Works matching Coronal mass ejections
Results: 3120
Microwave radio emissions as a proxy for coronal mass ejection speed in arrival predictions of interplanetary coronal mass ejections at 1 AU.
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- Journal of Space Weather & Space Climate, 2017, v. 7, p. 1, doi. 10.1051/swsc/2016038
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Interplanetary Coronal Mass Ejections During Solar Cycles 23 and 24: Sun–Earth Propagation Characteristics and Consequences at the Near-Earth Region.
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- Solar Physics, 2019, v. 294, n. 5, p. N.PAG, doi. 10.1007/s11207-019-1443-5
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Coronal Mass Ejections and Non-recurrent Forbush Decreases.
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- Solar Physics, 2014, v. 289, n. 10, p. 3949, doi. 10.1007/s11207-014-0534-6
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A Quick Method for Estimating the Propagation Direction of Coronal Mass Ejections Using STEREO-COR1 Images.
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- Solar Physics, 2008, v. 252, n. 2, p. 385, doi. 10.1007/s11207-008-9267-8
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On the Interplanetary Coronal Mass Ejection Shocks in the Vicinity of the Earth.
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- Earth, Moon & Planets, 2012, v. 109, n. 1-4, p. 13, doi. 10.1007/s11038-012-9398-7
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Which Photospheric Characteristics Are Most Relevant to Active-Region Coronal Mass Ejections?
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- Solar Physics, 2019, v. 294, n. 9, p. N.PAG, doi. 10.1007/s11207-019-1523-6
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Unraveling the Internal Magnetic Field Structure of the Earth-directed Interplanetary Coronal Mass Ejections During 1995 – 2015.
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- Solar Physics, 2019, v. 294, n. 7, p. N.PAG, doi. 10.1007/s11207-019-1477-8
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Flux Accretion and Coronal Mass Ejection Dynamics.
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- Solar Physics, 2018, v. 293, n. 7, p. 1, doi. 10.1007/s11207-018-1329-y
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Fitting and Reconstruction of Thirteen Simple Coronal Mass Ejections.
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- Solar Physics, 2018, v. 293, n. 5, p. 1, doi. 10.1007/s11207-018-1288-3
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First Simultaneous Views of the Axial and Lateral Perspectives of a Coronal Mass Ejection.
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- Solar Physics, 2016, v. 291, n. 6, p. 1799, doi. 10.1007/s11207-016-0941-y
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Coronal Mass Ejections from the Same Active Region Cluster: Two Different Perspectives.
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- Solar Physics, 2015, v. 290, n. 6, p. 1671, doi. 10.1007/s11207-015-0717-9
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Interplanetary Propagation Behavior of the Fast Coronal Mass Ejection on 23 July 2012.
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- Solar Physics, 2015, v. 290, n. 3, p. 919, doi. 10.1007/s11207-014-0642-3
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Identification of Interplanetary Coronal Mass Ejections at Ulysses Using Multiple Solar Wind Signatures.
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- Solar Physics, 2014, v. 289, n. 10, p. 3843, doi. 10.1007/s11207-014-0540-8
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Solar Sources of Interplanetary Coronal Mass Ejections During the Solar Cycle 23/24 Minimum.
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- Solar Physics, 2014, v. 289, n. 10, p. 3773, doi. 10.1007/s11207-014-0552-4
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Propagation of Fast Coronal Mass Ejections and Shock Waves Associated with Type II Radio-Burst Emission: An Analytic Study.
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- Solar Physics, 2013, v. 285, n. 1/2, p. 391, doi. 10.1007/s11207-012-0103-9
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Connecting Coronal Mass Ejections and Magnetic Clouds: A Case Study Using an Event from 22 June 2009.
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- Solar Physics, 2012, v. 281, n. 1, p. 369, doi. 10.1007/s11207-012-0036-3
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Uncovering the Birth of a Coronal Mass Ejection from Two-Viewpoint SECCHI Observations.
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- Solar Physics, 2012, v. 280, n. 2, p. 509, doi. 10.1007/s11207-012-9933-8
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Estimating Travel Times of Coronal Mass Ejections to 1 AU Using Multi-spacecraft Coronagraph Data.
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- Solar Physics, 2012, v. 279, n. 2, p. 477, doi. 10.1007/s11207-012-0005-x
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Coronal Mass Ejections from Magnetic Systems Encompassing Filament Channels Without Filaments.
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- Solar Physics, 2012, v. 277, n. 1, p. 185, doi. 10.1007/s11207-011-9881-8
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Coronal Mass Ejections as Expanding Force-Free Structures.
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- Solar Physics, 2011, v. 270, n. 2, p. 537, doi. 10.1007/s11207-011-9761-2
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Galactic Cosmic Ray Intensity Response to Interplanetary Coronal Mass Ejections/Magnetic Clouds in 1995 - 2009.
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- Solar Physics, 2011, v. 270, n. 2, p. 609, doi. 10.1007/s11207-011-9774-x
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From the Sun to the Earth: The 13 May 2005 Coronal Mass Ejection.
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- Solar Physics, 2010, v. 265, n. 1/2, p. 49, doi. 10.1007/s11207-010-9602-8
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Ooty Interplanetary Scintillation – Remote-Sensing Observations and Analysis of Coronal Mass Ejections in the Heliosphere.
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- Solar Physics, 2010, v. 265, n. 1/2, p. 137, doi. 10.1007/s11207-010-9593-5
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Near-Earth Interplanetary Coronal Mass Ejections During Solar Cycle 23 (1996 – 2009): Catalog and Summary of Properties.
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- Solar Physics, 2010, v. 264, n. 1, p. 189, doi. 10.1007/s11207-010-9568-6
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On 3D Reconstruction of Coronal Mass Ejections: I. Method Description and Application to SECCHI-COR Data.
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- Solar Physics, 2009, v. 259, n. 1/2, p. 123, doi. 10.1007/s11207-009-9416-8
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Why Do Temperature and Velocity Have Different Relationships in the Solar Wind and in Interplanetary Coronal Mass Ejections?
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- Solar Physics, 2009, v. 257, n. 1, p. 169, doi. 10.1007/s11207-009-9338-5
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Expected in Situ Velocities from a Hierarchical Model for Expanding Interplanetary Coronal Mass Ejections.
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- Solar Physics, 2008, v. 250, n. 2, p. 347, doi. 10.1007/s11207-008-9221-9
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Time‐of‐Arrival of Coronal Mass Ejections: A Two‐Phase Kinematics Approach Based on Heliospheric Imaging Observations.
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- Space Weather: The International Journal of Research & Applications, 2022, v. 20, n. 7, p. 1, doi. 10.1029/2022SW003070
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A Machine Learning Approach to Predicting SEP Events Using Properties of Coronal Mass Ejections.
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- Space Weather: The International Journal of Research & Applications, 2022, v. 20, n. 7, p. 1, doi. 10.1029/2021SW002797
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Machine Learning for Predicting the B<sub>z</sub> Magnetic Field Component From Upstream in Situ Observations of Solar Coronal Mass Ejections.
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- Space Weather: The International Journal of Research & Applications, 2021, v. 19, n. 12, p. 1, doi. 10.1029/2021SW002859
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On the Sources and Sizes of Uncertainty in Predicting the Arrival Time of Interplanetary Coronal Mass Ejections Using Global MHD Models.
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- Space Weather: The International Journal of Research & Applications, 2021, v. 19, n. 6, p. 1, doi. 10.1029/2021SW002775
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The Visual Complexity of Coronal Mass Ejections Follows the Solar Cycle.
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- Space Weather: The International Journal of Research & Applications, 2020, v. 18, n. 10, p. 1, doi. 10.1029/2020SW002556
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Higher-speed coronal mass ejections and their geoeffectiveness.
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- Journal of Astrophysics & Astronomy, 2018, v. 39, n. 3, p. 1, doi. 10.1007/s12036-018-9526-5
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Solar cycle variation of interplanetary coronal mass ejection latitudes.
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- Journal of Astrophysics & Astronomy, 2010, v. 31, n. 3, p. 165, doi. 10.1007/s12036-010-0014-9
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Prediction of Geomagnetic Storms Associated with Interplanetary Coronal Mass Ejections.
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- Astronomy Reports, 2024, v. 68, n. 2, p. 192, doi. 10.1134/S1063772924700185
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Search for Solar Sources of Interplanetary Coronal Mass Ejections Using the Reverse Model of Magnetodynamic Interaction of the Solar Wind in the Heliosphere.
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- Astronomy Reports, 2023, v. 67, n. 3, p. 280, doi. 10.1134/S106377292303006X
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MHD Model of the Interaction of a Coronal Mass Ejection with the Hot Jupiter HD 209458b.
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- Astronomy Reports, 2021, v. 65, n. 8, p. 676, doi. 10.1134/S1063772921090092
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Solar Wind Properties and Geospace Impact of Coronal Mass Ejection‐Driven Sheath Regions: Variation and Driver Dependence.
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- Space Weather: The International Journal of Research & Applications, 2019, v. 17, n. 8, p. 1257, doi. 10.1029/2019SW002217
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Forecasting the Structure and Orientation of Earthbound Coronal Mass Ejections.
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- Space Weather: The International Journal of Research & Applications, 2019, v. 17, n. 4, p. 498, doi. 10.1029/2018SW001944
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PROPERTIES OF CORONAL MASS EJECTIONS PROPAGATING IN THE HELIOSPHERE.
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- Journal of Physical Studies, 2012, v. 16, n. 1/2, p. 1, doi. 10.30970/jps.16.1901
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Investigations on halo coronal mass ejections, sunspots and their geoeffectiveness in the rising phase of the solar cycle 25.
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- Astrophysics & Space Science, 2024, v. 369, n. 10, p. 1, doi. 10.1007/s10509-024-04367-7
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Near-surface atmospheric electric field changes through magnetic clouds via coronal mass ejections.
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- Geoscience Letters, 2023, v. 10, n. 1, p. 1, doi. 10.1186/s40562-023-00299-2
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On the viscosity effects in the shock wave observed in the solar wind after the December 13, 2006 coronal mass ejection.
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- Astrophysical Bulletin, 2015, v. 70, n. 1, p. 117, doi. 10.1134/S1990341315010137
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Understanding the Origins of Problem Geomagnetic Storms Associated with "Stealth" Coronal Mass Ejections.
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- Space Science Reviews, 2021, v. 217, n. 8, p. 1, doi. 10.1007/s11214-021-00857-0
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Interplanetary Coronal Mass Ejections Observed in the Heliosphere: 3. Physical Implications.
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- Space Science Reviews, 2009, v. 147, n. 1/2, p. 89, doi. 10.1007/s11214-009-9577-7
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Interplanetary Coronal Mass Ejections Observed in the Heliosphere: 2. Model and Data Comparison.
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- Space Science Reviews, 2009, v. 147, n. 1/2, p. 55, doi. 10.1007/s11214-009-9550-5
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In-Situ Solar Wind and Magnetic Field Signatures of Interplanetary Coronal Mass Ejections.
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- Space Science Reviews, 2006, v. 123, n. 1-3, p. 31, doi. 10.1007/s11214-006-9010-4
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Relationship between speed of Full Halo Coronal Mass Ejections and Cosmic ray intensity.
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- Journal of Ultra Scientist of Physical Sciences - Section B (Physics, Geology, Nano Technology Engineering, Bio Sciences, Material Science Management), 2017, v. 29, n. 11, p. 342, doi. 10.22147/jusps-B/291104
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Studying the Anisotropy of the Muon Flux during Nongeoeffective Coronal Mass Ejections of 2016.
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- Physics of Atomic Nuclei, 2018, v. 81, n. 9, p. 1370, doi. 10.1134/S106377881809003X
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A Solar‐Centric Approach to Improving Estimates of Exposure Processes for Coronal Mass Ejections.
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- Risk Analysis: An International Journal, 2020, v. 40, n. 5, p. 1020, doi. 10.1111/risa.13461
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