Fig. 5
Mean power spectra of cos2γ (top panel) and cos2ψ (bottom panel) over SGC34 for a set of αM and fM parameters in the multipole range 40 <ℓ< 160. The 1σ error bars are computed from the standard deviations of the 100Monte-Carlo realizations of the dust model. The alignment of the CNM structures with BPOS (see Sect.5.1 for details) constrains the value of 
and 
for the CNM component.
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