Results 121 to 130 of about 3,043 (224)
Soft X-ray heating of the solar chromosphere during the gradual phase of two solar flares
In this paper we perform an analysis of the energetics of the solar flaring chromosphere irradiated by soft X-rays (SXR) emitted from overlying hot flare loops.
Berlicki, Arkadiusz +3 more
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A proposed mechanism for solar chromospheric heating is magnetohydrodynamic waves propagating upward along magnetic field lines and dissipating their energy in the chromosphere.
Mayu Koyama, Toshifumi Shimizu
doaj +1 more source
87th Annual Meeting of the Meteoritical Society 2025: Abstracts
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
wiley +1 more source
ALFVÉN WAVE HEATING of the SOLAR CHROMOSPHERE: 1.5D MODELS
ALFVÉN WAVE HEATING of the SOLAR CHROMOSPHERE: 1.5D ...
Sergiy Shelyag (13094397) +2 more
core
Rotation is one of the fundamental characteristics of the Sun, and it plays a crucial role in understanding the magnetic activities and dynamo processes.
Ruoxue Sha +6 more
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Solar UV radiation influence the Earth's climate and upper atmosphere. The UV emission from the Sun modulates with the sunspot cycle with an 11-year periodicity.
(G) Chandrika +2 more
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Context. The solar chromosphere is a dynamic and crucial interface between the solar interior and its interplanetary environment, regulating how energy is locally deposited into heat and transported into the upper atmospheric layers.
Noraz Q., Carlsson M., Aulanier G.
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Propagation and energy dissipation of shock waves in the solar chromosphere [PDF]
The solar atmosphere is permeated by various types of waves that originate from subsurface convection. As these waves propagate upward, they encounter they encounter a steep decrease in the density of the medium, leading to their steepening into shock ...
Erdélyi, R. +2 more
core +1 more source
Alfvén Wave Heating of Solar Chromosphere Reexamined
Models of heating the weakly ionized solar atmosphere by collisional damping of upward-propagating Alfvén waves, calculated under the assumption that only incompressible (intermediate-mode) MHD waves are involved, have predicted heating rates that do not
Vytenis M. Vasyliūnas
doaj +1 more source

