Fine Structures of Tiny Quiet Sun Jets Observed by Solar Orbiter and Big Bear Solar Observatory
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
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
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]
Tziotziou K +14 more
europepmc +1 more source
Source Region of the Solar Wind: Statistics of the Doppler Velocities at the Chromosphere
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
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]
Yuan D +14 more
europepmc +1 more source
Comparative Analysis of Ellerman and Quiet Sun Ellerman Bombs in the Solar Atmosphere
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
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]
Jafarzadeh S +14 more
europepmc +1 more source

