  The anomalous microwave emission (AME) still lacks a conclusive explanation.
This excess of emission, roughly between 10 and 50 GHz, correlates spatially
with interstellar dust, prompting a "spinning dust" hypothesis: electric dipole
emission by rapidly rotating, small dust grains. The typical peak frequency
range of the AME profile implicates grains on the order of ~1 nm, suggesting
polycyclic aromatic hydrocarbon molecules (PAHs). We compare AKARI/Infrared
Camera (IRC), with its thorough PAH-band coverage, to AME intensity estimates
from the Planck Collaboration, in the {\lambda} Orionis region. We look also at
infrared dust emission from other mid IR and far-IR bands. The results and
discussion contained here apply to an angular scale of approximately 1{\deg}.
In general, our results support an AME-from-dust hypothesis. In {\lambda}
Orionis, we find that certainly dust mass correlates with AME, and that
PAH-related emission in the AKARI/IRC 9 {\mu}m band may correlate slightly more
strongly.
