593 citations
- Centre National de la Recherche ScientifiqueFR145 papers
- Université de BordeauxFR114 papers
- Laboratoire d'Astrophysique de BordeauxFR52 papers
- Sorbonne UniversitéFR36 papers
- Institut du CerveauFR24 papers
- Université Paris Sciences et LettresFR20 papers
- Université Paris-SaclayFR19 papers
- Laboratoire d’Etudes du Rayonnement et de la Matière en Astrophysique et AtmosphèresFR16 papers
- Aix-Marseille UniversitéFR15 papers
- Instituto de Física FundamentalES15 papers
- Spanish National ObservatoryES14 papers
- InsermFR13 papers
14 papers · 1 filter
High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona
Yuhang Gao, Hui Tian, Richard Morton +5
The acceleration and heating of the fast solar wind remain long-standing challenges in space physics. One type of leading theoretical models requires high-frequency magnetohydrodyn…
Kinetic Processes to Radio Burst: First Observational-driven Study in Coronal Loops
Mehdi Yousefzadeh, Marian Karlicky, Artem Koval +3
Understanding the origin of coherent solar radio bursts requires linking macroscopic coronal structures with the kinetic processes responsible for wave generation. We investigate e…
The Efficiency of Harmonic Emissions Excited by Energetic Electrons in Coronal Loops
Mehdi Yousefzadeh, Alexey Kuznetsov, Yao Chen +1
Magnetic reconnection is a key process that drives the energy release in solar flares. This process can occur at multiple locations along the coronal loop. The reconnection generat…
Why "solar tsunamis" rarely leave their imprints in the chromosphere
Ruisheng Zheng, Yihan Liu, Wenlong Liu +10
Solar coronal waves frequently appear as bright disturbances that propagate globally from the eruption center in the solar atmosphere, just like the tsunamis in the ocean on Earth.…
Unveiling the mechanism for the rapid acceleration phase in a solar eruption
Ze Zhong, Yang Guo, Thomas Wiegelmann +2
Two major mechanisms have been proposed to drive the solar eruptions: the ideal magnetohydrodynamic instability and the resistive magnetic reconnection. Due to the close coupling a…
The deformation of an erupting magnetic flux rope in a confined solar flare
Ruisheng Zheng, Yihan Liu, Liang Zhang +7
Magnetic flux ropes (MFRs), sets of coherently twisted magnetic field lines, are believed as core structures of various solar eruptions. Their evolution plays an important role to…