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Impulsive Electromagnetic Emission near a Black Hole

  • Authors: Christopher Thompson

2019 The Astrophysical Journal 874 48.

  • Provider: AAS Journals

Caption: Figure 12.

Red curve: rms variation in the linear polarization angle of the prompt electromagnetic pulse, as seen by an observer positioned at a fixed latitude but random orbital phase relative to the emission point. Black curve: rms ϕ component of the electric vector, also averaged over the angle ϕ of emission. Polarization variance is minimized where detection volume is maximized (Figure 11).

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