Works matching Solar granulation
Results: 214
Acoustic wave propagation through solar granulation: Validity of effective-medium theories, coda waves.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2020, v. 643, p. 1, doi. 10.1051/0004-6361/202039201
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- Article
Latitude dependence of the solar granulation during the minimum of activity in 2009.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2017, v. 598, p. 1, doi. 10.1051/0004-6361/201527736
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Two-dimensional spectroscopic time series of solar granulation.
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- Solar Physics, 2004, v. 223, n. 1/2, p. 13, doi. 10.1007/s11207-004-1226-4
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- Article
Structure of the Long-Living Elements of Solar Granulation.
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- Kinematics & Physics of Celestial Bodies, 2018, v. 34, n. 1, p. 13, doi. 10.3103/S0884591318010026
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- Article
On 2D radiative transfer in solar granulation. The case of Fe I lines.
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- Astrophysics & Space Science, 2008, v. 318, n. 1/2, p. 93, doi. 10.1007/s10509-008-9904-6
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- Article
Dynamics of Granulation Convection in the Solar Photosphere Near the Equator.
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- Journal of Nonlinear Mathematical Physics, 2025, v. 32, n. 1, p. 1, doi. 10.1007/s44198-024-00255-4
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- Article
Does the solar granulation change with the activity cycle?
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2018, v. 616, p. 1, doi. 10.1051/0004-6361/201732085
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Convection structure in the solar photosphere at granulation and mesogranulation scales.
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- Kinematics & Physics of Celestial Bodies, 2015, v. 31, n. 2, p. 65, doi. 10.3103/S0884591315020026
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- Article
Specifics of the solar photospheric convection at granulation, mesogranulation, and supergranulation scales.
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- Kinematics & Physics of Celestial Bodies, 2014, v. 30, n. 4, p. 173, doi. 10.3103/S0884591314040023
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Mesostructure of the Solar Granulation.
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- Astronomy Letters, 2000, v. 26, n. 3, p. 192, doi. 10.1134/1.20381
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Data compression for local correlation tracking of solar granulation.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2016, v. 587, p. 1, doi. 10.1051/0004-6361/201526805
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- Article
Effects of granulation on the visibility of solar oscillations.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2015, v. 580, p. 1, doi. 10.1051/0004-6361/201526445
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- Article
Stellar Turbulent Convection: The Multiscale Nature of the Solar Magnetic Signature.
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- Atmosphere, 2021, v. 12, n. 8, p. 938, doi. 10.3390/atmos12080938
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- Article
Do Long-Lived Features Really Exist in the Solar Photosphere? II. Contrast of Time-Averaged Granulation Images.
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- Solar Physics, 2008, v. 249, n. 2, p. 307, doi. 10.1007/s11207-008-9146-3
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- Article
Spatial variations of Stokes profiles of magnetoactive lines Fe I.
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- Kinematics & Physics of Celestial Bodies, 2014, v. 30, n. 6, p. 261, doi. 10.3103/S0884591314060075
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- Article
Magnetic field effect on the fine structure of convective motions in the solar atmosphere.
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- Kinematics & Physics of Celestial Bodies, 2012, v. 28, n. 4, p. 155, doi. 10.3103/S0884591312040034
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- Article
Structure of the solar photosphere studied from the radiation hydrodynamics code ANTARES.
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- Astrophysics & Space Science, 2017, v. 362, n. 9, p. 1, doi. 10.1007/s10509-017-3151-7
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Is the sky the limit?: Performance of the revamped Swedish 1-m Solar Telescope and its blue- and red-beam reimaging systems.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 626, p. 1, doi. 10.1051/0004-6361/201935735
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- Article
Measurement of Astronomical Seeing Using Long Exposure Solar Images.
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- Solar Physics, 2019, v. 294, n. 1, p. 1, doi. 10.1007/s11207-019-1393-y
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Do Quasi-Regular Structures Really Exist in the Solar Photosphere? I. Observational Evidence.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 93, doi. 10.1007/s11207-006-0231-1
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Multifractal Analysis Of Solar Magnetograms.
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- Solar Physics, 2005, v. 228, n. 1/2, p. 29, doi. 10.1007/s11207-005-3525-9
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Structure Properties of Supergranulation and Granulation.
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- Solar Physics, 2004, v. 221, n. 1, p. 33, doi. 10.1023/B:SOLA.0000033368.00217.de
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Reduction of interpolation errors when using local correlation tracking for motion detection.
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- Solar Physics, 2003, v. 217, n. 1, p. 69, doi. 10.1023/A:1027322016500
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NUMERICAL SIMULATIONS OF SOLAR AND STELLAR CONVECTION USING THE ANTARES CODE.
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- EAS Publications Series, 2010, v. 44, p. 97, doi. 10.1051/eas/1044016
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NUMERICAL SIMULATIONS OF STELLAR SURFACE CONVECTION AND RELATED PHENOMENA.
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- EAS Publications Series, 2008, v. 28, p. 9, doi. 10.1051/eas:0828002
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- Article
Dynamic bifurcation for the granulation convection in the solar photosphere.
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- Boundary Value Problems, 2017, v. 2017, n. 1, p. 1, doi. 10.1186/s13661-017-0842-5
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The Sun at small scales.
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- Nature, 1998, v. 396, n. 6707, p. 114, doi. 10.1038/24044
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Solar Surface Convection.
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- Living Reviews in Solar Physics, 2009, v. 6, n. 2, p. 1
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HEIGHT OF THE GRANULATION CONTRAST INVERSION LAYER DERIVED FROM A CROSS-CORRELATION METHOD.
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- EAS Publications Series, 2012, v. 55, p. 79, doi. 10.1051/eas/1255010
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Plasma properties and Stokes profiles during the lifetime of a photospheric magnetic bright point.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2014, v. 566, p. 1, doi. 10.1051/0004-6361/201322882
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- Article
Two-dimensional segmentation of small convective patterns in radiation hydrodynamics simulations.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2014, v. 563, p. 1, doi. 10.1051/0004-6361/201321601
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Modelling of solar granulation.
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- Proceedings of the International Astronomical Union, 2006, v. 2, n. S239, p. 89, doi. 10.1017/S1743921307000208
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Contrast of time-averaged images of the solar granulation.
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- Proceedings of the International Astronomical Union, 2004, v. 2004, n. IAUS223, p. 231, doi. 10.1017/S174392130400568X
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- Article
Magnetic Field as a Tracer for Studying the Differential Rotation of the Solar Corona.
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- Solar Physics, 2018, v. 293, n. 9, p. 1, doi. 10.1007/s11207-018-1349-7
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- Article
Peculiarity of the Oscillation Stratification in Sunspot Penumbrae.
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- Solar Physics, 2016, v. 291, n. 11, p. 3339, doi. 10.1007/s11207-016-0953-7
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Properties of Magnetic Tongues over a Solar Cycle.
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- Solar Physics, 2016, v. 291, n. 6, p. 1625, doi. 10.1007/s11207-016-0926-x
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Using the WSA Model to Test the Parker Spiral Approximation for SEP Event Magnetic Connections.
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- Solar Physics, 2016, v. 291, n. 6, p. 1829, doi. 10.1007/s11207-016-0934-x
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Evolution of Small-Scale Magnetic Elements in the Vicinity of Granular-Sized Swirl Convective Motions.
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- Solar Physics, 2015, v. 290, n. 2, p. 301, doi. 10.1007/s11207-014-0626-3
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Spatio-Temporal Scaling of Turbulent Photospheric Line-of-Sight Magnetic Field in Active Region NOAA 11158.
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- Solar Physics, 2015, v. 290, n. 2, p. 335, doi. 10.1007/s11207-014-0636-1
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The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: SHARPs - Space-Weather HMI Active Region Patches.
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- Solar Physics, 2014, v. 289, n. 9, p. 3549, doi. 10.1007/s11207-014-0529-3
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The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: Overview and Performance.
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- Solar Physics, 2014, v. 289, n. 9, p. 3483, doi. 10.1007/s11207-014-0516-8
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The Quest to Understand Supergranulation and Large-Scale Convection in the Sun.
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- Solar Physics, 2014, v. 289, n. 9, p. 3403, doi. 10.1007/s11207-014-0471-4
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Additional Evidence Supporting a Model of Shallow, High-Speed Supergranulation.
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- Solar Physics, 2014, v. 289, n. 9, p. 3421, doi. 10.1007/s11207-014-0537-3
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Photospheric Magnetic Field: Relationship Between North-South Asymmetry and Flux Imbalance.
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- Solar Physics, 2014, v. 289, n. 8, p. 2845, doi. 10.1007/s11207-014-0512-z
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- Article
Tracking Back the Solar Wind to Its Photospheric Footpoints from Wind Observations - A Statistical Study.
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- Solar Physics, 2014, v. 289, n. 8, p. 3109, doi. 10.1007/s11207-014-0508-8
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Time-Series Analysis of Supergranule Characteristics at Solar Minimum.
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- Solar Physics, 2014, v. 289, n. 4, p. 1101, doi. 10.1007/s11207-013-0383-8
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Active Regions with Superpenumbral Whirls and Their Subsurface Kinetic Helicity.
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- Solar Physics, 2014, v. 289, n. 2, p. 475, doi. 10.1007/s11207-012-0218-z
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Changes in Quasi-periodic Variations of Solar Photospheric Fields: Precursor to the Deep Solar Minimum in Cycle 23?
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- Solar Physics, 2014, v. 289, n. 1, p. 41, doi. 10.1007/s11207-013-0335-3
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Analysis of Supergranule Sizes and Velocities Using <i>Solar Dynamics Observatory</i> (SDO)/<i>Helioseismic Magnetic Imager</i> (HMI) and <i>Solar and Heliospheric Observatory</i> (SOHO)/<i>Michelson Doppler Imager</i> (MDI) Dopplergrams.
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- Solar Physics, 2014, v. 289, n. 1, p. 11, doi. 10.1007/s11207-013-0330-8
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Velocity and Temperature Response Functions of 61 Photospheric Lines in the Near-Infrared H Band (1500 – 1800 nm) – II.
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- Solar Physics, 2014, v. 289, n. 1, p. 27, doi. 10.1007/s11207-013-0340-6
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