Results 11 to 20 of about 2,606 (253)
Solar Emission Lines in the Extreme Ultraviolet.
T. Violett, William A. Rense
exaly +2 more sources
Identification of Extreme Ultraviolet Solar Emission Lines.
Harold Zirin
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Proxy-based Prediction of Solar Extreme Ultraviolet Emission Using Deep Learning [PDF]
Abstract High-energy radiation from the Sun governs the behavior of Earth’s upper atmosphere and such radiation from any planet-hosting star can drive the long-term evolution of a planetary atmosphere. However, much of this radiation is unobservable because of absorption by Earth’s atmosphere and the interstellar medium.
Anthony Pineci +3 more
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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
Abstract The hydrogen Lyα (H i Lyα) emission during solar flares has rarely been studied in spatially resolved images, and its physical origin has not been fully understood. In this paper, we present novel Lyα images for a C1.4 solar flare (SOL2021-08-20T22:00) from the Extreme Ultraviolet Imager aboard Solar Orbiter, together with multi-
Y. Li +9 more
openaire +5 more sources
Explosive events in the solar atmosphere seen in extreme-ultraviolet emission lines [PDF]
We present observations of explosive events (EEs) in the solar atmosphere obtained with the Solar Ultraviolet Measurements of Emitted Radiation (SUMER) spectrometer on the Solar and Heliospheric Observatory (SOHO) in the wavelength range from about 750 A to 790 A.
Mendoza-Torres, J. +2 more
openaire +2 more sources
A Model for Gradual-phase Heating Driven by MHD Turbulence in Solar Flares
Coronal flare emission is commonly observed to decay on timescales longer than those predicted by impulsively driven, one-dimensional flare loop models.
William Ashfield IV, Dana Longcope
doaj +1 more source
Impulsive extreme-ultraviolet and hard X-ray emission during solar flares
S R Kane
exaly +2 more sources
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
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The propagation direction and true velocity of a solar coronal mass ejection, which are among the most decisive factors for its geo-effectiveness, are difficult to determine through single-perspective imaging observations. Here we show that Sun-as-a-star
Yu Xu +5 more
doaj +1 more source

