Works matching DE "MAGNETIC fields in the solar corona"
Results: 143
Space Climate and Solar Energetic Particles.
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- Iranian Journal of Astronomy & Astrophysics, 2024, v. 11, n. 1, p. 1, doi. 10.22128/ijaa.2024.768.1176
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Solar transient events and their importance for coronal heating.
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- Science Progress, 2004, v. 87, n. 2, p. 101, doi. 10.3184/003685004783238562
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Modeling the Magnetic Field of the Inner Corona in a Radially Expanding Solar Wind.
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- Physics (2624-8174), 2023, v. 5, n. 1, p. 161, doi. 10.3390/physics5010012
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Evidence for shock generation in the solar corona in the absence of coronal mass ejections.
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- Astronomy Reports, 2017, v. 61, n. 9, p. 805, doi. 10.1134/S1063772917080030
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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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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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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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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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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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A Large-Scale Dataset of Three-Dimensional Solar Magnetic Fields Extrapolated by Nonlinear Force-Free Method.
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- Scientific Data, 2023, v. 10, n. 1, p. 1, doi. 10.1038/s41597-023-02091-5
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Comparison of Solar Wind Parameters with Characteristics of Coronal Holes.
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- Geomagnetism & Aeronomy, 2024, v. 64, n. 8, p. 1250, doi. 10.1134/S0016793224700348
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Magnetic-Field Concentration and the Twisted Solar Coronal Loops.
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- Geomagnetism & Aeronomy, 2021, v. 61, n. 7, p. 1052, doi. 10.1134/S0016793221070203
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Manifestations in the Solar Corona of the Process of Magnetic-Field Generation.
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- Geomagnetism & Aeronomy, 2020, v. 60, n. 7, p. 831, doi. 10.1134/S0016793220070178
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Evolutionary Changes in the Configuration of the Magnetic Field of the Solar Corona in the Epoch of the Minimum.
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- Geomagnetism & Aeronomy, 2019, v. 59, n. 8, p. 1103, doi. 10.1134/S0016793219080127
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Modification of "Pressed" Atmospheres in Active Regions of Ultracool Stars.
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- Geomagnetism & Aeronomy, 2017, v. 57, n. 7, p. 859, doi. 10.1134/S0016793217070271
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On the Constancy of the Width of Coronal Magnetic Loops.
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- Geomagnetism & Aeronomy, 2017, v. 57, n. 7, p. 841, doi. 10.1134/S001679321707026X
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Model of quiescent prominence with the helical magnetic field.
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- Geomagnetism & Aeronomy, 2016, v. 56, n. 8, p. 1090, doi. 10.1134/S0016793216080193
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Method for the determination of the height of a solar filament.
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- Geomagnetism & Aeronomy, 2016, v. 56, n. 1, p. 1, doi. 10.1134/S0016793216010059
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Kinetic approach to the formation of 3D electromagnetic structures in flows of expanding plasma coronas. II. flow anisotropy parameters.
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- Geomagnetism & Aeronomy, 2015, v. 55, n. 8, p. 1009, doi. 10.1134/S0016793215080101
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Ultrafine magnetic structures in the chromosphere.
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- Geomagnetism & Aeronomy, 2015, v. 55, n. 7, p. 846, doi. 10.1134/S0016793215070294
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Nonlinear interaction between wave and convective disturbances in the solar corona.
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- Geomagnetism & Aeronomy, 2015, v. 55, n. 7, p. 850, doi. 10.1134/S0016793215070270
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Effects of extraordinary solar cosmic ray events on variations in the atmospheric electric field at high latitudes.
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- Geomagnetism & Aeronomy, 2015, v. 55, n. 5, p. 650, doi. 10.1134/S0016793215050151
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Effect of Coulomb collisions on the particle acceleration in collapsing magnetic traps.
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- Astronomy Letters, 2009, v. 35, n. 1, p. 57, doi. 10.1134/S1063773709010071
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On the causes of the observed magnetic field imbalance in solar active regions.
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- Astronomy Letters, 2006, v. 32, n. 11, p. 787, doi. 10.1134/S1063773706110090
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Relation of the coronal green line intensity to magnetic fields and sunspot areas in the solar cycle.
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- Astronomy Letters, 2006, v. 32, n. 10, p. 698, doi. 10.1134/S1063773706100057
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Calculating the Potential Magnetic Field of a Local Region on the Sun Using the Measured Oblique Component.
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- Astronomy Letters, 2002, v. 28, n. 5, p. 345, doi. 10.1134/1.1476983
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Penetration of Coronal Magnetic Fields into Solar-Wind Streams.
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- Astronomy Letters, 2000, v. 26, n. 8, p. 539, doi. 10.1134/1.1306990
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`S' Marks the Spot.
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- Weatherwise, 1999, v. 52, n. 3, p. 15
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Spectral Lines in FUV and EUV for Diagnosing Coronal Magnetic Field.
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- Solar Physics, 2022, v. 297, n. 7, p. 1, doi. 10.1007/s11207-022-02024-2
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Analytical Three-dimensional Magnetohydrostatic Equilibrium Solutions for Magnetic Field Extrapolation Allowing a Transition from Non-force-free to Force-free Magnetic Fields.
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- Solar Physics, 2019, v. 294, n. 12, p. 1, doi. 10.1007/s11207-019-1561-0
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Determination of the Coronal and Interplanetary Magnetic Field Strength and Radial Profiles from Large-Scale Photospheric Magnetic Fields.
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- Solar Physics, 2018, v. 293, n. 7, p. 1, doi. 10.1007/s11207-018-1324-3
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Flux Rope Formation Due to Shearing and Zipper Reconnection.
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- Solar Physics, 2018, v. 293, n. 6, p. 1, doi. 10.1007/s11207-018-1318-1
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Computation of Relative Magnetic Helicity in Spherical Coordinates.
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- Solar Physics, 2018, v. 293, n. 6, p. 1, doi. 10.1007/s11207-018-1314-5
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Cyclic Evolution of Coronal Fields from a Coupled Dynamo Potential-Field Source-Surface Model.
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- Solar Physics, 2016, v. 291, n. 2, p. 339, doi. 10.1007/s11207-015-0831-8
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Blind Stereoscopy of the Coronal Magnetic Field.
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- Solar Physics, 2015, v. 290, n. 10, p. 2765, doi. 10.1007/s11207-015-0791-z
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Influence of Non-Potential Coronal Magnetic Topology on Solar-Wind Models.
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- Solar Physics, 2015, v. 290, n. 10, p. 2791, doi. 10.1007/s11207-015-0795-8
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Frozen-in Fractals All Around: Inferring the Large-Scale Effects of Small-Scale Magnetic Structure.
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- Solar Physics, 2015, v. 290, n. 7, p. 1897, doi. 10.1007/s11207-015-0733-9
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A Challenging Solar Eruptive Event of 18 November 2003 and the Causes of the 20 November Geomagnetic Superstorm. IV. Unusual Magnetic Cloud and Overall Scenario.
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- Solar Physics, 2014, v. 289, n. 12, p. 4653, doi. 10.1007/s11207-014-0596-5
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Effects of Field-Aligned Flows on Standing Kink and Sausage Modes Supported by Coronal Loops.
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- Solar Physics, 2014, v. 289, n. 5, p. 1663, doi. 10.1007/s11207-013-0420-7
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Polarimetric Properties of Flux Ropes and Sheared Arcades in Coronal Prominence Cavities.
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- Solar Physics, 2013, v. 288, n. 2, p. 617, doi. 10.1007/s11207-013-0325-5
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Sunspot Bright Points.
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- Solar Physics, 2013, v. 288, n. 1, p. 171, doi. 10.1007/s11207-013-0306-8
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On Ponderomotive Effects Induced by Alfvén Waves in Inhomogeneous 2.5D MHD Plasmas.
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- Solar Physics, 2013, v. 288, n. 1, p. 205, doi. 10.1007/s11207-013-0298-4
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The Force-Free Electrodynamics Method for the Extrapolation of Coronal Magnetic Fields from Vector Magnetograms.
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- Solar Physics, 2013, v. 282, n. 2, p. 419, doi. 10.1007/s11207-012-0154-y
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Coronal Magnetic Field Structure and Evolution for Flaring AR 11117 and Its Surroundings.
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- Solar Physics, 2012, v. 281, n. 1, p. 53, doi. 10.1007/s11207-012-9961-4
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Solar Magnetic Carpet II: Coronal Interactions of Small-Scale Magnetic Fields.
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- Solar Physics, 2012, v. 278, n. 1, p. 149, doi. 10.1007/s11207-011-9924-1
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Pre-Flare Flows in the Corona.
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- Solar Physics, 2010, v. 267, n. 2, p. 361, doi. 10.1007/s11207-010-9661-x
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Vlasov - Maxwell, Self-consistent Electromagnetic Wave Emission Simulations in the Solar Corona.
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- Solar Physics, 2010, v. 267, n. 2, p. 393, doi. 10.1007/s11207-010-9660-y
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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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