Extreme-Ultraviolet Emission from Solar Prominences
The Astrophysical Journal, 1972 Spectra and spectroheliograms of prominences have been obtained at wavelengths of 300 to 1400 A from instruments aboard the OSO 4 and OSO 6 spacecraft. Quiescent prominences appear in emission above the limb for all strong lines formed at temperatures below 300,000 K, but not at higher temperatures.
R. W. Noyes +5 more
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Explosive events in the solar atmosphere seen in extreme-ultraviolet emission lines [PDF]
Astronomy & Astrophysics, 2005 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
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Measurements of extreme-ultraviolet emission-line profiles near the solar limb
The Astrophysical Journal, 1978 Line profiles of optically thin extreme-ultraviolet emission lines observed in a quiet sun region at positions within and above the white-light limb with the NRL slit spectrograph (S082-B) on Skylab are discussed. Absolute line intensities and full widths at half-maximum are presented for lines formed over the temperature range from about 10,000 to 22 ...
J. T. Mariska, U. Feldman, G. A. Doschek
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Radiative Hydrodynamic Models of the Optical and Ultraviolet Emission from Solar Flares [PDF]
The Astrophysical Journal, 2005 We report on radiative hydrodynamic simulations of moderate and strong solar flares. The flares were simulated by calculating the atmospheric response to a beam of non-thermal electrons injected at the apex of a one-dimensional closed coronal loop, and include heating from thermal soft X-ray, extreme ultraviolet and ultraviolet (XEUV) emission.
Allred, J. C. +3 more
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Rocket Observations of Profiles of Solar Ultraviolet Emission Lines
The Astrophysical Journal, 1969 E. C., Jr. Bruner, W. A. Rense
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The Ultraviolet Emission Spectrum of the Solar Chromosphere and Corona [PDF]
Monthly Notices of the Royal Astronomical Society, 1967 W. M. Burton, A. Ridgeley, R. Wilson
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Coronal Microjets in Quiet-Sun Regions Observed with the Extreme Ultraviolet Imager on Board the Solar Orbiter [PDF]
Astrophysical Journal Letters, 2021 We report the smallest coronal jets ever observed in the quiet Sun with recent high-resolution observations from the High Resolution Telescopes (HRIEUV and HRILyα ) of the Extreme Ultraviolet Imager on board the Solar Orbiter (SO).
Zhenyong Hou +10 more
semanticscholar +1 more source
Emission-Line Intensities in the Solar Ultraviolet.
The Astrophysical Journal, 1959 A. Aboud, W. E. Behring, W. A. Rense
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Proxy-based Prediction of Solar Extreme Ultraviolet Emission Using Deep Learning [PDF]
The Astrophysical Journal Letters, 2021 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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Image Super-resolution Methods for FY-3E X-EUVI 195 Å Solar Images
The Astrophysical Journal Supplement Series, 2023 Solar eruptions and the solar wind are sources of space weather disturbances, and extreme-ultraviolet (EUV) observations are widely used to research solar activity and space weather forecasts.
Qinglin Yang +4 more
doaj +1 more source