Results 121 to 130 of about 5,669 (225)
We investigate the height variation of the line-of-sight (LOS) magnetic field in solar active-region (AR) plage from the upper photosphere to the upper chromosphere using cospatial ultraviolet and infrared spectropolarimetric observations from the ...
Iñigo Juanikorena Berasategi +33 more
doaj +1 more source
The role and contribution of magnetic fields, characterized via their magnetic flux, to the statistical structuring of the solar atmosphere. [PDF]
Li KJ, Xu JC, Feng W.
europepmc +1 more source
Measuring the magnetic fields in the chromospheres of low-mass stars. [PDF]
Cang T +13 more
europepmc +2 more sources
Accurately assessing the balance between acoustic wave energy fluxes and radiative losses is critical for understanding how the solar chromosphere is thermally regulated.
J. M. da Silva Santos +5 more
doaj +1 more source
Magnetic Fields beneath Active Region Coronal Loops
We examine the hypothesis that multipolar magnetic fields advected by photospheric granules can contribute to heating the active chromosphere and corona.
Philip G. Judge, L. Kleint, C. Kuckein
doaj +1 more source
Vortex Motions in the Solar Atmosphere: Definitions, Theory, Observations, and Modelling. [PDF]
Tziotziou K +14 more
europepmc +1 more source
Determining the Magnetic Field of Active Region Plages Using the Whole CLASP2/2.1 Spectral Window
The Chromospheric LAyer SpectroPolarimeter missions, CLASP2 and CLASP2.1, demonstrated that the near-UV spectral region between 279.30 and 280.68 nm is suitable for studying the magnetism of the solar chromosphere.
David Afonso Delgado +18 more
doaj +1 more source
Simulations of Magnetohydrodynamics and CO Formation from the Convection Zone to the Chromosphere
We present the results of simulations of the formation and the evolution of carbon monoxide (CO) and of magnetic fields in the solar atmosphere, extending from the upper convection zone to the middle chromosphere.
Sven Wedemeyer-Böhm +5 more
core
Transverse oscillations and an energy source in a strongly magnetized sunspot. [PDF]
Yuan D +14 more
europepmc +1 more source

