Results 131 to 140 of about 14,496 (257)
Near-ultraviolet Spectropolarimetry as a Tracer of Magnetic Markers of Flux Rope Formation
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
Effects of Ion Magnetization on the Farley–Buneman Instability in the Solar Chromosphere [PDF]
Alex Fletcher +3 more
openalex +1 more source
Structure of sunspot light bridges in the chromosphere and transition region
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 HARD X-RAY SOURCE SIZES IN A BEAM-HEATED AND IONIZED CHROMOSPHERE [PDF]
Aidan O’Flannagain +2 more
openalex +1 more source
Solar Flare Ribbon Fronts. II. Evolution of Heating Rates in Individual Flare Footpoints
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
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]
G. Cauzzi +4 more
openalex +1 more source
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
Observations of the upper solar chromosphere with SUMER [PDF]
K. Wilhelm, W. Kalkofen
openalex +1 more source

