Works matching DE "SOLAR magnetic fields"
Results: 1560
The rush to the poles and the role of magnetic buoyancy in the solar dynamo.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2025, v. 693, p. 1, doi. 10.1051/0004-6361/202450968
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The Sun at millimeter wavelengths: V. Magnetohydrodynamic waves in a fibrillar structure.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2025, v. 693, p. 1, doi. 10.1051/0004-6361/202451833
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Investigating explosive events in a 3D quiet-Sun model: Transition region and coronal response.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2025, v. 693, p. 1, doi. 10.1051/0004-6361/202450862
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Characterizing X‐ray activity cycles of young solar‐like stars with solar observations.
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- Astronomische Nachrichten, 2022, v. 343, n. 4, p. 1, doi. 10.1002/asna.20210066
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Rotation anomaly of the Sun.
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- Astronomische Nachrichten, 2020, v. 341, n. 6/7, p. 588, doi. 10.1002/asna.202013625
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Transfer learning in spatial–temporal forecasting of the solar magnetic field.
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- Astronomische Nachrichten, 2020, v. 341, n. 4, p. 384, doi. 10.1002/asna.202013690
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Cloud model inversions of strong chromospheric absorption lines using principal component analysis.
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- Astronomische Nachrichten, 2020, v. 341, n. 1, p. 64, doi. 10.1002/asna.202013652
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Investigating Chinese mathematical techniques to calculate sunrise and sunset times in Datongli.
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- Astronomische Nachrichten, 2018, v. 339, n. 6, p. 520, doi. 10.1002/asna.201813480
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Harmony of the solar system.
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- Astronomische Nachrichten, 2018, v. 339, n. 6, p. 513, doi. 10.1002/asna.201813475
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Small‐scale dynamos in simulations of stratified turbulent convection.
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- Astronomische Nachrichten, 2018, v. 339, n. 2/3, p. 127, doi. 10.1002/asna.201813477
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Solar Irradiance Models and Measurements: A Comparison in the 220-240 nm wavelength band.
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- Surveys in Geophysics, 2012, v. 33, n. 3/4, p. 475, doi. 10.1007/s10712-011-9166-7
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Total Solar Irradiance Observations.
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- Surveys in Geophysics, 2012, v. 33, n. 3/4, p. 453, doi. 10.1007/s10712-011-9168-5
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Effects of field line expansion on Alfvén waves and vortices.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 691, p. 1, doi. 10.1051/0004-6361/202451507
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Global and local dynamics of X-flare-producing active regions during solar cycle 25 peak phase.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 691, p. 1, doi. 10.1051/0004-6361/202451428
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Solar active region evolution and imminent flaring activity through color-coded visualization of photospheric vector magnetograms.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 691, p. 1, doi. 10.1051/0004-6361/202451393
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Testing the flux tube expansion factor: Solar wind speed relation with Solar Orbiter data.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 691, p. 1, doi. 10.1051/0004-6361/202451272
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Automated detection of exploding granules with SDO/HMI data.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 691, p. 1, doi. 10.1051/0004-6361/202451128
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Solar internetwork magnetic fields: Statistical comparison between observations and MHD simulations.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 691, p. 1, doi. 10.1051/0004-6361/202451079
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The mean solar butterfly diagram and poloidal field generation rate at the surface of the Sun.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 691, p. 1, doi. 10.1051/0004-6361/202450739
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High-resolution observations of recurrent jets from an arch filament system.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 691, p. 1, doi. 10.1051/0004-6361/202449715
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Spatially resolved plasma composition evolution in a solar flare – The effect of reconnection outflow.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 691, p. 1, doi. 10.1051/0004-6361/202449246
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Connectivity between the solar photosphere and chromosphere in a vortical structure: Observations of multi-phase, small-scale magnetic field amplification.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 691, p. 1, doi. 10.1051/0004-6361/202349081
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The extremely strong non-neutralized electric currents of the unique solar active region NOAA 13664.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202451627
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A search for mode coupling in magnetic bright points.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202451199
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Can we rely on EUV emission to identify coronal waveguides?
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202451196
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Reconstructing solar magnetic fields from historical observations: X. Effect of magnetic field inclination and boundary structure on AIA 1600 Å emission.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202451027
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Energy and helicity evolution in a flux emergence simulation.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202450924
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Derivation of a generalized Kappa distribution from the scaling properties of solar wind magnetic field fluctuations at kinetic scales.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202450714
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Directional discontinuities in the inner heliosphere from Parker Solar Probe and Solar Orbiter observations.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202450684
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Non-linear torsional Alfvén waves evolving in stratified viscous plasmas: Coronal hole plumes.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202450550
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Coronal magnetic field and emission properties of small-scale bright and faint loops in the quiet Sun.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202450343
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Magnetograms underestimate even unipolar magnetic flux nearly everywhere on the solar disk.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202450267
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Assessment of the near-Sun magnetic field of the 10 March 2022 coronal mass ejection observed by Solar Orbiter.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202450204
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Variation in the polarity separation of sunspot groups throughout their evolution.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202450194
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Charge sign dependence of recurrent Forbush decreases in 2016–2017.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202449836
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Dependence of coronal mass ejections on the morphology and toroidal flux of their source magnetic flux ropes.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202449731
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High-resolution observations of two pores with the integral field unit (IFU) of the GREGOR Infrared Spectrograph (GRIS).
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202347571
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Magnetic field diagnostics of prominences with the Mg II k line 3D Stokes inversions versus traditional methods.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 689, p. 1, doi. 10.1051/0004-6361/202450743
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Unexpected frequency of horizontal oscillations of magnetic structures in the solar photosphere.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 687, p. 1, doi. 10.1051/0004-6361/202450693
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Horizontally and vertically polarized kink oscillations in curved solar coronal loops.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 687, p. 1, doi. 10.1051/0004-6361/202449991
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Filament eruption by multiple reconnections.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 687, p. 1, doi. 10.1051/0004-6361/202449774
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Combining magneto-hydrostatic constraints with Stokes profile inversions: IV. Imposing ∇⋅B = 0 condition.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 687, p. 1, doi. 10.1051/0004-6361/202449572
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Extreme-ultraviolet (EUV) observables of simulated plasmoid-mediated reconnection in the solar corona.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 687, p. 1, doi. 10.1051/0004-6361/202449357
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The MODEST catalog of depth-dependent spatially coupled inversions of sunspots observed by Hinode/SOT-SP.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 687, p. 1, doi. 10.1051/0004-6361/202449269
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Impact of far-side structures observed by Solar Orbiter on coronal and heliospheric wind simulations.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 687, p. 1, doi. 10.1051/0004-6361/202349040
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Transition to a weaker Sun: Changes in the solar atmosphere during the decay of the Modern Maximum.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 685, p. 1, doi. 10.1051/0004-6361/202449231
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Comparison of magnetic data products from Solar Orbiter SO/PHI-FDT and SDO/HMI.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 685, p. 1, doi. 10.1051/0004-6361/202349096
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Improved reconstruction of solar magnetic fields from imaging spectropolarimetry through spatio-temporal regularisation.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 685, p. 1, doi. 10.1051/0004-6361/202348810
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A magnetic reconnection model for the hot explosion with both ultraviolet and Hα wing emissions.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 685, p. 1, doi. 10.1051/0004-6361/202347012
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Magnetochronology of solar-type star dynamos.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 684, p. 1, doi. 10.1051/0004-6361/202347939
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