Modeling solar chromospheric spicules with intense lasers

Modeling solar chromospheric spicules with intense lasers

Solar spicules are small-scale jet-like structures in the lower solar atmosphere. Currently, the formation of these widely distributed structures lacks a complete explanation. It is still unclear whether they play an essential role in corona heating. Here, based on the magnetohydrodynamic scaling tr...

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Bibliographic Details
Main Authors: Jianzhao Wang, Jiayong Zhong, Weiming An, Weimin Zhou, Chen Wang, Bo Zhang, Yongli Ping, Wei Sun, Xiaoxia Yuan, Pengfei Tang, Yapeng Zhang, Qian Zhang, Chunqing Xing, Zhengdong Liu, Jiacheng Yu, Jun Xiong, Shukai He, Roger Hutton, Yuqiu Gu, Gang Zhao, Jie Zhang
Format: Article
Language:English
Published: Frontiers Media S.A. 2023-09-01
Series:Frontiers in Physics
Subjects:
solar spicules
magnetohydrodynamic (MHD)
magnetic reconnection
high energy density physics
laboratory astrophysics
Online Access:https://www.frontiersin.org/articles/10.3389/fphy.2023.1273568/full

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https://www.frontiersin.org/articles/10.3389/fphy.2023.1273568/full

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