The Structure of Coronal Loops
It is widely believed that the simple coronal loops observed by XUV imagers, such as EIT, TRACE, or XRT, actually have a complex internal structure consisting of many (perhaps hundreds) of unresolved, interwoven "strands".
Antiochos, Spiro K.
core
Investigating the Relationship Between Physical Properties and Spatial Irregularities at Coronal Hole Boundaries. [PDF]
Ngampoopun N +7 more
europepmc +1 more source
Stereoscopic observations reveal coherent morphology and evolution of solar coronal loops
Coronal loops generally trace magnetic lines of force in the upper solar atmosphere. Understanding the loop morphology and its temporal evolution has implications for coronal heating models that rely on plasma heating due to reconnection at current ...
L. P. Chitta +4 more
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Evolution of Open Magnetic Flux and Heliospheric Current Sheet-Associated Streamer Wind Across Multiple Solar Cycles. [PDF]
MacTaggart JR +4 more
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Nonlinear Dynamics and Wave Heating in Solar Coronal Loops
. We present the rst results of 2.5D nonlinear magnetohydrodynamic wave heating simulations of solar coronal loops with inclusion of the modeling of the coupling to the transition region and chromosphere. Magnetic ux tubes with xed lengths are considered
A.J.C. Beliën +3 more
core
Revealing Flare Energetics and Dynamics with SDO EVE Solar Extreme Ultraviolet Spectral Irradiance Observations. [PDF]
Woods TN +9 more
europepmc +1 more source
30-min decayless kink oscillations in a very long bundle of solar coronal plasma loops. [PDF]
Zhong S +4 more
europepmc +1 more source
The Sun as a driver of the inner heliosphere: Modern investigations of fundamental plasma processes. [PDF]
Ervin T, Nakhleh AJ, Bharati Das S.
europepmc +1 more source
Day-to-Day Boundary Fluctuations in Coronal Holes: Causes and Consequences. [PDF]
Ugarte-Urra I +3 more
europepmc +1 more source
Multiwavelength Multipoint Observations of the October 28, 2021 Type III Radio Burst. [PDF]
Martinez Oliveros JC +8 more
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