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Main Authors: Srivastava, A. K., Singh, Anshika, Singh, Balveer, Murawski, K., Zaqarashvili, T. V., Yuan, D., Scullion, E., Mishra, Sudheer K., Dwivedi, B. N.
Format: Preprint
Published: 2024
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Online Access:https://arxiv.org/abs/2403.14603
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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