Evidence of a complex structure within the 2013 August 19 coronal mass ejection. Radial and longitudinal evolution in the inner heliosphere
arXiv:2203.02713 · doi:10.1051/0004-6361/202142966
Abstract
Context: Late on 2013 August 19, a coronal mass ejection (CME) erupted from an active region located near the far-side central meridian from Earth's perspective. The event and its accompanying shock were remotely observed by the STEREO-A, STEREO-B and SOHO spacecraft. The interplanetary counterpart (ICME) was intercepted by MESSENGER near 0.3 au, and by both STEREO-A and STEREO-B, near 1 au, which were separated by 78° in heliolongitude. The main objective of this study is to follow the radial and longitudinal evolution of the ICME throughout the inner heliosphere, and to examine possible scenarios for the different magnetic flux-rope configuration observed on the solar disk, and measured in situ at the locations of MESSENGER and STEREO-A, separated by 15° in heliolongitude, and at STEREO-B, which detected the ICME flank. Results: We find that the magnetic flux-rope structure detected at STEREO-B belongs to the same ICME detected at MESSENGER and STEREO-A. The opposite helicity deduced at STEREO-B, might be due to the spacecraft intercepting one of the legs of the structure far from the flux-rope axis, while STEREO-A and MESSENGER are crossing through the core of the magnetic flux rope. The different flux-rope orientations measured at MESSENGER and STEREO-A arise probably because the two spacecraft measure a curved, highly distorted and rather complex magnetic flux-rope topology. The ICME may have suffered additional distortion in its evolution in the inner heliosphere, such as the west flank is propagating faster than the east flank when arriving 1 au. Conclusions: This work illustrates how the ambient conditions can significantly affect the expansion and propagation of the CME/ICME, introducing additional irregularities to the already asymmetric eruption, and how these complex structures cannot be directly reconstructed with the current models available.
19 pages, 10 figures
References in corpus (10)
- The Solar Orbiter mission -- Science overview
- Constraints on the Global Structure of Magnetic Clouds: Transverse Size and Curvature
- Progressive transformation of a flux rope to an ICME
- The Solar Orbiter Science Activity Plan: translating solar and heliospheric physics questions into action
- Determining the Intrinsic CME Flux Rope Type Using Remote-sensing Solar Disk Observations
- Relationship between EIT Post Eruption Arcades, Coronal Mass Ejections, Coronal Neutral Line and Magnetic Clouds
- The unusual widespread solar energetic particle event on 2013 August 19. Solar origin and particle longitudinal distribution
- Successive Injection of Opposite Magnetic Helicity in Solar Active Region NOAA 11928
- The 2019 International Women's Day event: A two-step solar flare with multiple eruptive signatures and low Earth impact
- Analysis of the Helical Kink Stability of Differently Twisted Magnetic Flux Ropes
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