Results 121 to 130 of about 5,669 (225)

Magnetic Field Stratification in Active-region Plage from Ca ii K and Ca ii 8542 Å Spectropolarimetry

open access: yesThe Astrophysical Journal Letters
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

Measuring the magnetic fields in the chromospheres of low-mass stars. [PDF]

open access: yesNat Commun
Cang T   +13 more
europepmc   +2 more sources

Constraints on Acoustic Wave Energy Fluxes and Radiative Losses in the Solar Chromosphere from Non-LTE Inversions

open access: yesThe Astrophysical Journal
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

open access: yesThe Astrophysical Journal
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]

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

Determining the Magnetic Field of Active Region Plages Using the Whole CLASP2/2.1 Spectral Window

open access: yesThe Astrophysical Journal
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

open access: yes, 2020
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]

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

Home - About - Disclaimer - Privacy