Characteristics and Importance of "ICME-in-Sheath" Phenomenon and Upper Limit for Geomagnetic Storm Activity
arXiv:2006.09699 · doi:10.3847/2041-8213/ab9d25
Abstract
As an important source for large geomagnetic storms, an "ICME-in-sheath" is a completely shocked interplanetary coronal mass ejection (ICME) stuck in the sheath between a shock and host ejecta. Typical characteristics are identified from coordinated multi-sets of observations: (1) it is usually short in duration and lasts a few hours at 1 AU; (2) its solar wind parameters, in particular the magnetic field, seem to keep enhanced for a large range of distances; and (3) common ICME signatures are often lost. The host ejecta could be a single ICME or a complex ejecta, being fast enough to drive a shock. These results clarify previous misinterpretations of this phenomenon as a normal part of a sheath region. The "ICME-in-sheath" phenomenon, together with a preconditioning effect, produced an extreme set of the magnetic field, speed and density near 1 AU in the 2012 July 23 case, all around their upper limits at the same time. This is probably the most extreme solar wind driving at 1 AU and enables us to estimate the plausible upper limit for geomagnetic storm activity. With an appropriate modification in the southward field, we suggest that a geomagnetic storm with a minimum of about nT could occur in principle. The magnetopause would be compressed to about 3.3 Earth radii from the Earth's center, well inside the geosynchronous orbit.
arXiv commentAccepted for publication in The Astrophysical Journal Letters
References in corpus (15)
- Observations of an extreme storm in interplanetary space caused by successive coronal mass ejections
- Reconstructing CMEs with Coordinated Imaging and In Situ Observations: Global Structure, Kinematics, and Implications for Space Weather Forecasting
- On Sun-to-Earth Propagation of Coronal Mass Ejections
- Multi-point shock and flux rope analysis of multiple interplanetary coronal mass ejections around 2010 August 1 in the inner heliosphere
- Interactions between Coronal Mass Ejections Viewed in Coordinated Imaging and In Situ Observations
- CME-CME Interactions as Sources of CME Geo-effectiveness: The Formation of the Complex Ejecta and Intense Geomagnetic Storm in Early September 2017
- Plasma and Magnetic Field Characteristics of Solar Coronal Mass Ejections in Relation to Geomagnetic Storm Intensity and Variability
- Shocks inside CMEs: A Survey of Properties from 1997 to 2006
- Asymmetry in the CME-CME interaction process for the events from 2011 February 14-15
- The 2010 August 01 type II burst: A CME-CME Interaction, and its radio and white-light manifestations
- 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
- Magnetohydrodynamic simulation of the interaction between two interplanetary magnetic clouds and its consequent geoeffectiveness
- Properties of the Fast Forward Shock Driven by the July 23 2012 Extreme Coronal Mass Ejection
- A Comparative Study of 2017 July and 2012 July Complex Eruptions: Are Solar Superstorms "Perfect Storms" in Nature?
- Propagation and Interaction Properties of Successive Coronal Mass Ejections in Relation to a Complex Type II Radio Burst
Cited by in corpus (6)
- Extreme solar events
- Detection of small magnetic flux ropes from the third and fourth Parker Solar Probe encounters
- Polytropic behavior in the structures of Interplanetary Coronal Mass Ejections
- Dependence of great geomagnetic storm intensity (SYM-H-200 nT) on associated solar wind parameters
- Categorization of Coronal Mass Ejection Driven Sheath Regions: Characteristics of STEREO Events
- Estimation of the solar wind extreme events