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The Hanle Effect as a Diagnostic of Magnetic Fields in Stellar Envelopes. I. Theoretical Results for Integrated Line Profiles

  • Authors: R. Ignace, K. H. Nordsieck, and J. P. Cassinelli

Ignace, Nordsieck, & Cassinelli 1997 The Astrophysical Journal 486 550.

  • Provider: AAS Journals

Caption: Fig. 3.

The stellar coordinate system. The Z*‐axis is the symmetry axis, and the observer views the star along the Z‐axis that is located in the X*Z* plane. The Y and Y*‐axes (not shown) are into the page and coincident. The viewing inclination angle, i, is measured from the Z*‐axis to the Z‐axis. The angles thetav and phiv are the spherical polar angles in the stellar coordinate system. The three arrows labeled nB, ni, and ns are unit vectors for the directions of the magnetic field, incident intensity, and scattered intensity, respectively. The vector r is the spatial position of the scattering point P with respect to the origin.

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