On Sun-to-Earth Propagation of Coronal Mass Ejections
arXiv:1304.3777 · doi:10.1088/0004-637X/769/1/45
Abstract
We investigate how coronal mass ejections (CMEs) propagate through, and interact with, the inner heliosphere between the Sun and Earth, a key question in CME research and space weather forecasting. CME Sun-to-Earth kinematics are constrained by combining wide-angle heliospheric imaging observations, interplanetary radio type II bursts and in situ measurements from multiple vantage points. We select three events for this study, the 2012 January 19, 23, and March 7 CMEs. Different from previous event studies, this work attempts to create a general picture for CME Sun-to-Earth propagation and compare different techniques for determining CME interplanetary kinematics. Key results are obtained concerning CME Sun-to-Earth propagation. Our comparison between different techniques (and data sets) also has important implications for CME observations and their interpretations. Future CME observations and space weather forecasting are discussed based on these results. See detail in the PDF.
ApJ, in press
References in corpus (5)
- Constraints on the Global Structure of Magnetic Clouds: Transverse Size and Curvature
- Determining the azimuthal properties of coronal mass ejections from multi-spacecraft remote-sensing observations with stereo secchi
- A Comprehensive View of the 2006 December 13 CME: From the Sun to Interplanetary Space
- Accuracy and Limitations of Fitting and Stereoscopic Methods to Determine the Direction of Coronal Mass Ejections from Heliospheric Imagers Observations
- POLAR Investigation of the Sun - POLARIS
Cited by in corpus (65)
- The Challenge of Machine Learning in Space Weather Nowcasting and Forecasting
- Observations of an extreme storm in interplanetary space caused by successive coronal mass ejections
- The Interaction of Successive Coronal Mass Ejections: A Review
- Connecting speeds, directions and arrival times of 22 coronal mass ejections from the Sun to 1 AU
- Origin and Structures of Solar Eruptions I: Magnetic Flux Rope (Invited Review)
- Investigating Two Successive Flux Rope Eruptions In A Solar Active Region
- Quantitative Comparison of Methods for Predicting the Arrival of Coronal Mass Ejections at Earth based on multi-view imaging
- Chromosphere to 1 AU Simulation of the 2011 March 7th Event: A Comprehensive Study of Coronal Mass Ejection Propagation
- Plasma and Magnetic Field Characteristics of Solar Coronal Mass Ejections in Relation to Geomagnetic Storm Intensity and Variability
- Drag-Based Ensemble Model (DBEM) for Coronal Mass Ejection Propagation
- A STEREO Survey of Magnetic Cloud Coronal Mass Ejections Observed at Earth in 2008--2012
- Interplanetary Propagation Behavior of the Fast Coronal Mass Ejection from 23 July 2012
- Radial Evolution of Coronal Mass Ejections Between MESSENGER, Venus Express, STEREO, and L1: Catalog and Analysis
- On Sun-to-Earth Propagation of Coronal Mass Ejections: 2. Slow Events and Comparison with Others
- Sun-to-Earth Characteristics of Two Coronal Mass Ejections Interacting near 1 AU: Formation of a Complex Ejecta and Generation of a Two-Step Geomagnetic Storm
- Propagation of the 2012 March Coronal Mass Ejections from the Sun to Heliopause
- Homologous large-amplitude Nonlinear fast-mode Magnetosonic Waves Driven by Recurrent Coronal Jets
- Sun-to-Earth Characteristics of the 2012 July 12 Coronal Mass Ejection and Associated Geo-effectiveness
- Combined Multipoint Remote and In Situ Observations of the Asymmetric Evolution of a Fast Solar Coronal Mass Ejection
- Probabilistic Drag-Based Ensemble Model (DBEM) Evaluation for Heliospheric Propagation of CMEs
- On the Statistical Relationship between CME Speed and Soft X-ray Flux and Fluence of the Associated Flare
- CMEs in the Heliosphere: I. A Statistical Analysis of the Observational Properties of CMEs Detected in the Heliosphere from 2007 to 2017 by STEREO/HI-1
- Magnetic Field Restructuring Associated with Two Successive Solar Eruptions
- Geometry, Kinematics and Heliospheric Impact of a Large CME-driven Shock in 2017 September
- A Comparative Study of 2017 July and 2012 July Complex Eruptions: Are Solar Superstorms "Perfect Storms" in Nature?
- Characteristics of a Gradual Filament Eruption and Subsequent CME Propagation in Relation to a Strong Geomagnetic Storm
- The spectroscopic imprint of the pre-eruptive configuration resulting into two major coronal mass ejections
- A comparison of reconstruction methods for the estimation of CME kinematics based on SECCHI/HI observations
- Sun-to-Earth Propagation of the 2015 June 21 Coronal Mass Ejection Revealed by Optical, EUV, and Radio Observations
- The effect of stream interaction regions on ICME structures observed in longitudinal conjunction
- Sheath-Accumulating Propagation of Interplanetary Coronal Mass Ejection
- A Stealth CME Bracketed between Slow and Fast Wind Producing Unexpected Geo-effectiveness
- Comparing the Properties of ICME-Induced Forbush Decreases at Earth and Mars
- Assessing the collision nature of coronal mass ejections in the inner heliosphere
- Low-frequency type II radio detections and coronagraph data to describe and forecast the propagation of 71 CMEs/shocks
- Roles of photospheric motions and flux emergence in the major solar eruption on 2017 September 6
- On Understanding the Nature of Collision of Coronal Mass Ejections Observed by \textit{STEREO}
- Modeling Interplanetary Expansion and Deformation of CMEs with ANTEATR-PARADE I: Relative Contribution of Different Forces
- Interplanetary and Geomagnetic Consequences of Interacting CMEs of 13-14 June 2012
- Propagation of Coronal Mass Ejections from the Sun to Earth
- Propagating Conditions and the Time of ICMEs Arrival: A Comparison of the Effective Acceleration Model with ENLIL and DBEM Models
- Investigation of energetic particle release using multi-point imaging and in situ observations
- CMEs in the Heliosphere: III. A Statistical Analysis of the Kinematic Properties Derived from Stereoscopic Geometrical Modelling Techniques Applied to CMEs Detected in the Heliosphere from 2008 to 2014 by STEREO/HI-1
- Characteristics and Importance of "ICME-in-Sheath" Phenomenon and Upper Limit for Geomagnetic Storm Activity
- Comparison of magnetic properties in a magnetic cloud and its solar source on April 11-14 2013
- Multi-spacecraft Observations of the Coronal and Interplanetary Evolution of a Solar Eruption Associated with Two Active Regions
- Comparison of CME/shock propagation models with heliospheric imaging and in situ observations
- Quantifying the Propagation of Fast Coronal Mass Ejections from the Sun to Interplanetary Space Combining Remote Sensing and Multi-Point in-situ Observations
- Evolution of CME Properties in the Inner Heliosphere: Prediction for Solar Orbiter and Parker Solar Probe
- Quantifying the uncertainty in CME kinematics derived from geometric modelling of Heliospheric Imager data
- Synthetic Radio Imaging for Quiescent and CME-flare Scenarios
- Relationship between Successive Flares in the Same Active Region and Space-Weather HMI Active Region Patch (SHARP) Parameters
- Kinetic Properties of an Interplanetary Shock Propagating inside a Coronal Mass Ejection
- Tracking and Validating ICMEs Propagating Toward Mars Using STEREO Heliospheric Imagers Combined With Forbush Decreases Detected by MSL/RAD
- Propagation and Interaction Properties of Successive Coronal Mass Ejections in Relation to a Complex Type II Radio Burst
- Using Coordinated Observations in Polarised White Light and Faraday Rotation to Probe the Spatial Position and Magnetic Field of an Interplanetary Sheath
- Electron acceleration and radio emission following the early interaction of two coronal mass ejections
- STEREO-Wind Radio Positioning of an Unusually Slow Drifting Event
- Propagation Characteristics of Two Coronal Mass Ejections From the Sun Far into Interplanetary Space
- Multispacecraft Remote Sensing and In Situ Observations of the 2020 November 29 Coronal Mass Ejection and Associated Shock: From Solar Source to Heliospheric Impacts
- Space weather: the solar perspective -- an update to Schwenn (2006)
- Limb Observations of Global Solar Coronal Extreme-ultraviolet Wavefronts: The Inclination, Kinematics, Coupling with the Expanding Coronal Mass Ejections, and Connection with the Coronal Mass Ejection Driven Shocks
- A Solar Eruption with Relatively Strong Geo-effectiveness Originating from Active Region Peripheral Diffusive Polarities
- Earth-affecting Solar Transients: A Review of Progresses in Solar Cycle 24
- IAU commission 10 "Solar Activity": Legacy report and triennial report for 2012-2015