Results 101 to 110 of about 3,072 (224)
The Bright Rim Prominences according to 2.5D Radiative Transfer
The Astrophysical Journal LettersSolar prominences observed close to the limb commonly include a bright feature that, from the perspective of the observer, runs along the interface between itself and the underlying chromosphere. Despite several idealized models being proposed to explain
Jack M. Jenkins +4 more
doaj +1 more source
Zero-Field Dichroism in the Solar Chromosphere
Physical Review Letters, 2003 We explain the linear polarization of the Ca II infrared triplet observed close to the edge of the solar disk. In particular, we demonstrate that the physical origin of the enigmatic polarizations of the 866.2 nm and 854.2 nm lines lies in the existence of atomic polarization in their metastable lower levels, which produces differential absorption of ...
Sainz, R. Manso, Bueno, J. Trujillo
openaire +3 more sources
Preferential Appearance of Hα Moreton Waves along Photospheric Magnetic Network Boundaries
The Astrophysical Journal LettersMoreton waves are rare chromospheric signatures of large-scale coronal disturbances, often associated with big flares and coronal mass ejections. Using high-cadence, full-disk H α spectroscopic observations from Chinese H α Solar Explorer, together with ...
C. H. Zhai +3 more
doaj +1 more source
The Non-Magnetic Solar Chromosphere [PDF]
, 2007 . We summarize recent results from self-consistent non-LTE radiation hydrodynamicssimulations of the propagation of acoustic waves through the non-magnetic solar chromosphere. References to more detailed write-ups of the work are given.
Mats Carlsson, Robert F. Stein
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The Gondola for the Sunrise iii Balloon-Borne Solar Observatory [PDF]
Publisher Copyright: © The Author(s) 2025.Sunrise iii is a balloon-borne solar observatory dedicated to investigating the physics governing the magnetism and dynamics in the lower solar atmosphere.
Korpi-Lagg, Andreas +24 more
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3-D hydrodynamic simulations of the solar chromosphere [PDF]
, 2020 . We present first results of three-dimensional numerical simulations of the non-magnetic solar chromosphere, computed with the radiation hydrodynamics code CO 5 BOLD.
B Freytag +4 more
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Determining the Magnetic Field of Active Region Plages Using the Whole CLASP2/2.1 Spectral Window
The Astrophysical JournalThe 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
Dynamics of the Quiet Solar Chromosphere [PDF]
, 1999 The solar chromosphere has never been static although it was often modeled so.Even the quiet-sun internetwork chromosphere has become thoroughly dynamic with the acoustic shock interpretation of the Ca II K 2V grains.
Rutten, R.J. +3 more
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Soft X-ray heating of the solar chromosphere during the gradual phase of two solar flares [PDF]
, 2004 In this paper we perform an analysis of the energetics of the solar flaring chromosphere irradiated by soft X-rays (SXR) emitted from overlying hot flare loops.
Berlicki, Arkadiusz +3 more
core +1 more source
ALFVÉN WAVE HEATING of the SOLAR CHROMOSPHERE: 1.5D MODELS [PDF]
, 2016 ALFVÉN WAVE HEATING of the SOLAR CHROMOSPHERE: 1.5D ...
Sergiy Shelyag (13094397) +2 more
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