Fig. 18
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All-sky Mollweide displays of derived H I parameters. Top: velocity distribution for coherent FIR and H I filaments in the velocity range − 30 < vLSR < 30 km s−1. Middle: distribution of the velocity dispersions along filaments for 
km s−1. Bottom: spatial distribution of harmonic mean H I Doppler temperatures for 2 < log(TD) < 4.
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