Results 21 to 30 of about 155,544 (195)
Impulsive Hard X-Ray and Ultraviolet Emission during Solar Flares
S. R. Kane, R. F. Donnelly
openaire +2 more sources
The CHIANTI atomic database provides sets of assessed data that are used for simulating spectral observations of astrophysical plasmas. This article describes updates that will be released as version 10.1 of the database.
Kenneth P. Dere +3 more
doaj +1 more source
Further Measurements of Emission Line Profiles in the Solar Ultraviolet Spectrum [PDF]
B. C. Boland +8 more
openaire +2 more sources
Ultraviolet Emission Lines in the Solar Spectrum.
W. E. Behring +2 more
openaire +2 more sources
The \begin{document}$ {\rm{CO}}_2^+$\end{document} ultraviolet doublet (UVD) emission near 289 nm is an important feature of dayside airglow emission from planetary upper atmospheres. In this study, we analyzed the brightness profiles of \begin{document}$
ZiChuan Li +5 more
doaj +1 more source
Statistical analysis for EUV dynamic spectra and their impact on the ionosphere during solar flares
The X-rays and extreme ultraviolet (EUV) emitted during solar flares can rapidly change the physical composition of Earth’s ionosphere, causing space weather phenomena.
Shohei Nishimoto +9 more
doaj +1 more source
Radiation Pressure Acting on the Neutral He Atoms in the Heliosphere
Interstellar neutral helium (ISN He) is an important source of information on the physical state of the local interstellar medium. Radiation pressure acting on the neutral helium atoms in the heliosphere has always been neglected; its effect has been ...
I. Kowalska-Leszczynska +2 more
doaj +1 more source
Solar Ultraviolet Bursts [PDF]
The term “ultraviolet (UV) burst” is introduced to describe small, intense, transient brightenings in ultraviolet images of solar active regions. We inventorize their properties and provide a definition based on image sequences in transition-region lines.
P. Young +18 more
semanticscholar +1 more source
The Role of Magnetic Shear in Reconnection-driven Flare Energy Release
Using observations from the Solar Dynamics Observatory’s Atmosphere Imaging Assembly and the Ramaty High Energy Solar Spectroscopic Imager, we present novel measurements of the shear of post-reconnection flare loops (PRFLs) in SOL20141218T21:40 and study
J. Qiu +8 more
doaj +1 more source
INTENSITY ENHANCEMENT OF O vi ULTRAVIOLET EMISSION LINES IN SOLAR SPECTRA DUE TO OPACITY [PDF]
Opacity is a property of many plasmas. It is normally expected that if an emission line in a plasma becomes optically thick, then its intensity ratio to that of another transition that remains optically thin should decrease.
F. Keenan +8 more
semanticscholar +1 more source

