Observation of Six Pre-Flare VLP Pulsations in Solar Corona by Malihe Jalalirad, Narges Fathalian

Subjects: “…solar corona…”
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A Scenario for Origin of Global 4 mHz Oscillations in Solar Corona by Li Xue, Chengliang Jiao, Lixin Zhang

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Reconstructing a Helical Magnetic Field in the Solar Corona using Lagrange Multiplier Technique by Nasim IldarTanha, Sadollah Nasiri

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Modeling the Magnetic Connection from Earth to Solar Corona during the May 11 Geomagnetic Superstorm by Alessandro Ippolito, Tommaso Alberti, Fabio Giannattasio

“…This study aims at improving our understanding of the magnetic connectivity between Earth and the solar corona by reconstructing the magnetic footpoint of the Earth on the solar surface during this geomagnetic superstorm. …”
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Constraining Solar Emission Radius at 42 MHz During the 2024 Total Solar Eclipse Using a Student-commissioned Radio Telescope by Olivia R. Young, Timothy E. Dolch, Joseph F. Helmboldt, Christopher Mentrek, Louis P. Dartez, Michael T. Lam, Sophia V. Sosa Fiscella, Evan Bretl, Colin Joyce, Johannes Loock, Grace Meyer, Annabel Peltzer, Joseph Petullo, Parker Reed, Emerson Sigtryggsson, Benjamin Bassett, Andrew B. Hawken, Alejandro Z. Heredia, Paige Lettow, Whit Lewis, Mikayla Manna, Nicholas Mirochnikoff, Michael Zemcov

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Toward High-order Solar Corona Simulations: A High-order Hyperbolized Poisson Approach for Magnetic Field Initialization by Rayan Dhib, Firas Ben Ameur, Vatsalya Sharma, Andrea Lani, Stefaan Poedts

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Behavior of Magnetohydrodynamic Waves in the Viscous Coronal Loops by Roza Rezaei, Zahra Fazel

Subjects: “…solar corona…”
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An Empirical Relationship Between Coronal Density and Solar Wind Velocity in the Middle Corona With Applications to Space Weather by Kaine A. Bunting, Huw Morgan

Subjects: “…solar corona…”
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Dissipation of Magnetohydrodynamic Waves in the Solar Stratified Flux Tubes by Zahra Fazel

Subjects: “…solar corona…”
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Radial Evolution of MHD Turbulence Anisotropy in Low Mach Number Solar Wind by Xingyu Zhu, Gary P. Zank, Lingling Zhao, Ashok Silwal

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Solar Coronal Mass Ejection and Post–Coronal Mass Ejection Blob Formation in Two-fluid Simulations by J. C. Du, Z. W. Ma

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X-Ray/Radio Quasiperiodic Pulsations Associated with Plasmoids in Solar Flare Current Sheets by Pankaj Kumar, Judith T. Karpen, Joel T. Dahlin

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Prediction of Solar Coronal Structures Using Fourier Neural Operators Based on the Solar Photospheric Magnetic Field Observation by Jingmin Zhao, Xueshang Feng

Subjects: “…solar corona…”
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Identifying the Coronal Holes in Open Magnetic Field Regions Using Deep Learning by Guan-Han Huang, Chia-Hsien Lin

Subjects: “…Solar corona…”
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Multiple Episodes of Remote Brightenings Driven by a Coronal Extreme-ultraviolet Jet on the Sun by Chao Zhang, Zhenghua Huang, Hengyuan Wei, Youqian Qi, Mijie Shi, Hui Fu, Xiuhui Zuo, Weixin Liu, Mingzhe Sun, Ming Xiong, Lidong Xia

Subjects: “…Solar corona…”
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Failure of a Solar Filament Eruption Caused by Magnetic Reconnection with Overlying Coronal Loops by Leping Li, Hongqiang Song, Yijun Hou, Guiping Zhou, Baolin Tan, Kaifan Ji, Yongyuan Xiang, Zhenyong Hou, Yang Guo, Ye Qiu, Yingna Su, Haisheng Ji, Qingmin Zhang, Yudi Ou

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The Effect of Steady Flow on the Physical Quantities of Slow mMagneto Acoustic Waves in Solar Coronal Plasma by Abbas Abedini

“…textbf{Damping of slow magnetohydrodynamic(MHD) waves and oscillations are believed to contribute to the heating of the solar corona. Since the launch of solar space telescopes, many observational evidences for the occurrence of slow MHD waves have been detected in various structures of the solar corona.}In this paper, the effect of steady flow of coronal plasma textbf{on the damping time and other physical quantities} of slow magneto-acoustic waves in the presence of thermal conduction and compressive viscosity is studied.The perturbed and linearized MHD Equations of a flowing coronal plasma are solved both analytically and numerically by Mac Cormack method to investigate the effect of steady flows on physical quantities of slow magneto-acoustic waves.The results of this study show that with increasing magnitude values of the Mach number from 0 to 0.6 and increasing the compressive viscosity and thermal conduction coefficient with increasing the temperature from 2 to 6 MK, the oscillation periods, the damping times and the damping qualities change significantly. …”
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Space Climate and Solar Energetic Particles by Ehsan Tavabi, Sima Zeighami, Yones Kharaghani

“…In this paper, we investigate the effect of solar corona magnetic activities during 11-year periods and energetic particles on global warming. …”
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Investigating the Sensitivity of Alfvén Pulse Interactions to Plasma Beta in the Corona by Naser Karimi, Mahdi Alizadeh, Zianab Shajei

“…Two competing theories, the wave theory and reconnection theory, provide explanations for solar corona heating, supported by observations of wave phenomena and magnetic reconnection on the Sun. …”
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ALMA Observations of Solar Spicules in a Polar Coronal Hole by T. S. Bastian, C. Alissandrakis, A. Nindos, M. Shimojo, S. M. White

“…However, the possibility that electric currents, fast kink and torsional waves, or other wave modes carried by spicules may play a role in transporting energy into the solar corona cannot be excluded.…”
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