Aspect ratios of far-infrared and H I filaments in the diffuse interstellar medium at high Galactic latitudes

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Table 2

Locations and distances for the loop I and IV regions according to Panopoulou et al. (2021) with derived magnetic field strengths.

Region	Location (l, b)	Distance (pc)	〈δB〉 (μG)	〈B_ST〉 (μG)
I_B	33^°.95, 38^°.03	112 ± 17 pc	8.5 ± .1	7.3 ± .1
I_C	26°.68, 58°.73	≤105pc	5.3 ± .1	4.8 ± .2
I_D	358°. 17, 74°.06	135 ± 20 pc	4.1 ± .1	3.6 ± .2

IV_A	328°.74, 33°.59	180 ± 15 pc	4.0 ± .1	3.1 ± .2

Notes. For the field Ic, we used a distance of 105 pc. Uncertainties are the expected errors in the case of a random distribution without systematic effects.

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