not a prediction, but assuming an inner core tilt generating a decadal (6 year) polar motion of 1 (0.1) mas