Results 121 to 130 of about 43,284 (218)
Solar Coronal Loops Resolved by Hinode and SDO
Revised version accepted by ApJ ...
Brooks, David H. +2 more
openaire +2 more sources
Spatiotemporal Low First Ionization Potential Abundance: A Catalyst for Coronal Condensation
Radiative losses play a critical role in the cooling of plasmas. When chromospheric plasma is sufficiently heated, it can flow into coronal loops, which subsequently cool down due to radiation. From observations, we infer that this cooling does not occur
Luke Fushimi Benavitz +3 more
doaj +1 more source
Aims. Solar type II radio bursts are commonly attributed to coronal shocks driven by coronal mass ejections (CMEs). However, some metric type II bursts have occasionally been reported to occur in the absence of a CME and to be associated with weak solar ...
Cui Yingli +14 more
doaj +1 more source
The energy that heats the magnetically closed solar corona originates in the complex motions of the massive photosphere. Turbulent photospheric convection slowly displaces the footpoints of coronal field lines, causing them to become twisted and tangled.
Craig D. Johnston +7 more
doaj +1 more source
Turbulent Suppression of Alfvénic Wave Resonances in Coronal Loops
Alfvénic wave turbulence is a leading mechanism for explaining the heating of the solar corona and the acceleration of the solar wind. Alfvénic waves are observed to be prevalent throughout the inner corona.
Edris Tajfirouze +2 more
doaj +1 more source
Coronal rain (CR) is a crucial part of the mass cycle between the corona and chromosphere. It includes flare-driven CR and two types of quiescent CR, along nonflaring active region closed loops and along open structures, separately, labeled as type I ...
Fangfang Qiao +6 more
doaj +1 more source
Apparent Transverse Motion of Light Bridges Coupled to Coronal Loop Dynamics
Light bridges (LBs) are commonly observed in active regions and are interpreted as signatures of magnetoconvective processes in sunspots. Several studies have attempted to classify them in the past based on their morphological characteristics.
Atul Bhat +3 more
doaj +1 more source
Using both analytical and numerical means, we demonstrate that linear stability analysis of a hydrodynamic stratified atmosphere or a 1D coronal loop model in nonadiabatic settings features a thermal continuum corresponding to highly localized ...
Rony Keppens +4 more
doaj +1 more source
Investigating the Relationship Between Physical Properties and Spatial Irregularities at Coronal Hole Boundaries. [PDF]
Ngampoopun N +7 more
europepmc +1 more source
Evolution of Open Magnetic Flux and Heliospheric Current Sheet-Associated Streamer Wind Across Multiple Solar Cycles. [PDF]
MacTaggart JR +4 more
europepmc +1 more source

