CME-CME Interactions as Sources of CME Geo-effectiveness: The Formation of the Complex Ejecta and Intense Geomagnetic Storm in Early September 2017
arXiv:1911.10817 · doi:10.3847/1538-4365/ab6216
Abstract
Coronal mass ejections (CMEs) are the primary sources of intense disturbances at Earth, where their geo-effectiveness is largely determined by their dynamic pressure and internal magnetic field, which can be significantly altered during interactions with other CMEs in interplanetary space. We analyse three successive CMEs that erupted from the Sun during September 4-6, 2017, investigating the role of CME-CME interactions as source of the associated intense geomagnetic storm (Dst_min=-142 nT on September 7). To quantify the impact of interactions on the (geo-)effectiveness of individual CMEs, we perform global heliospheric simulations with the EUHFORIA model, using observation-based initial parameters with the additional purpose of validating the predictive capabilities of the model for complex CME events. The simulations show that around 0.45 AU, the shock driven by the September 6 CME started compressing a preceding magnetic ejecta formed by the merging of two CMEs launched on September 4, significantly amplifying its Bz until a maximum factor of 2.8 around 0.9 AU. The following gradual conversion of magnetic energy into kinetic and thermal components reduced the Bz amplification until its almost complete disappearance around 1.8 AU. We conclude that a key factor at the origin of the intense storm triggered by the September 4-6, 2017 CMEs was their arrival at Earth during the phase of maximum Bz amplification. Our analysis highlights how the amplification of the magnetic field of individual CMEs in space-time due to interaction processes can be characterised by a growth, a maximum, and a decay phase, suggesting that the time interval between the CME eruptions and their relative speeds are critical factors in determining the resulting impact of complex CMEs at various heliocentric distances (helio-effectiveness).
References in corpus (17)
- Observations of an extreme storm in interplanetary space caused by successive coronal mass ejections
- JHelioviewer - Time-dependent 3D visualisation of solar and heliospheric data
- Connecting speeds, directions and arrival times of 22 coronal mass ejections from the Sun to 1 AU
- Progressive transformation of a flux rope to an ICME
- Global and local expansion of magnetic clouds in the inner heliosphere
- Global Trends of CME Deflections Based on CME and Solar Parameters
- Observation-based modelling of magnetised Coronal Mass Ejections with EUHFORIA
- Determining the Intrinsic CME Flux Rope Type Using Remote-sensing Solar Disk Observations
- Predicting the magnetic vectors within coronal mass ejections arriving at Earth: 1. Initial Architecture
- Interplanetary Propagation Behavior of the Fast Coronal Mass Ejection from 23 July 2012
- Relationship between EIT Post Eruption Arcades, Coronal Mass Ejections, Coronal Neutral Line and Magnetic Clouds
- Shocks inside CMEs: A Survey of Properties from 1997 to 2006
- Preconditioning of interplanetary space due to transient CME disturbances
- Spectral Analysis of the September 2017 Solar Energetic Particle Events
- Magnetohydrodynamic simulation of the interaction between two interplanetary magnetic clouds and its consequent geoeffectiveness
- Magnetohydrodynamic Simulation of the Interaction between Interplanetary Strong Shock and Magnetic Cloud and its Consequent Geoeffectiveness
- The causes of quasi-homologous CMEs
Cited by in corpus (30)
- The Solar and Geomagnetic Storms in May 2024: A Flash Data Report
- On the Mesoscale Structure of CMEs at Mercury's Orbit: BepiColombo and Parker Solar Probe Observations
- CMEs and SEPs During November-December 2020: A Challenge for Real-Time Space Weather Forecasting
- First simultaneous in situ measurements of a coronal mass ejection by Parker Solar Probe and STEREO-A
- Implementing the MULTI-VP coronal model in EUHFORIA: test case results and comparisons with the WSA coronal model
- CME Evolution in the Structured Heliosphere and Effects at Earth and Mars During Solar Minimum
- Modelling a multi-spacecraft coronal mass ejection encounter with EUHFORIA
- The effect of stream interaction regions on ICME structures observed in longitudinal conjunction
- A comparative study of two X2.2 and X9.3 solar flares observed with HARPS-N: Reconciling Sun-as-a-star spectroscopy and high-spatial resolution solar observations in the context of the solar-stellar connection
- Using radio triangulation to understand the origin of two subsequent type II radio bursts
- A Coronal Mass Ejection and Magnetic Ejecta Observed In Situ by STEREO-A and Wind at 55 Angular Separation
- Causes and Consequences of Magnetic Complexity Changes within Interplanetary Coronal Mass Ejections: a Statistical Study
- Rotation and interaction of the September 8 and 10, 2014 CMEs tested with EUHFORIA
- Exploring the radial evolution of Interplanetary Coronal Mass Ejections using EUHFORIA
- Successive interacting coronal mass ejections: How to create a perfect storm?
- The spheromak tilting and how it affects modelling coronal mass ejections
- Evolution of coronal mass ejections and the corresponding Forbush decreases: modelling vs multi-spacecraft observations
- Solar Ring Mission: Building a Panorama of the Sun and Inner-heliosphere
- An MHD Modeling of Successive X2.2 and X9.3 Solar Flares of 2017 September 6
- Characteristics and Importance of "ICME-in-Sheath" Phenomenon and Upper Limit for Geomagnetic Storm Activity
- Modeling a Coronal Mass Ejection from an Extended Filament Channel. II. Interplanetary Propagation to 1 au
- Clustering of fast Coronal Mass Ejections during the solar cycles 23 and 24 and implications for CME-CME interactions
- Constraining the CME Core Heating and Energy Budget with SOHO/UVCS
- Investigation of two coronal mass ejections from circular ribbon source region: Origin, Sun-Earth propagation and Geo-effectiveness
- Validation of heliospheric modeling algorithms through pulsar observations II: simulations with EUHFORIA
- Validation of EUHFORIA cone and spheromak Coronal Mass Ejection Models
- Effects of optimisation parameters on data-driven magnetofrictional modelling of active regions
- Saturation of the compression of two interacting magnetic flux tubes evidenced in the laboratory
- Space weather: the solar perspective -- an update to Schwenn (2006)
- Magnetic Structure and Propagation of Two Interacting CMEs from the Sun to Saturn