Results 21 to 30 of about 1,066 (184)
Turbulence in the Solar Photosphere [PDF]
Space Science Reviews, 2001 16 pages, 1 ...
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Atomic data and the spectrum of the solar photosphere [PDF]
Physica Scripta, 1993 Even though the solar photospheric abundances are now on the whole in very good agreement with the meteoritic values, some problems remain which will only be solved with a higher level of accuracy in the atomic data, especially the transition probabilities for faint lines.
Grevesse, Nicolas +1 more
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The Astrophysical Journal, 2023 Observations show that there are twisted magnetic flux tubes and plasma flow throughout the solar atmosphere. The main purpose of this work is to obtain the damping rate of sausage modes in the presence of magnetic twist and plasma flow.
Mohammad Sadeghi +2 more
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Latitudinal Variation of the Solar Photospheric Intensity [PDF]
The Astrophysical Journal, 2008 24 pages, 8 figs, accepted in ...
Rast, Mark P. +2 more
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STOCHASTIC COUPLING OF SOLAR PHOTOSPHERE AND CORONA [PDF]
The Astrophysical Journal, 2013 36 pageS, 11 figures, 3 ...
Uritsky, Vadim M. +3 more
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The Astrophysical JournalWe report and discuss the phase shift and phase travel time of low-frequency ( ν < 5.0 mHz) acoustic waves estimated within the photosphere and photosphere–chromosphere interface regions, utilizing multiheight velocities in the quiet Sun.
Hirdesh Kumar +4 more
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Solar and stellar photospheric abundances
Living Reviews in Solar Physics, 2016 The determination of photospheric abundances in late-type stars from spectroscopic observations is a well-established field, built on solid theoretical foundations. Improving those foundations to refine the accuracy of the inferred abundances has proven challenging, but progress has been made.
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MAGNETOHYDRODYNAMICS OF THE WEAKLY IONIZED SOLAR PHOTOSPHERE [PDF]
The Astrophysical Journal, 2012 We investigate the importance of ambipolar diffusion and Hall currents for high-resolution comprehensive ('realistic') photospheric simulations. To do so we extended the radiative magnetohydrodynamics code \emph{MURaM} to use the generalized Ohm's law under the assumption of local thermodynamic equilibrium.
Cheung, M., Cameron, R.
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Type‐III Solar Radio Bursts at Mars: A 16.5‐Year Catalog From Mars Express‐MARSIS at 0.1–5.5 MHz
Space Weather, Volume 24, Issue 10, October 2026.Abstract The most intense radio feature in the Solar System are the solar Type‐III radio bursts, which are associated with electron beams that propagate along open magnetic field lines. Although solar radio bursts have been studied since the 1940s, observations remain mainly restricted within 1 AU.
Beatriz Sánchez‐Cano +22 more
wiley +1 more source
A High-resolution, Inversion-based Synoptic Study of Solar Granulation
The Astrophysical JournalThe convectively driven, weakly magnetized regions of the solar photosphere dominate the Sun’s surface at any given time, but the temporal variations of these quiet regions of the photosphere throughout the solar cycle are still not well known.
James W. Crowley +3 more
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