Results 141 to 150 of about 3,043 (224)
. The natural state of the Solar chromosphere is very dynamic. Any photospheric disturbance will grow and naturally form shocks over the twenty scale-heights in density between the photosphere and the corona.
Mats Carlsson, Robert F. Stein
core
Revealing Flare Energetics and Dynamics with SDO EVE Solar Extreme Ultraviolet Spectral Irradiance Observations. [PDF]
Woods TN +9 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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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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Numerical Modeling of Prominences and Coronal Rain with the MPI-AMRVAC Code. [PDF]
Liakh V, Jenkins J.
europepmc +1 more source
Alfvén Waves in Partially Ionised Solar Steady-State Plasmas. [PDF]
Alshehri NF, Ballai I, Verth G, Fedun V.
europepmc +1 more source
Magnetic activity and spectral behavior of RS CVn binary system (IM Pegasi) in the ultraviolet. [PDF]
Sanad MR, Rahman HIA, Badawy WA.
europepmc +1 more source
Spatial variation of energy transport mechanisms within solar flare ribbons. [PDF]
Kerr GS +12 more
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