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Analysis of Large Deflections of Prominence–CME Events during the Rising Phase of Solar Cycle 24

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Abstract

The analysis of the deflection of coronal mass ejection (CME) events plays an important role in the improvement of the forecasting of their geo-effectiveness. Motivated by the scarcity of comprehensive studies of CME events with a focus on the governing conditions that drive deflections during their early stages, we performed an extensive analysis of 13 CME events that exhibited large deflections during their early development in the low corona. The study was carried out by exploiting solar-corona-imaging observations at different heights and wavelengths from instruments onboard several space- and ground-based solar observatories, namely the Project for Onboard Autonomy 2 (PROBA2), Solar Dynamics Observatory (SDO), Solar TErrestrial RElations Observatory (STEREO), Solar and Heliospheric Observatory (SOHO) spacecraft, and from the National Solar Observatory (NSO). The selected events were observed between October 2010 and September 2011, to take advantage of the location in near quadrature of the STEREO spacecraft and Earth in this time period. In particular, we determined the 3D trajectory of the front envelope of the CMEs and their associated prominences with respect to their solar sources by means of a forward-modeling and tie-pointing tool, respectively. By using a potential-field source-surface model, we estimated the coronal magnetic fields of the ambient medium through which the events propagate to investigate the role of the magnetic-energy distribution in the non-radial propagation of both structures (front envelope and prominence) and in their kinematic properties. The ambient magnetic environment during the eruption and early stages of the events is found to be crucial in determining the trajectory of the CME events, in agreement with previous reports.

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Acknowledgements

M.V. Sieyra and M. Cécere acknowledge the PROBA2 Guest Investigator program grant received to carry out this work and the SWAP data provided by the PROBA2 team. M.V. Sieyra acknowledges support from CONICET as postdoc fellow. M. Cécere, H. Cremades, F.A. Iglesias, and A. Costa are members of the Carrera del Investigador Científico (CONICET). A. Sahade is doctoral fellow of CONICET. M. Cécere and A. Sahade acknowledge support from ANPCyT under grant number PICT No. 2016-2480. M. Cécere, M.V. Sieyra, and A. Sahade also acknowledge support by SECYT-UNC grant number PC No. 33620180101147CB. M.V. Sieyra, H. Cremades, and F.A. Iglesias are grateful for the support of project UTN UTI4915TC. M. Mierla, M. West, and E. D’Huys acknowledge support from the Belgian Federal Science Policy Office (BELSPO) through the ESA-PRODEX programme, grant No. 4000120800. G. Stenborg acknowledges the support from the NASA STEREO/SECCHI program NNG17PP27I. The authors are grateful to an anonymous reviewer for useful comments and suggestions. Data courtesy of NASA/SDO and the AIA science team. The SOHO/LASCO data used here are produced by a consortium of the Naval Research Laboratory (USA), Max-Planck-Institut für Aeronomie (Germany), Laboratoire d’Astrophysique de Marseille (France), and the University of Birmingham (UK). SOHO is a mission of international cooperation between ESA and NASA. The STEREO/SECCHI-EUVI, COR1, and COR2 data are produced by an international consortium of the NRL, LMSAL and NASA GSFC (USA), RAL and Univ. Birmingham (UK), MPS (Germany), CSL (Belgium), IOTA and IAS (France). This work utilizes data from the National Solar Observatory Integrated Synoptic Program, which is operated by the Association of Universities for Research in Astronomy, under a cooperative agreement with the National Science Foundation and with additional financial support from the National Oceanic and Atmospheric Administration, the National Aeronautics and Space Administration, and the United States Air Force. The GONG network of instruments is hosted by the Big Bear Solar Observatory, High Altitude Observatory, Learmonth Solar Observatory, Udaipur Solar Observatory, Instituto de Astrofísica de Canarias, and Cerro Tololo Interamerican Observatory.

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Authors and Affiliations

  1. Universidad Tecnológica Nacional – Facultad Regional Mendoza, CONICET, CEDS, Rodriguez 243, Mendoza, Argentina

    M. Valeria Sieyra, Hebe Cremades & Francisco A. Iglesias

  2. Instituto de Astronomía Teórica y Experimental, CONICET-UNC, Córdoba, Argentina

    Mariana Cécere, Abril Sahade & Andrea Costa

  3. Solar-Terrestrial Center of Excellence—SIDC, Royal Observatory of Belgium, Brussels, Belgium

    Marilena Mierla, Matthew J. West & Elke D’Huys

  4. Institute of Geodynamics of the Romanian Academy, Bucharest, Romania

    Marilena Mierla

  5. Space Science Division, US Naval Research Laboratory, Washington, DC, 20375, USA

    Guillermo Stenborg

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  1. M. Valeria Sieyra
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  2. Mariana Cécere
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  3. Hebe Cremades
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  4. Francisco A. Iglesias
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  5. Abril Sahade
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  6. Marilena Mierla
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  7. Guillermo Stenborg
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  8. Andrea Costa
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  9. Matthew J. West
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  10. Elke D’Huys
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Correspondence to M. Valeria Sieyra.

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PROBA-2 at Ten Years

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Sieyra, M.V., Cécere, M., Cremades, H. et al. Analysis of Large Deflections of Prominence–CME Events during the Rising Phase of Solar Cycle 24. Sol Phys 295, 126 (2020). https://doi.org/10.1007/s11207-020-01694-0

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