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How Transverse Waves Drive Turbulence in the Solar Corona
Published 2022-02-01“…As a result, over much of the past century, these waves have attracted great interest in the context of the coronal heating problem. They are a potential source of the energy required to maintain the high-temperature plasma and may accelerate the fast solar wind. …”
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Coronal Loop Heating by Nearly Incompressible Magnetohydrodynamic and Reduced Magnetohydrodynamic Turbulence Models
Published 2023-01-01“…The transport of waves and turbulence beyond the photosphere is central to the coronal heating problem. Turbulence in the quiet solar corona has been modeled on the basis of the nearly incompressible magnetohydrodynamic (NI MHD) theory to describe the transport of low-frequency turbulence in open magnetic field regions. …”
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Multifrequency Microwave Imaging of Weak Transients from the Quiet Solar Corona
Published 2023-01-01“…Understanding the dynamics of the quiet solar corona is important for answering key questions including the coronal heating problem. Multiple studies have suggested small-scale magnetic-reconnection events may play a crucial role. …”
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Magnetic Tornado Properties: A Substantial Contribution to the Solar Coronal Heating via Efficient Energy Transfer
Published 2023-01-01“…In solving the solar coronal heating problem, it is crucial to comprehend the mechanisms by which energy is conveyed from the photosphere to the corona. …”
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Spectroscopic Observations of Coronal Rain Formation and Evolution Following an X2 Solar Flare
Published 2024-01-01“…A significant impediment to solving the coronal heating problem is that we currently only observe active region loops in their cooling phase. …”
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An Unsupervised Machine Learning-based Algorithm for Detecting Weak Impulsive Narrowband Quiet Sun Emissions and Characterizing Their Morphology
Published 2023-01-01“…They are hypothesized to be the radio signatures of coronal nanoflares and could potentially have a bearing on the long standing coronal heating problem. In view of the significance of this discovery, this work has been followed up by multiple independent studies. …”
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Hybrid Detection Algorithm and Study on the Quantity and Brightness Evolution Characteristics of Photospheric Bright Point Groups
Published 2023-01-01“…Studying the characteristics of these small-scale strong magnetic fields with kilogauss magnitudes could be of significant importance for investigating the coronal heating problem. Compared to the study of a few specific BPs, investigating the collective features of BP groups can provide us with a better understanding of the overall characteristics of BPs. …”
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AWSoM Magnetohydrodynamic Simulation of a Solar Active Region. II. Statistical Analysis of Alfvén Wave Dissipation and Reflection, Scaling Laws, and Energy Budget on Coronal Loops
Published 2024-01-01“…The coronal heating problem has been a major challenge in solar physics, and a tremendous amount of effort has been made over the past several decades to solve it. …”
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Deciphering Solar Coronal Heating: Energizing Small-scale Loops through Surface Convection
Published 2023-01-01“…Our results constitute a step forward in the understanding of the many different facets of the solar coronal heating problem.…”
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Wave turbulence in magnetized plasmas
Published 2009-02-01“…The solar wind and the coronal heating problems are presented as two examples of application of anisotropic wave turbulence. …”
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