Energy and Mass Transport Associated with Impulsive Spicular Flows in Solar Coronal Holes
How the solar atmosphere is heated from a temperature of about 5000 to 6000 K in the lower atmosphere to about 1–2 MK in the corona has challenged the astrophysical community for nearly 80 yr.
Lei Ni +5 more
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Solar Force-free Magnetic Fields
The structure and dynamics of the solar corona is dominated by the magnetic field. In most areas in the corona magnetic forces are so dominant that all non-magnetic forces like plasma pressure gradient and gravity can be neglected in the lowest order ...
Thomas Wiegelmann, Takashi Sakurai
doaj
Investigating the Relationship Between Physical Properties and Spatial Irregularities at Coronal Hole Boundaries. [PDF]
Ngampoopun N +7 more
europepmc +1 more source
Revealing Flare Energetics and Dynamics with SDO EVE Solar Extreme Ultraviolet Spectral Irradiance Observations. [PDF]
Woods TN +9 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
Imaging spectroscopy reveals spike-like repeating radio burst pairs in the solar corona. [PDF]
Ma 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
Multiwavelength Multipoint Observations of the October 28, 2021 Type III Radio Burst. [PDF]
Martinez Oliveros JC +8 more
europepmc +1 more source
SuryaBench: Benchmark Dataset for Advancing Machine Learning in Heliophysics and Space Weather Prediction. [PDF]
Roy S +24 more
europepmc +1 more source
The Behaviour of the EUV Corona Before Flares in Regions with High Free Magnetic Energy. [PDF]
Harra L +8 more
europepmc +1 more source

