Works matching DE "MAGNETIC fields in the solar corona"
Results: 141
`S' Marks the Spot.
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- Weatherwise, 1999, v. 52, n. 3, p. 15
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Thermomagnetic instability in hot spherical plasma shells.
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- Astronomische Nachrichten, 2017, v. 338, n. 1, p. 56, doi. 10.1002/asna.201613221
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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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Spectral cleaving in solar type II radio bursts: Observations and interpretation.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 689, p. 1, doi. 10.1051/0004-6361/202451010
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MHD simulations of the in situ generation of kink and sausage waves in the solar corona by collision of dense plasma clumps.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 626, p. 1, doi. 10.1051/0004-6361/201935539
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Phase mixing of Alfvén waves propagating in non-reflective magnetic plasma configurations.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2017, v. 600, p. 1, doi. 10.1051/0004-6361/201629892
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Twisted versus braided magnetic flux ropes in coronal geometry.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2016, v. 591, p. 1, doi. 10.1051/0004-6361/201528053
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Using coronal seismology to estimate the magnetic field strength in a realistic coronal model.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2015, v. 581, p. 1, doi. 10.1051/0004-6361/201526237
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Standing kink oscillations of thin twisted magnetic tubes with continuous equilibrium magnetic field.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2015, v. 580, p. 1, doi. 10.1051/0004-6361/201526168
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Coronal heating in multiple magnetic threads.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2015, v. 580, p. 1, doi. 10.1051/0004-6361/201525995
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On the nature of transverse coronal waves revealed by wavefront dislocations.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2015, v. 579, p. 1, doi. 10.1051/0004-6361/201424340
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Coronal magnetic field modeling using stereoscopy constraints.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2015, v. 577, p. 1, doi. 10.1051/0004-6361/201322548
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Steps towards a high precision solar rotation profile: Results from SDO/AIA coronal bright point data.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2015, v. 575, p. 1, doi. 10.1051/0004-6361/201424929
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The solar cycle variation of topological structures in the global solar corona.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2014, v. 565, p. 1, doi. 10.1051/0004-6361/201323048
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Coronal magnetic topology and the production of solar impulsive energetic electrons.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2013, v. 556, n. 6, p. 1, doi. 10.1051/0004-6361/201322072
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Seismic signature of envelope penetrative convection: the CoRoT star HD 52265.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2012, v. 544, n. 2, p. L13-1, doi. 10.1051/0004-6361/201220000
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Hanle effect from a dipolar magnetic structure: the case of the solar corona and the case of a star.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2012, v. 539, p. 1, doi. 10.1051/0004-6361/201118245
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Large-scale 3D MHD simulation on the solar flux emergence and the small-scale dynamic features in an active region.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2012, v. 539, p. 1, doi. 10.1051/0004-6361/201118009
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Lagrangian coherent structures in photospheric flows and their implications for coronal magnetic structure.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2012, v. 539, p. 1, doi. 10.1051/0004-6361/201118278
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Nature of the heating mechanism for the diffuse solar corona.
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- Nature, 1998, v. 393, n. 6685, p. 545, doi. 10.1038/31166
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Evidence for a downward mass flux in the penumbral region of a sunspot.
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- Nature, 1997, v. 389, n. 6646, p. 47, doi. 10.1038/37933
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- Article
Topological classification of global magnetic fields in the solar corona.
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- Dynamical Systems: An International Journal, 2018, v. 33, n. 3, p. 536, doi. 10.1080/14689367.2017.1406457
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Solar physics: Magnetic dance.
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- Nature Physics, 2013, v. 9, n. 2, p. 66, doi. 10.1038/nphys2550
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The Sun's Global Photospheric and Coronal Magnetic Fields: Observations and Models.
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- Living Reviews in Solar Physics, 2012, v. 9, n. 6, p. 1, doi. 10.12942/lrsp-2012-6
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Solar Force-free Magnetic Fields.
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- Living Reviews in Solar Physics, 2012, v. 9, n. 5, p. 5
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Turbulence and chaotic structure generated by nonlinear kinetic Alfvén waves near magnetic null points in solar corona.
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- Astrophysics & Space Science, 2024, v. 369, n. 11, p. 1, doi. 10.1007/s10509-024-04380-w
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Modeling coronal magnetic field using spherical geometry: cases with several active regions.
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- Astrophysics & Space Science, 2013, v. 347, n. 1, p. 21, doi. 10.1007/s10509-013-1493-3
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Resonantly damped oscillations of elliptically shaped stratified emerging coronal loops.
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- Astrophysics & Space Science, 2013, v. 347, n. 1, p. 29, doi. 10.1007/s10509-013-1510-6
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Thermal Cyclotron Radiation by Isolated Magnetic White Dwarfs and Constraints on the Parameters of Their Coronas.
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- Astronomy Reports, 2004, v. 48, n. 2, p. 121, doi. 10.1134/1.1648076
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Parameter Distributions for the Drag‐Based Modeling of CME Propagation.
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- Space Weather: The International Journal of Research & Applications, 2022, v. 20, n. 9, p. 1, doi. 10.1029/2021SW002925
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Sources of Solar Total Irradiance Variations.
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- Solar Physics, 2009, v. 257, n. 1, p. 71, doi. 10.1007/s11207-009-9337-6
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Possible Role of MHD Waves in Heating the Solar Corona.
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- 2009
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- Correction Notice
Automated detection of EUV Polar Coronal Holes during Solar Cycle 23.
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- Solar Physics, 2009, v. 257, n. 1, p. 99, doi. 10.1007/s11207-009-9369-y
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3D MHD Coronal Oscillations about a Magnetic Null Point: Application of WKB Theory.
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- Solar Physics, 2008, v. 251, n. 1/2, p. 563, doi. 10.1007/s11207-007-9107-2
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Very Large Array, SOHO, and RHESSI Observations of Magnetic Interactions and Particle Propagation across Large-Scale Coronal Loops.
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- Solar Physics, 2008, v. 250, n. 1, p. 89, doi. 10.1007/s11207-008-9195-7
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A Statistical Survey of Hard X-ray Spectral Characteristics of Solar Flares with Two Footpoints.
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- Solar Physics, 2008, v. 250, n. 1, p. 53, doi. 10.1007/s11207-008-9193-9
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Nonlinear Force-Free Modeling of Coronal Magnetic Fields. II. Modeling a Filament Arcade and Simulated Chromospheric and Photospheric Vector Fields.
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- Solar Physics, 2008, v. 247, n. 2, p. 269, doi. 10.1007/s11207-007-9110-7
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Can We Improve the Preprocessing of Photospheric Vector Magnetograms by the Inclusion of Chromospheric Observations?
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- Solar Physics, 2008, v. 247, n. 2, p. 249, doi. 10.1007/s11207-008-9130-y
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Time-Latitudinal Dynamics of Magnetic Fields and the Green Corona Over Three Solar Cycles.
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- Solar Physics, 2007, v. 241, n. 2, p. 263, doi. 10.1007/s11207-007-0239-1
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Filamentary Structures of Coronal White-Light Images.
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- Solar Physics, 2007, v. 241, n. 2, p. 251, doi. 10.1007/s11207-007-0250-6
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Ion-Acoustic Wave Generation by Two Kinetic Alfvén Waves and Particle Heating.
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- Solar Physics, 2007, v. 241, n. 2, p. 317, doi. 10.1007/s11207-007-0331-6
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Periodic Appearance of Coronal Holes and the Related Variation of Solar Wind Parameters.
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- Solar Physics, 2007, v. 241, n. 2, p. 371, doi. 10.1007/s11207-007-0336-1
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Observational Evidence for Rising Penumbral Flux Tubes?
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- Solar Physics, 2007, v. 241, n. 2, p. 223, doi. 10.1007/s11207-007-0367-7
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Magnetic Stereoscopy of Coronal Loops in NOAA 8891.
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- Solar Physics, 2007, v. 241, n. 2, p. 235, doi. 10.1007/s11207-007-0370-z
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The Trace Telescope Point Spread Function for the 171 Å Filter.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 531, doi. 10.1007/s11207-006-1994-0
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Properties of Interplanetary Coronal Mass Ejections at One AU During 1995 – 2004.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 393, doi. 10.1007/s11207-006-0133-2
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Spatial and Temporal Scales of Coronal Magnetic Restructuring in the Development of Coronal Mass Ejections.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 257, doi. 10.1007/s11207-006-0181-7
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Fast Segmentation of Solar Extreme Ultraviolet Images.
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- Solar Physics, 2006, v. 239, n. 1/2, p. 519, doi. 10.1007/s11207-006-0140-3
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Two Regularities in the Coronal Green-Line Brightness – Magnetic Field Coupling and the Heating of the Corona.
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- Solar Physics, 2006, v. 238, n. 2, p. 271, doi. 10.1007/s11207-006-0214-2
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Umbral Three-Minute Oscillations and Running Penumbral Waves.
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- Solar Physics, 2006, v. 238, n. 2, p. 231, doi. 10.1007/s11207-006-0160-z
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- Article