We then review recently developed millennial - scale spherical harmonic geomagnetic field models and compare their dipole predictions to virtual
axial dipole and virtual geomagnetic pole (VGP) reconstructions, discussing uncertainties in absolute values and variations.
VADMs are obtained by translating archeomagnetic intensity results to the strength of a pure
axial dipole field with that intensity at the given geographic latitudes.
Here we review several spherical harmonic models and compare their dipole field predictions to reconstructions based on virtual
axial dipole moments and virtual geomagnetic poles.
Methods to scale them to absolute intensities include comparison to globally averaged virtual
axial dipole moments (VADM) or to nearby archeomagnetic intensity data.
Not exact matches
So if the C were displaced axially from perfect symmetry, then a
dipole moment would exist; and the same goes for any assymmetrical
axial momentum for the three atoms, so any change would open the molecule to the 4.0 miron assymmetrical stretch mode which is THE strongest CO2 line, and any displacement or momentum out of the linear cofiguration, will open the moleculae to the 15 micron (667 cm ^ -1) LWIR line that is most active in earth atmosphere.