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Solar coronal loops are the building blocks of the solar corona. These dynamic structures are shaped by the magnetic field that expands into the solar atmosphere.
Patrick Antolin, Clara Froment
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Coronal Heating Rate in the Slow Solar Wind
This Letter reports the first observational estimate of the heating rate in the slowly expanding solar corona. The analysis exploits the simultaneous remote and local observations of the same coronal plasma volume, with the Solar Orbiter/Metis and the ...
Daniele Telloni +61 more
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We propose that coronal heating in EUV coronal plumes is weaker, not stronger, than in adjacent nonplume coronal magnetic funnels. This expectation stems from (i) the observation that an EUV plume is born as the magnetic flux at the foot of the plume’s ...
Ronald L. Moore +3 more
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Solar Coronal Heating by Kinetic Alfvén Waves
The utilization of the Cairns distribution serves as a vital tool for characterizing the nonthermal attributes commonly observed in space plasmas.
Syed Ayaz, Gang Li, Imran A. Khan
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Coronal Heating from Alfvén Wave Turbulence in Solar Coronal Loops
This work is supported by the NSF-REU Solar Physics program at SAO, grant number AGS-1850750.
Hamann, Sydney
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In the solar coronal numerical simulation, the coronal heating/acceleration and the magnetic divergence cleaning techniques are very important. The coronal–interplanetary total variation diminishing (COIN-TVD) magnetohydrodynamic (MHD) model is developed
Chang Liu +9 more
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Deciphering Solar Coronal Heating: Energizing Small-scale Loops through Surface Convection
The solar atmosphere is filled with clusters of hot small-scale loops commonly known as coronal bright points (CBPs). These ubiquitous structures stand out in the Sun by their strong X-ray and/or extreme-ultraviolet (EUV) emission for hours to days ...
D. Nóbrega-Siverio +6 more
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The Role of High-frequency Transverse Oscillations in Coronal Heating
Transverse oscillations that do not show significant damping in solar coronal loops are found to be ubiquitous. Recently, the discovery of high-frequency transverse oscillations in small-scale loops has been accelerated by the Extreme Ultraviolet Imager ...
Daye Lim +5 more
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OBSERVING THE ROOTS OF SOLAR CORONAL HEATING—IN THE CHROMOSPHERE [PDF]
14 pages, 5 figures, accepted for publication in ApJ ...
De Pontieu, Bart +3 more
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Estimating Ion Temperatures at the Polar Coronal Hole Boundary
The temperatures of the heavy ions ( T _i ) in the solar corona provide critical information about the heating mechanism of the million-degree corona.
Yingjie Zhu, Judit Szente, Enrico Landi
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