The 2019 International Women's Day event: A two-step solar flare with multiple eruptive signatures and low Earth impact
arXiv:2106.15417 · doi:10.1051/0004-6361/202140752
Abstract
We present a detailed analysis of an eruptive event that occurred on early 2019 March 8 in active region AR 12734, to which we refer as the International Women's day event. The event under study is intriguing in several aspects: 1) low-coronal eruptive signatures come in ''pairs'' (a double-peak flare, two coronal dimmings, and two EUV waves); 2) although the event is characterized by a complete chain of eruptive signatures, the corresponding coronagraphic signatures are weak; 3) although the source region of the eruption is located close to the center of the solar disc and the eruption is thus presumably Earth-directed, heliospheric signatures are very weak with little Earth-impact. We analyze a number of multi-spacecraft and multi-instrument (both remote-sensing and in situ) observations, including Soft X-ray, (extreme-) ultraviolet (E)UV), radio and white-light emission, as well as plasma, magnetic field and particle measurements. We employ 3D NLFF modeling to investigate the coronal magnetic field configuration in and around the active region, the GCS model to make a 3D reconstruction of the CME geometry and the 3D MHD numerical model EUHFORIA to model the background state of the heliosphere. Our results indicate two subsequent eruptions of two systems of sheared and twisted magnetic fields, which merge already in the upper corona and start to evolve further out as a single entity. The large-scale magnetic field significantly influences both, the early and the interplanetary evolution of the structure. During the first eruption the stability of the overlying field was disrupted which enabled the second eruption. We find that during the propagation in the interplanetary space the large-scale magnetic field, i.e. , the location of heliospheric current sheet between the AR and the Earth likely influences propagation and the evolution of the erupted structure(s).
20 pages, 14 figures
References in corpus (26)
- The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: SHARPs -- Space-weather HMI Active Region Patches
- Preprocessing of vector magnetograph data for a non-linear force-free magnetic field reconstruction
- Why Is the Great Solar Active Region 12192 Flare-Rich But CME-Poor?
- No Trace Left Behind: Stereo Observation of a Coronal Mass Ejection without Low Coronal Signatures
- Magnetic Properties of Solar Active Regions that Govern Large Solar Flares and Eruptions
- Nonlinear force-free modeling of the solar coronal magnetic field
- High cadence observations of a global coronal wave by EUVI/STEREO
- The Confined X-class Flares of Solar Active Region 2192
- First Evidence of Coexisting EIT Wave and Coronal Moreton Wave from SDO/AIA Observations
- Understanding the Physical Nature of Coronal "EIT Waves"
- Magnetic helicity estimations in models and observations of the solar magnetic field. Part I: Finite volume methods
- Geoeffectiveness of Coronal Mass Ejections in the SOHO era
- Statistical Analysis of Large-scale EUV Waves Observed by STEREO/EUVI
- In situ measurements of the variable slow solar wind near sector boundaries
- In Situ Properties of Small and Large Flux Ropes in the Solar Wind
- Spectroscopy and Differential Emission Measure diagnostics of a coronal dimming associated with a fast halo CME
- Implementing the MULTI-VP coronal model in EUHFORIA: test case results and comparisons with the WSA coronal model
- Magnetic Flux of EUV Arcade and Dimming Regions as a Relevant Parameter for Early Diagnostics of Solar Eruptions - Sources of Non-Recurrent Geomagnetic Storms and Forbush Decreases
- On the reliability of magnetic energy and helicity computations based on nonlinear force-free coronal magnetic field models
- Coronal dimmings associated with coronal mass ejections on the solar limb
- Using radio triangulation to understand the origin of two subsequent type II radio bursts
- 3D reconstructions of EUV wave front heights and their influence on wave kinematics
- The Neupert Effect of Flare UltraViolet and Soft X-ray Emissions
- Imaging evidence for solar wind outflows originating from a CME footpoint
- Two-stage evolution of an extended C-class eruptive flaring activity from sigmoid active region NOAA 12734: SDO and Udaipur-CALLISTO observations
- Space weather: the solar perspective -- an update to Schwenn (2006)
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