Results 131 to 140 of about 2,286 (221)

The Structure of Coronal Loops

open access: yes, 2009
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]

open access: yesSol Phys
Ngampoopun N   +7 more
europepmc   +1 more source

Stereoscopic observations reveal coherent morphology and evolution of solar coronal loops

open access: yes
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
core   +1 more source

Nonlinear Dynamics and Wave Heating in Solar Coronal Loops

open access: yes, 1999
. 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]

open access: yesSol Phys
Woods TN   +9 more
europepmc   +1 more source

Multiwavelength Multipoint Observations of the October 28, 2021 Type III Radio Burst. [PDF]

open access: yesSol Phys
Martinez Oliveros JC   +8 more
europepmc   +1 more source

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