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The observation and analysis of stellar photospheres/
Published 1976Subjects: “…Stellar photospheres…”
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The observation and analysis of stellar photospheres /
Published 2005Subjects: “…Stellar photospheres…”
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Photospheric magnetic vortex structures
Published 2011-05-01“…Using direct numerical magneto-hydrodynamic (MHD) simulations, we demonstrate the evidence of two physically different types of vortex motions in the solar photosphere. Baroclinic motions of plasma in non-magnetic granules are the primary source of vorticity in granular regions of the solar photosphere, however, there is a significantly more efficient mechanism of vorticity production in strongly magnetised intergranular lanes. …”
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Solar and stellar photospheric abundances
Published 2016-07-01“…Abstract The determination of photospheric abundances in late-type stars from spectroscopic observations is a well-established field, built on solid theoretical foundations. …”
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On the Origin of the Photospheric Magnetic Field
Published 2022-01-01“…This article presents results that challenge the paradigms that (1) the convection zone is the source of the radial magnetic field in the photosphere and (2) that coronal currents are neutralized from the perspective of the photosphere. …”
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PMI: The Photospheric Magnetic Field Imager
Published 2020-01-01“…We describe the design and the capabilities of the Photospheric Magnetic field Imager (PMI), a compact and lightweight vector magnetograph, which is being developed for ESA’s Lagrange mission to the Lagrange L5 point. …”
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Quantifying Poynting Flux in the Quiet Sun Photosphere
Published 2023-01-01Subjects: Get full text
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Dynamic bifurcation for the granulation convection in the solar photosphere
Published 2017-08-01Subjects: Get full text
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Computation and analysis of flow patterns in the solar photosphere.
Published 2010Get full text
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Turbulence in a Coronal Loop Excited by Photospheric Motions
Published 2020-04-01“…Photospheric motions are believed to be the source of coronal heating and of velocity fluctuations detected in the solar corona. …”
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The role of photospheric converging motion in initiation of solar eruptions
Published 2022-10-01“…It is well-known that major solar eruptions are often produced by active regions with continual photospheric shearing and converging motions. Here, through high-accuracy magnetohydrodynamics simulation, we show how solar eruption is initiated in a single bipolar configuration as driven by first shearing and then converging motions at the bottom surface. …”
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DIFFERENT MODES OF TURBULENCE IN THE ACTIVE REGIONS OF THE SOLAR PHOTOSPHERE
Published 2013-11-01“…In work the range of different methods for the analysis of characteristics of turbulent processes in the active regions of the solar photosphere has been used. The changes of fluctuations distribution function and its moments were analyzed, spectral analysis was carried out. …”
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Deconstructing Photospheric Spectral Lines in Solar and Stellar Flares
Published 2024-01-01Subjects: Get full text
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The photospheric origin of the Yonetoku relation in gamma-ray bursts
Published 2019-04-01“…Here, Ito et al. show the reproduction of this relation in 3D hydrodynamical simulations followed by radiative transfer calculations, which suggest the photospheric emission is the dominant component in the prompt phase of GRBs.…”
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Novel Approach to Forecasting Photospheric Emergence of Active Regions
Published 2023-01-01“…We analyze the lower photospheric flow organization prior, during and following the rise of an active region, uncovering the repelling and attracting photospheric structures that act as sources and sinks for magnetic element transport. …”
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Prominence oscillations and stability - Communicating the distant photospheric boundary
Published 1997“…The photosphere provides an important boundary condition for prominence support. …”
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Testing the Steady-State Fluctuation Relation in the Solar Photospheric Convection
Published 2020-06-01Subjects: Get full text
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Changes in Photospheric Lorentz Force in Eruptive and Confined Solar Flares
Published 2024-01-01“…Solar flares are known to leave imprints on the magnetic field in the photosphere, often manifested as an abrupt and permanent change in the downward-directed Lorentz force in localized areas inside the active region. …”
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The Sun's Global Photospheric and Coronal Magnetic Fields: Observations and Models
Published 2012-11-01Subjects: Get full text
Article