Results 91 to 100 of about 285 (167)

Fine Structures of Tiny Quiet Sun Jets Observed by Solar Orbiter and Big Bear Solar Observatory

open access: yesThe Astrophysical Journal Letters
We present the first joint high-resolution observations of small-scale EUV jets using Solar Orbiter (SolO)’s Extreme Ultraviolet Imager and High Resolution Imager (EUI/HRI _EUV ) and H α imaging from the Visible Imaging Spectrometer installed on the 1.6 ...
Jeongwoo Lee   +5 more
doaj   +1 more source

Three-dimensional Magnetic Field Structure of a Quiet-Sun Region Revealed by SUNRISE III/SCIP

open access: yesThe Astrophysical Journal Letters
The balloon-borne stratospheric solar observatory S unrise iii successfully completed 6.5 days of observations in 2024 July. One of its focal-plane instruments, the Sunrise Chromospheric Infrared spectroPolarimeter (SCIP), is a slit-scanning ...
Masahito Kubo   +40 more
doaj   +1 more source

Validating Solar Atmosphere Models with High-resolution Spectra: The Case of Balmer Lines

open access: yesThe Astrophysical Journal
Stellar and solar atmosphere models are critical tools for numerous astrophysical applications, including the determination of stellar fundamental parameters, the study of stellar dynamos, and the characterization of exoplanetary atmospheres ...
Serena Criscuoli   +3 more
doaj   +1 more source

Vortex Motions in the Solar Atmosphere: Definitions, Theory, Observations, and Modelling. [PDF]

open access: yesSpace Sci Rev, 2023
Tziotziou K   +14 more
europepmc   +1 more source

Source Region of the Solar Wind: Statistics of the Doppler Velocities at the Chromosphere

open access: yesThe Astrophysical Journal Letters
The solar wind has been extensively studied recently with in situ observations, and the understanding of its counterpart near the solar surface has also progressed significantly.
Fu Yu   +10 more
doaj   +1 more source

Steady-state Heating of Diffuse Coronal Plasma in a Solar Active Region

open access: yesThe Astrophysical Journal
The solar corona is much hotter than lower layers of the solar atmosphere—the photosphere and chromosphere. The coronal temperature is up to 1 MK in quiet Sun areas, while up to several megakelvins in active regions, which implies a key role of the ...
Gregory D. Fleishman   +2 more
doaj   +1 more source

Transverse oscillations and an energy source in a strongly magnetized sunspot. [PDF]

open access: yesNat Astron, 2023
Yuan D   +14 more
europepmc   +1 more source

Comparative Analysis of Ellerman and Quiet Sun Ellerman Bombs in the Solar Atmosphere

open access: yesThe Astrophysical Journal
Ellerman bombs (EBs) and quiet-Sun Ellerman bombs (QSEBs) are small-scale signatures of magnetic reconnection in the lower solar atmosphere, observed in active regions and quiet-Sun areas, respectively. We investigate and compare some of their properties
Ravi Chaurasiya   +2 more
doaj   +1 more source

Bifrost Models of the Quiet Sun. I. Comparison with Solar Observations

open access: yesThe Astrophysical Journal
Studying the emergence of magnetic fields is essential for understanding the physical mechanisms behind various phenomena in the solar atmosphere. Most importantly, the emerging fields offer valuable insights into how energy and mass are transferred to ...
M. Gošić   +4 more
doaj   +1 more source

An overall view of temperature oscillations in the solar chromosphere with ALMA. [PDF]

open access: yesPhilos Trans A Math Phys Eng Sci, 2021
Jafarzadeh S   +14 more
europepmc   +1 more source

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