A heliospheric density and magnetic field model | Astronomy & Astrophysics (A&A)

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Table 7.

Modelled magnetic field parameters as a function of radial distance in the solar corona.

r/R_⊙	B_r	B_z	\|B_z\|/B_r
	[nT]	[nT]
1.0	12 310	99 303	8.067
1.2	12 285	27 275	2.228
1.4	11 828	7072	0.598
1.6	11 124	967	0.087
1.8	10 308	−797	0.077
2.0	9465	−1169	0.124
3.0	5950	−467	0.078
4.0	3.863	−150	0.039
5.0	2654	−55	0.021

Notes. The table shows the radial component B_r and the z-component B_z according to Eqs. (14) and (15), respectively, and the ratio |B_z|/B_r.

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