Results 131 to 140 of about 16,413 (221)
Source Materials and Heating of Alfvénic Slow and Hot Solar Wind Revealed by Heavy Ions
This work quantitatively studies the differences of heavy ions among non-Alfvénic slow wind (N-ASSW), classical fast wind (FSW), and Alfvénic slow and hot wind (ASSW and AHSW) by effect size and Kolmogorov–Smirnov statistic.
Shuyi Meng, Shuo Yao
doaj +1 more source
During solar cycle minimum, polar coronal holes show a prominent radio brightening cap. The analysis of polar microwave enhanced radiation in polar coronal holes is helpful for understanding the magnetic field characteristics and the origin of the solar ...
Jing Huang +6 more
doaj +1 more source
Recent advances in solar coronal extreme ultraviolet waves
Solar coronal extreme ultraviolet (EUV) waves are spectacular propagating disturbances in the appearance of EUV emission enhancements in the solar corona, similar to the tsunamis on the Earth. These ‘solar tsunamis’ are closely associated with various solar eruptions, from large-scale coronal mass ejections (CMEs) and solar flares to small-scale solar ...
openaire +1 more source
Magnetohydrodynamic Waves in Solar Coronal Arcades
R. Oliver, A. W. Hood, E. R. Priest
openaire +1 more source
Theoretical studies of the physics of the solar atmosphere [PDF]
Significant advances in our theoretical basis for understanding several physical processes related to dynamical phenomena on the sun were achieved. We have advanced a new model for spicules and fibrils.
Hollweg, Joseph V.
core +1 more source
Coronal cavities, often associated with prominences, are crucial structures in understanding coronal heating and the eruption mechanism of coronal mass ejections.
Chenxi Huangfu +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
A series of solar energetic electron (SEE) events was observed from 2022 November 9 to November 15 by Solar Orbiter, STEREO-A, and near-Earth spacecraft.
D. Lario +30 more
doaj +1 more source
Properties of Magnetic Switchbacks in the Near-Sun Solar Wind. [PDF]
Badman ST +26 more
europepmc +1 more source
Evidence for small-scale torsional Alfvén waves in the solar corona. [PDF]
Morton RJ +5 more
europepmc +1 more source

