Results 131 to 140 of about 14,496 (257)

Near-ultraviolet Spectropolarimetry as a Tracer of Magnetic Markers of Flux Rope Formation

open access: yesThe Astrophysical Journal
We investigate the suitability of the combined spectral windows of Mg ii h and k and the Fe ii lines around 261 nm as magnetic markers of filament formation.
David Afonso Delgado   +3 more
doaj   +1 more source

Structure of sunspot light bridges in the chromosphere and transition region

open access: yes, 2017
Light bridges (LBs) are elongated structures with enhanced intensity embedded in sunspot umbra and pores. We studied the properties of a sample of 60 LBs observed with the Interface Region Imaging Spectrograph (IRIS). Using IRIS near- and far-ultraviolet
Rezaei, Reza
core   +1 more source

Solar Flares and the Chromosphere

open access: yes, 2010
5 pages, 3 ...
Fletcher, L.   +6 more
openaire   +2 more sources

SOLAR HARD X-RAY SOURCE SIZES IN A BEAM-HEATED AND IONIZED CHROMOSPHERE [PDF]

open access: bronze, 2015
Aidan O’Flannagain   +2 more
openalex   +1 more source

Solar Flare Ribbon Fronts. II. Evolution of Heating Rates in Individual Flare Footpoints

open access: yesThe Astrophysical Journal
Solar flare ribbon fronts appear ahead of the bright structures that normally characterize solar flares, and can persist for an extended period of time in spatially localized patches before transitioning to “regular” bright ribbons. They likely represent
Graham S. Kerr   +3 more
doaj   +1 more source

Comparison between variations in solar UV radiation and sunspot parameters with Mg II daily index as a proxy

open access: yesPhysics Open
Solar UV radiation influence the Earth's climate and upper atmosphere. The UV emission from the Sun modulates with the sunspot cycle with an 11-year periodicity.
(G) Chandrika   +2 more
doaj   +1 more source

The solar chromosphere at high resolution with IBIS [PDF]

open access: bronze, 2009
G. Cauzzi   +4 more
openalex   +1 more source

Solar Chromospheric Heating by Magnetohydrodynamic Waves: Dependence on the Inclination of the Magnetic Field

open access: yesThe Astrophysical Journal
A proposed mechanism for solar chromospheric heating is magnetohydrodynamic waves propagating upward along magnetic field lines and dissipating their energy in the chromosphere.
Mayu Koyama, Toshifumi Shimizu
doaj   +1 more source

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