Exploring the generation and annihilation of three dimensional nulls through MHD simulations in initially chaotic magnetic field devoid of nulls
Yogesh Kumar Maurya (1, 2), Ramit Bhattacharyya (1), David I., Pontin (3), and Sanjay Kumar (4) ((1) Udaipur Solar Observatory, Physical, Research Laboratory, Udaipur, Rajasthan, India, (2) Department of Physics,, Indian Institute of Technology, Gandhinagar, Gujarat, India

TL;DR
This study uses advanced MHD simulations and null-tracking tools to demonstrate that three-dimensional magnetic nulls can be generated and annihilated in initially chaotic magnetic fields, clarifying their formation mechanisms.
Contribution
It provides a detailed, precise analysis of null generation and annihilation in chaotic magnetic fields using improved null-tracking and field line tracing methods.
Findings
Nulls can form spontaneously in initially chaotic magnetic fields.
Nulls are dynamically created and destroyed through magnetic reconnection.
The study clarifies null topologies and their evolution over time.
Abstract
Three-dimensional (3D) magnetic nulls are abundant in the solar atmosphere, as been firmly established through contemporary observations. They are established to be important magnetic structures in, for example, jets and circular ribbon flares. While simulations and extrapolations support this, the mechanisms behind 3D null generation remain an open question. Recent magnetohydrodynamics (MHD) simulations propose that magnetic reconnection is responsible for both generating and annihilating 3D nulls, a novel concept. However, these simulations began with initial magnetic fields already supporting pre-existing nulls, raising the question of whether magnetic reconnection can create nulls in fields initially devoid of them. Previously, this question was briefly explored in a simulation with an initial chaotic magnetic field. However, the study failed to precisely identify locations,…
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Taxonomy
TopicsGeomagnetism and Paleomagnetism Studies
