Works matching Solar corona
Results: 2363
MESSENGER Observations of Magnetohydrodynamic Waves in the Solar Corona from Faraday Rotation.
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- Solar Physics, 2013, v. 285, n. 1/2, p. 71, doi. 10.1007/s11207-012-0162-y
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Intensity Oscillation in the Corona as Observed during the Total Solar Eclipse of 29 March 2006.
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- Solar Physics, 2009, v. 260, n. 1, p. 125, doi. 10.1007/s11207-009-9434-6
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Photometric Flattening Index of the Solar Corona in the Solar Cycle.
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- Kinematics & Physics of Celestial Bodies, 2023, v. 39, n. 3, p. 164, doi. 10.3103/S0884591323030066
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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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Study of the Solar Wind Plasma Thermodynamics in the Solar Corona Based on the Charge State of Heavy Ions.
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- Astronomy Letters, 2024, v. 50, n. 6, p. 408, doi. 10.1134/S106377372470021X
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HERSCHEL/SCORE, imaging the solar corona in visible and EUV light: CCD camera characterization.
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- Analytical & Bioanalytical Chemistry, 2010, v. 397, n. 6, p. 2033, doi. 10.1007/s00216-010-3697-5
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Tomographic Reconstruction of the Solar K-Corona Using Neural Fields.
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- Solar Physics, 2023, v. 298, n. 11, p. 1, doi. 10.1007/s11207-023-02226-2
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Flattening Index of the Solar Corona and the Sun's Magnetic Field.
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- Solar Physics, 2022, v. 297, n. 3, p. 1, doi. 10.1007/s11207-022-01973-y
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An X Band Radio Channel Model for Propagation Through the Solar Corona.
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- Radio Science, 2018, v. 53, n. 9, p. 1014, doi. 10.1029/2018RS006578
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The Dipolar Solar Minimum Corona.
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- Universe (2218-1997), 2021, v. 7, n. 12, p. 1, doi. 10.3390/universe7120507
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Spectroscopic Observation of Oscillations in the Corona During the Total Solar Eclipse of 22 July 2009.
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- Solar Physics, 2011, v. 270, n. 1, p. 213, doi. 10.1007/s11207-011-9732-7
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Electron Temperatures and Flow Speeds of the Low Solar Corona: MACS Results from the Total Solar Eclipse of 29 March 2006 in Libya.
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- Solar Physics, 2011, v. 270, n. 1, p. 235, doi. 10.1007/s11207-011-9736-3
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Flattening Index of the Solar Corona and the Solar Cycle.
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- Solar Physics, 2011, v. 270, n. 1, p. 347, doi. 10.1007/s11207-011-9749-y
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Electron-Temperature Maps of the Low Solar Corona: ISCORE Results from the Total Solar Eclipse of 29 March 2006 in Libya.
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- Solar Physics, 2009, v. 260, n. 2, p. 347, doi. 10.1007/s11207-009-9457-z
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A Low-Frequency (30 – 110 MHz) Antenna System for Observations of Polarized Radio Emission from the Solar Corona.
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- Solar Physics, 2008, v. 253, n. 1/2, p. 319, doi. 10.1007/s11207-008-9272-y
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A possible reference to the solar corona in a contemporary report of the AD1239 eclipse.
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- Journal for the History of Astronomy, 2022, v. 53, n. 4, p. 415, doi. 10.1177/00218286221125189
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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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Method of Searching for Nanoflares and Their Spatial Distribution in the Solar Corona.
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- Astronomy Letters, 2022, v. 48, n. 9, p. 550, doi. 10.1134/S1063773722090079
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On the spatial and temporal characteristics and formation mechanisms of soft X-ray emission in the solar corona.
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- Astronomy Letters, 2007, v. 33, n. 6, p. 396, doi. 10.1134/S1063773707060059
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Observations of the Solar Corona from Space.
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- Space Science Reviews, 2020, v. 216, n. 8, p. N.PAG, doi. 10.1007/s11214-020-00743-1
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Kinetic Models for Whistler Wave Scattering of Electrons in the Solar Corona and Wind.
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- Space Science Reviews, 2012, v. 172, n. 1-4, p. 303, doi. 10.1007/s11214-011-9749-0
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Wind in the Solar Corona: Dynamics and Composition.
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- Space Science Reviews, 2006, v. 124, n. 1-4, p. 35, doi. 10.1007/s11214-006-9098-6
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The Grad B Drifts Of The Electron And Proton (Seps) At Solar Corona.
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- Journal of the College Of Basic Education, 2024, p. 65
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Nonlinear Interaction of a 3D Kinetic Alfvén Wave with a Null Point and Turbulence Generation in the Solar Corona.
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- Solar Physics, 2022, v. 297, n. 11, p. 1, doi. 10.1007/s11207-022-02083-5
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3D Temperatures and Densities of the Solar Corona via Multi-Spacecraft EUV Tomography: Analysis of Prominence Cavities.
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- Solar Physics, 2009, v. 256, n. 1/2, p. 73, doi. 10.1007/s11207-009-9321-1
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The Fe IX Line at 17.1 nm in the Radiation Spectrum of Slow Magneto-Acoustic Waves Propagating in the Solar Corona.
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- Kinematics & Physics of Celestial Bodies, 2021, v. 37, n. 6, p. 300, doi. 10.3103/S0884591321060064
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Observation of Six Pre-Flare VLP Pulsations in Solar Corona.
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- Iranian Journal of Astronomy & Astrophysics, 2023, v. 10, n. 2, p. 62, doi. 10.22128/ijaa.2023.720.1163
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Nonlinear kinetic Alfvén-wave localized structures and turbulence generation in the solar corona.
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- Astrophysics & Space Science, 2022, v. 367, n. 9, p. 1, doi. 10.1007/s10509-022-04126-6
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MHD waves and instabilities of a temperature-anisotropic plasma in the solar corona as a source of its heating.
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- Astronomy Letters, 2011, v. 37, n. 9, p. 649, doi. 10.1134/S0320010811090038
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Spatial and Temporal Distribution of Solar Green-Line Corona for Solar Cycles 18 – 24.
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- Solar Physics, 2022, v. 297, n. 9, p. 1, doi. 10.1007/s11207-022-02050-0
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Radio Sounding Measurements of the Solar Corona Using Giant Pulses of the Crab Pulsar in 2018.
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- Solar Physics, 2020, v. 295, n. 6, p. 1, doi. 10.1007/s11207-020-01644-w
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Radio Occultation Observations of the Solar Corona Over 1.60–1.86 R<sub>⊙</sub>: Faraday Rotation and Frequency Shift Analysis.
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- Journal of Geophysical Research. Space Physics, 2019, v. 124, n. 10, p. 7761, doi. 10.1029/2019JA026937
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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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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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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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On Rotation of the Solar Corona.
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- Solar Physics, 2012, v. 281, n. 2, p. 611, doi. 10.1007/s11207-012-0105-7
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White-Light Observations and Polarimetric Analysis of the Solar Corona During the Eclipse of 1 August 2008.
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- Solar Physics, 2012, v. 277, n. 2, p. 267, doi. 10.1007/s11207-011-9910-7
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Dynamic Three-Dimensional Tomography of the Solar Corona.
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- Solar Physics, 2010, v. 262, n. 2, p. 495, doi. 10.1007/s11207-010-9536-1
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A Coherence-Based Approach for Tracking Waves in the Solar Corona.
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- Solar Physics, 2008, v. 252, n. 2, p. 321, doi. 10.1007/s11207-008-9257-x
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The Magnetic Field of the Solar Corona from Pulsar Observations.
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- Solar Physics, 2007, v. 245, n. 1, p. 109, doi. 10.1007/s11207-007-9030-6
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The Influence of the Electron κ-Distribution in the Solar Corona on the Fe VIII – Fe XV Line Intensities.
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- Solar Physics, 2006, v. 234, n. 2, p. 243, doi. 10.1007/s11207-006-1615-y
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Fine Structure of the Solar Corona in High-Frequency Resolution Radio Observations.
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- Cosmic Research, 2024, v. 62, n. 6, p. 588, doi. 10.1134/S0010952524600483
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A Comparative Analysis of Quasi-Periodic Processes in the Magnetospheric Current Sheet and the Current Sheets of the Solar Corona.
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- Cosmic Research, 2022, v. 60, n. 6, p. 420, doi. 10.1134/S0010952522060119
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Solar Corona as Indicator of Differential Rotation of Subphotospheric Layers.
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- Cosmic Research, 2019, v. 57, n. 6, p. 407, doi. 10.1134/S0010952519060042
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Magnetoacoustic wave propagation in the solar corona and filament dynamics.
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- Scientific Reports, 2024, v. 14, n. 1, p. 1, doi. 10.1038/s41598-024-80229-0
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ON THE SOLAR CORONA PETROGLYPH IN THE CHACO CANYON.
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- Mediterranean Archaeology & Archaeometry, 2014, v. 14, n. 3, p. 189
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How Transverse Waves Drive Turbulence in the Solar Corona.
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- Symmetry (20738994), 2022, v. 14, n. 2, p. N.PAG, doi. 10.3390/sym14020384
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Validating the Alfven Wave Solar Model (AWSoM) from the lower corona to 1 AU.
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- Geophysical Research Abstracts, 2019, v. 21, p. 1
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Numerical simulations of kinetic turbulence in the low beta regime: interpreting MMS observations in the Earth's magnetosheath and predicting PSP observations in the solar corona.
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- Geophysical Research Abstracts, 2019, v. 21, p. 1
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Two modes of the differential rotation of the solar corona.
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- Astronomy Reports, 2009, v. 53, n. 3, p. 262, doi. 10.1134/S1063772909030081
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