Numerical Simulations of Shock Wave–driven Chromospheric Jets | Zendy

L. Heggland | Zendy; Bart De Pontieu | Zendy; V. H. Hansteen | Zendy

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Numerical Simulations of Shock Wave–driven Chromospheric Jets

Author(s) -

L. Heggland,

Bart De Pontieu,

V. H. Hansteen

Publication year - 2007

Publication title -

the astrophysical journal

Language(s) - English

Resource type - Journals

eISSN - 1538-4357

pISSN - 0004-637X

DOI - 10.1086/518828

Subject(s) - shock wave , physics , amplitude , shock (circulatory) , observable , mechanics , atmosphere (unit) , solar atmosphere , magnetic field , astrophysics , computer simulation , computational physics , meteorology , optics , medicine , quantum mechanics

We present the results of numerical simulations of shock wave-driven jets inthe solar atmosphere. The dependence of observable quantities like maximumvelocity and deceleration on parameters such as the period and amplitude ofinitial disturbances and the inclination of the magnetic field is investigated.Our simulations show excellent agreement with observations, and shed new lighton the correlation between velocity and deceleration and on the regionaldifferences found in observations.Comment: 7 pages, 11 figures, submitted to Ap

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