Results 1 to 10 of about 18,115 (177)
Validation of computed extreme ultraviolet emission spectra during solar flares [PDF]
X-rays and extreme ultraviolet (EUV) emissions from solar flares rapidly change the physical composition of the Earth’s thermosphere and ionosphere, thereby causing space weather phenomena such as communication failures.
Shohei Nishimoto +4 more
doaj +2 more sources
Muon and Tau Neutrinos Spectra from Solar Flares [PDF]
Solar neutrino flares and mixing are considered. Most power-full solar flare as the ones occurred on 23th February 1956, September 29th 1989, 28th October and on 2nd-4th November 2003 are sources of cosmic rays, X, gamma and neutrino bursts. These flares
Bodek A. +9 more
core +3 more sources
An investigation of Fe XV emission lines in solar flare spectra [PDF]
Previously, large discrepancies have been found between theory and observation for Fe XV emission line ratios in solar flare spectra covering the 224-327 A wavelength range, obtained by the Naval Research Laboratory's S082A instrument on board Skylab ...
Aggarwal, K M +4 more
core +2 more sources
Investigating the Soft X-Ray Spectra of Solar Flare Onsets
In this study, we present the analysis of six solar flare events that occurred in 2022, using new data from the third-generation Miniature X-Ray Solar Spectrometer, also known as the Dual-zone Aperture X-ray Solar Spectrometer (DAXSS).
Anant Telikicherla +2 more
doaj +3 more sources
Analysis of Solar-like X-class Flare on Wolf 359 Observed Simultaneously with TESS and XMM-Newton
We present an analysis of a flare on the Wolf 359 star based on simultaneous observations of Transiting Exoplanet Survey Satellite and XMM-Newton. A stellar flare with energy comparable to an X-class solar flare is analyzed on this star for the first ...
M. Pietras +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
Element abundances from solar flare spectra [PDF]
Rapport d'abondances de Ar/Ca, K/Ca et Ca/Fe d'apres des spectres RX a haute resolution d'eruptions solaires obtenus par le satellite P78 ...
G. A. Doschek, U. Feldman, J. F. Seely
openaire +1 more source
Solar flares as proxy for the young Sun: satellite observed thermosphere response to an X17.2 flare of Earth's upper atmosphere [PDF]
We analyzed the measured thermospheric response of an extreme solar X17.2 flare that irradiated the Earth's upper atmosphere during the so-called Halloween events in late October/early November 2003.
S. Krauss +11 more
doaj +1 more source
The Transition Region of Solar Flare Loops
The transition region between the Sun’s corona and chromosphere is important to the mass and energy transfer from the lower atmosphere to the corona; consequently, this region has been studied intensely with ultraviolet and extreme ultraviolet (EUV ...
Costis Gontikakis +2 more
doaj +1 more source
Quasi-periodic pulsation (QPP) is a common phenomenon in solar flares. Studying QPP is important to further our understanding of the physical processes operating in flares.
Yangfan Guo +6 more
doaj +1 more source

