Simulation of quiet Sun waves in the Ca II infrared triplet

Details Simulation of quiet Sun waves in the Ca II infrared triplet Simulation of quiet Sun waves in the Ca II infrared triplet

2005-10-26

arxiv.org/abs/astro-ph/0510744v1

Astrophys.J.640:1142-1152,2006

Astronomy and Astrophysics

Astrophysics

Submitted to ApJ

Scientific paper

10.1086/500240

The Ca II infrared triplet around 8540 A is a good candidate for observing chromospheric magnetism. We show results from combining a radiation hydrodynamic simulation with a Stokes synthesis code. The simulation shows interesting time-varying behavior of the Stokes V profiles as waves propagate through the lines' formation regions. Disappearing and reappearing lobes in the Stokes V profiles as well as profile asymmetries are closely related to the atmospheric velocity gradients.

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