Results 91 to 100 of about 1,306 (183)

Energy and Mass Transport Associated with Impulsive Spicular Flows in Solar Coronal Holes

open access: yesThe Astrophysical Journal Letters
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
doaj   +1 more source

Solar Force-free Magnetic Fields

open access: yesLiving Reviews in Solar Physics, 2012
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]

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

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

SuryaBench: Benchmark Dataset for Advancing Machine Learning in Heliophysics and Space Weather Prediction. [PDF]

open access: yesSci Data
Roy S   +24 more
europepmc   +1 more source

The Behaviour of the EUV Corona Before Flares in Regions with High Free Magnetic Energy. [PDF]

open access: yesSol Phys
Harra L   +8 more
europepmc   +1 more source

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