Results 91 to 100 of about 938 (183)
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
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
SUTO-Solar Through-Turbulence Open Image Dataset. [PDF]
Popowicz A, Orlov V.
europepmc +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
Mapping solar magnetic fields from the photosphere to the base of the corona. [PDF]
Ishikawa R +27 more
europepmc +1 more source
The Sun as a driver of the inner heliosphere: Modern investigations of fundamental plasma processes. [PDF]
Ervin T, Nakhleh AJ, Bharati Das S.
europepmc +1 more source
Magnetic activity and spectral behavior of RS CVn binary system (IM Pegasi) in the ultraviolet. [PDF]
Sanad MR, Rahman HIA, Badawy WA.
europepmc +1 more source
Excitation of Chromospheric Emission [PDF]
openaire +1 more source
Spectroscopic Analysis and RHD Modeling of the First Ca II H and H ϵ Flare Spectra from DKIST/ViSP. [PDF]
Tamburri C +9 more
europepmc +1 more source
Temperature Gradients in the Chromosphere
R. G. Athay, R. N. Thomas
openaire +1 more source

