2007/03/19 by L. Heggland, B. De Pontieu, V. H. Hansteen · 1 citation
Physics and Astronomy · #astro-ph
paper · pdf · doi:10.1086/518828
published as Astrophys.J.666:1277-1283,2007 · 7 pages, 11 figures, submitted to ApJ
arxiv created 2007/03/19 · arxiv updated 2011/02/11
We present the results of numerical simulations of shock wave-driven jets in the solar atmosphere. The dependence of observable quantities like maximum velocity and deceleration on parameters such as the period and amplitude of initial disturbances and the inclination of the magnetic field is investigated. Our simulations show excellent agreement with observations, and shed new light on the correlation between velocity and deceleration and on the regional differences found in observations.