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| Main Authors: | , , , , , , , , |
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| Format: | Preprint |
| Published: |
2024
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/2403.14603 |
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| _version_ | 1866909145179881472 |
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| author | Srivastava, A. K. Singh, Anshika Singh, Balveer Murawski, K. Zaqarashvili, T. V. Yuan, D. Scullion, E. Mishra, Sudheer K. Dwivedi, B. N. |
| author_facet | Srivastava, A. K. Singh, Anshika Singh, Balveer Murawski, K. Zaqarashvili, T. V. Yuan, D. Scullion, E. Mishra, Sudheer K. Dwivedi, B. N. |
| contents | We present the formation of quasi-periodic cool spicule-like jets in the solar atmosphere using 2.5-D numerical simulation in two-fluid regime (ions+neutrals) under the presence of thermal conduction and ion-neutral collision. The non-linear, impulsive Alfvénic perturbations at the top of the photosphere trigger field aligned magnetoacoustic perturbations due to ponderomotive force. The transport of energy from Alfvén pulse to such vertical velocity perturbations due to ponderomotive force is considered as an initial trigger mechanism. Thereafter, these velocity perturbations steepen into the shocks followed by quasi-periodic rise and fall of the cool jets transporting mass in the overlying corona. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2403_14603 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Alfvén Pulse Driven Spicule-like Jets in the Presence of Thermal Conduction and Ion-Neutral Collision in Two-Fluid Regime Srivastava, A. K. Singh, Anshika Singh, Balveer Murawski, K. Zaqarashvili, T. V. Yuan, D. Scullion, E. Mishra, Sudheer K. Dwivedi, B. N. Solar and Stellar Astrophysics Plasma Physics Space Physics We present the formation of quasi-periodic cool spicule-like jets in the solar atmosphere using 2.5-D numerical simulation in two-fluid regime (ions+neutrals) under the presence of thermal conduction and ion-neutral collision. The non-linear, impulsive Alfvénic perturbations at the top of the photosphere trigger field aligned magnetoacoustic perturbations due to ponderomotive force. The transport of energy from Alfvén pulse to such vertical velocity perturbations due to ponderomotive force is considered as an initial trigger mechanism. Thereafter, these velocity perturbations steepen into the shocks followed by quasi-periodic rise and fall of the cool jets transporting mass in the overlying corona. |
| title | Alfvén Pulse Driven Spicule-like Jets in the Presence of Thermal Conduction and Ion-Neutral Collision in Two-Fluid Regime |
| topic | Solar and Stellar Astrophysics Plasma Physics Space Physics |
| url | https://arxiv.org/abs/2403.14603 |