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Fig. 4.

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Geometry of the pulsar and main parameters of the RVM. The pulsar angular momentum, Ωp, makes an angle ip with respect to the line of sight (along vector o). The angle θp is between magnetic dipole, B, and the NS angular momentum Ωp. Pulsar phase ϕ is the azimuthal angle of vector B in the plane (x, y) perpendicular to Ωp. The position angle χp is the angle measured counterclockwise between the direction to the north N and the projection of Ωp on the plane of the sky (N-E).

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