On transition region convection cells in simulations of {p}-mode propagation

Details On transition region convection cells in simulations of {p}-mode propagation On transition region convection cells in simulations of {p}-mode propagation

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007an....328..752m&link_type=abstract

Astronomische Nachrichten, Vol.328, Issue 8, p.752-755

Astronomy and Astrophysics

Astronomy

Convection, Sun: Oscillations, Sun: Photosphere, Sun: Transition Region

Scientific paper

This paper examines the way that transition region surface waves, generated in 2-D numerical simulations of the non-magnetic solar atmosphere when various synthetic photospheric drivers are applied, drive the granulation of the transition region/lower coronal region into convection cells. It is shown that these cells are generated by both synthetic point drivers and synthetic horizontally coherent {p}-mode drivers. These cells cause the conversion of driven signals in vertical velocity into coronal signals predominantly in horizontal velocity, which if carried over to a case with a magnetic field included could cause mode conversion.

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