Results 71 to 80 of about 11,539 (164)

Ca II λ854.2 nm in an enhanced network region simulated with MURaM-ChE

open access: yesAstronomy & Astrophysics
Context. The Ca IIλ854.2 nm line is widely used to study the chromosphere of the Sun. In the quiet Sun, the spatially averaged line profile shows a red asymmetry and a redshift of the line center. It is known that the effect of isotopic splitting must be
Ondratschek P. A.   +4 more
doaj   +1 more source

Buildup, Explosion, and Untwisting of a Solar Active Region Jet Observed with Solar Orbiter, IRIS, and SDO

open access: yesThe Astrophysical Journal
We present detailed analysis of an active region coronal jet accompanying a minifilament eruption that is fully captured and well resolved in high spatial resolution 174 Å coronal images from Solar Orbiter’s Extreme Ultraviolet Imager (EUI).
Navdeep K. Panesar   +8 more
doaj   +1 more source

A High-resolution, Inversion-based Synoptic Study of Solar Granulation

open access: yesThe Astrophysical Journal
The convectively driven, weakly magnetized regions of the solar photosphere dominate the Sun’s surface at any given time, but the temporal variations of these quiet regions of the photosphere throughout the solar cycle are still not well known.
James W. Crowley   +3 more
doaj   +1 more source

MODELING THE CHROMOSPHERE OF A SUNSPOT AND THE QUIET SUN

open access: yesThe Astrophysical Journal, 2015
E. Avrett   +4 more
openaire   +2 more sources

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

A Survey of Current Operations-Ready Thermospheric Density Models for Drag Modeling in LEO Operations. [PDF]

open access: yesJ Astronaut Sci
Mutschler S   +10 more
europepmc   +1 more source

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