X‐Ray–fluorescent Fe Kα Lines from Stellar Photospheres [PDF]
J. J. Drake +2 more
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Solar filaments are believed to be a clump of cold plasma accumulated in the magnetic dips. However, the magnetic configuration of filaments and the key factors for their formation remains elusive.
Haitang Li +9 more
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Case Studies on Pre-eruptive X-class Flares using R-value in the Lower Solar Atmosphere
The R -value is a measure of the strength of photospheric magnetic polarity inversion lines in active regions (ARs). This work investigates the possibility of a relation between R -value variations and the occurrence of X-class flares in ARs, not in the ...
Shreeyesh Biswal +5 more
doaj +1 more source
MODELING THE ROSSITER–MCLAUGHLIN EFFECT: IMPACT OF THE CONVECTIVE CENTER-TO-LIMB VARIATIONS IN THE STELLAR PHOTOSPHERE [PDF]
H. M. Cegla +5 more
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The Physical Natures of Class I and Flat-Spectrum Protostellar Photospheres: A Near-Infrared Spectroscopic Study [PDF]
Greg Doppmann +3 more
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Radiation Spectrum of the Photospheric Emission for a Turbulent Relativistic Jet
The prompt gamma rays of gamma-ray bursts (GRBs) may originate from the photosphere of a relativistic jet. However, only a few GRBs have been observed with evident blackbody-like emission, for example, GRB 090902B.
Guo-Yu Li +3 more
doaj +1 more source
Magnetic power spectrum in the undisturbed solar photosphere
V. I. Abramenko, Olga K. Kutsenko
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Erratum: "Making the Corona and the Fast Solar Wind: A Self-consistent Simulation for the Low-Frequency Alfvén Waves from Photosphere to 0.3 AU" ([URL ADDRESS="/cgi-bin/resolve?2005ApJ...632L..49S" STATUS="OKAY"]ApJ, 632, L49 [2005][/URL]) [PDF]
Takeru K. Suzuki, Shu‐ichiro Inutsuka
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Turbulent convection as a significant hidden provider of magnetic helicity in solar eruptions. [PDF]
Toriumi S, Hotta H, Kusano K.
europepmc +1 more source
On the Dipole-Like Progressive Wave in the Photosphere [PDF]
I. K. Csada
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