Three-dimensional magnetic field imaging of protoplanetary disks using Zeeman broadening and linear polarization observations

Open Access

Table 2

Zeeman signatures and the magnetic field components they are sensitive to.

Technique	Sensitivity	Equation
Circular pol.	B_los	Eq. (7)
Zeeman broad.	B²,	Eq. (9)
Linear pol.	,	Eq. (10)

GK effect	,
Dust polarization	,

Notes. The magnetic field components are divided into the line-of-sight component, B_los, and the two components in the plane of the sky, and .

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