Near infrared observations of solar chromosphere
The solar chromosphere is an excellent medium to explore the intricate interplay between plasma and magnetic fields in a regime where both are relevant and alternately dominant.
Tejomoortula, Usha Sree
core
From hand-ground lenses to Xihe solar space missions: an interview of Professor Cheng Fang. [PDF]
Li C.
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Solar Doppler Velocity Results from the SDO EVE Level 4 Lines Data Product. [PDF]
Woods TN +6 more
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Correlation between active regions' spectra at high radio frequencies and solar flare occurrences. [PDF]
Mulas S +33 more
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Vortex Motions in the Solar Atmosphere: Definitions, Theory, Observations, and Modelling. [PDF]
Tziotziou K +14 more
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The Behaviour of the EUV Corona Before Flares in Regions with High Free Magnetic Energy. [PDF]
Harra L +8 more
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Transverse oscillations and an energy source in a strongly magnetized sunspot. [PDF]
Yuan D +14 more
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Numerical Modeling of Prominences and Coronal Rain with the MPI-AMRVAC Code. [PDF]
Liakh V, Jenkins J.
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Alfvén Waves in Partially Ionised Solar Steady-State Plasmas. [PDF]
Alshehri NF, Ballai I, Verth G, Fedun V.
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Magnetic activity and spectral behavior of RS CVn binary system (IM Pegasi) in the ultraviolet. [PDF]
Sanad MR, Rahman HIA, Badawy WA.
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