Results 91 to 100 of about 938 (183)

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

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

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

Mapping solar magnetic fields from the photosphere to the base of the corona. [PDF]

open access: yesSci Adv, 2021
Ishikawa R   +27 more
europepmc   +1 more source

Excitation of Chromospheric Emission [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 1956
openaire   +1 more source

Spectroscopic Analysis and RHD Modeling of the First Ca II H and H ϵ Flare Spectra from DKIST/ViSP. [PDF]

open access: yesSol Phys
Tamburri C   +9 more
europepmc   +1 more source

Temperature Gradients in the Chromosphere

open access: yesPublications of the Astronomical Society of the Pacific, 1955
R. G. Athay, R. N. Thomas
openaire   +1 more source

Home - About - Disclaimer - Privacy