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- W2009787260 abstract "Recent solar observations (e.g., obtained with Hinode and STEREO) have revealed that coronal jets are a more frequent phenomenon than previously believed. This higher frequency results, in part, from the fact that jets exhibit a homologous behavior: successive jets recur at the same location with similar morphological features. We present the results of three-dimensional (3D) numerical simulations of our model for coronal jets. This study demonstrates the ability of the model to generate recurrent 3D untwisting quasi-homologous jets when a stress is constantly applied at the photospheric boundary. The homology results from the property of the 3D null-point system to relax to a state topologically similar to its initial configuration. In addition, we find two distinct regimes of reconnection in the simulations: an impulsive 3D mode involving a helical rotating current sheet that generates the jet and a quasi-steady mode that occurs in a 2D-like current sheet located along the fan between the sheared spines. We argue that these different regimes can explain the observed link between jets and plumes." @default.
- W2009787260 created "2016-06-24" @default.
- W2009787260 creator A5021930656 @default.
- W2009787260 creator A5065101273 @default.
- W2009787260 creator A5075665953 @default.
- W2009787260 date "2010-04-22" @default.
- W2009787260 modified "2023-10-18" @default.
- W2009787260 title "THREE-DIMENSIONAL MODELING OF QUASI-HOMOLOGOUS SOLAR JETS" @default.
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- W2009787260 doi "https://doi.org/10.1088/0004-637x/714/2/1762" @default.
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