Spectral index of synchrotron emission: insights from the diffuse and magnetised interstellar medium

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Table 3

Medians of the ratio between the standard deviation of B_⊥ and its median value, , of the brightness temperature spectral index, and of the polarisation fraction at a resolution of 6.7′ for the three POSs and the two cases of weak and strong field^(a).

	POS
Weak field (B₀ = 4 μG)	xy		− 2.66 ± 0.01

	yz		− 2.72 ± 0.02	0.34 ± 0.10

	zx		− 2.66 ± 0.01	0.55 ± 0.06

Strong field (B₀ = 20 μG)	xy	0.02 ± 0.01	− 2.54	0.70
	yz		− 2.84 ± 0.03

	zx	0.02 ± 0.01	− 2.54	0.70

Notes. ^(a) Errors have been estimated using the first and third quartiles. Errors smaller than 0.01 are not shown.

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