Results 171 to 180 of about 18,154 (212)

Radiative plasma simulations of black hole accretion flow coronae in the hard and soft states. [PDF]

Nat Commun
Nättilä J.
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Psoriasis and Seasonality: Exploring the Genetic and Epigenetic Interactions. [PDF]

Int J Mol Sci
Niedźwiedź M, Skibińska M, Ciążyńska M, Noweta M, Czerwińska A, Krzyścin J, Narbutt J, Lesiak A.   +7 more
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Detection of disk-jet coprecession in a tidal disruption event. [PDF]

Sci Adv
Wang Y, Lin Z, Wu L, Lei WH, Wei S, Zhang SN, Ji L, Del Palacio S, Baldi RD, Huang Y, Liu JF, Zhang B, Yang A, Chen RR, Zhang Y, Wang AL, Yang L, Charalampopoulos P, Williams-Baldwin DRA, Yao ZH, Xie FG, Bu D, Feng H, Cao X, Wu H, Li W, Qiao E, Leloudas G, Anderson JP, Shu X, Pasham DR, Zou H, Nicholl M, Wevers T, Müller-Bravo TE, Wang J, Wei JY, Qiu YL, Guo WJ, Gutiérrez CP, Gromadzki M, Inserra C, Makrygianni L, Onori F, Petrushevska T, Altamirano D, Galbany L, Peréz-Torres M, Chen TW.   +48 more
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Mapping the Sun's coronal magnetic field using the Zeeman effect. [PDF]

Sci Adv
Schad TA, Petrie GJD, Kuhn JR, Fehlmann A, Rimmele T, Tritschler A, Woeger F, Scholl I, Williams R, Harrington D, Paraschiv AR, Szente J.   +11 more
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X-ray Spectra from Solar Flares by Yohkoh Satellite

X-ray Spectra from Solar Flares by Yohkoh Satellite
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Solar flare pulsation spectra

2022
Таврический астрофизический журнал, Выпуск 3 (2) 2022, Pages 17 ...
Kupryakov, Yu.A., Gorshkov, A.B., Kashapova, L.K.   +2 more
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Solar flare high-energy electron spectra

Solar Physics, 1992
It is shown that the solar flare electron spectra in a large energy range fit well with a power law in energy. This is used as a basis to discuss the possible division of solar flares into various groups, and also to compare the spectra of electrons in interplanetary space and at the flare site.
D. Heristchi, T. Amari
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Cyclotron lines in the spectra of solar flares and solar active regions

Solar Physics, 1989
AbstractIt was shown by Zheleznyakov and Zlotnik (1980a, b) that in complex configurations of solar magnetic fields (in hot loops above the active centres, in neutral current sheets in the preflare phase, in hot X-ray kernels in the initial flare phase) a system of cyclotron lines in the spectrum of microwave radiation is likely to be formed.
V. V. Zheleznyakov, E. Ya. Zlotnik
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Spectra of solar flares from 8.5 � to 16 �

Solar Physics, 1973
X-ray spectra of solar flares in the spectral range from 8.5 A to ∼ 16 A have been obtained from a Naval Research Laboratory crystal spectrometer flown on the sixth Orbiting Solar Observatory (OSO-6). A list of emission features is presented and tentative identifications of some of the features are suggested.
G. A. Doschek, J. F. Meekins, Robert D. Cowan   +2 more
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Spectra of Solar Flares

Annual Review of Astronomy and Astrophysics, 1972
Solar flares emit electromagnetic radiation within a very broad range of wavelengths, from 0.02 A (2 X 10-10 cm) up to more than 600 m (6X 104 cm). This may be continuous emission in some parts of the spectrum, line emission in others, or a combination of both.
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