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A Geoeffective CME Caused by the Eruption of a Quiescent Prominence on 29 September 2013

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Abstract

The eruption of a large prominence that occurred away of active regions in the SOL2013-09-29 event produced a fast coronal mass ejection (CME) and a shock wave. The event caused considerable geospace disturbances, including a proton enhancement that have been addressed in previous studies. Continuing with the analysis of this event, we focus on the development of the CME and shock wave, assess an expected geospace impact using simplest considerations, and compare the expectations with in situ measurements near Earth. The high CME speed in this non-flare-associated event was determined by a considerable reconnected flux that corresponds to a pattern established by different authors. Estimations based on a few approaches showed the reconnection flux in this event to be comparable with a typical value in flare-associated eruptions. The shock wave was most likely impulsively excited by the erupting prominence in the same way as in flare-associated events and changed to the bow-shock regime later. The trajectory calculated for this scenario reproduces the Type II emission observed from 30 MHz to 70 kHz; its interruptions were probably caused by propagation effects. Properties of the near-Earth proton enhancement are discussed considering the results of recent studies.

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Acknowledgements

We thank A.K. Kochanov, A.M. Uralov, A.V. Belov, and I.M. Chertok for their assistance and fruitful discussions. We thank the anonymous reviewer for valuable remarks.

V. Grechnev (Sections 3.3, 4.3, 5, and 6) was funded by the Russian Science Foundation under grant 18-12-00172; the development of the methods used in Sections 3.3 and 6.2 was supported by the Program of Basic Research of the RAS Presidium No. 28. I. Kuzmenko (Sections 2, 3.1, 3.2, 4.1, and 4.2) was supported by the Russian State Contract No. 075-00389-19-00.

We appreciate the NASA/SDO and the AIA and HMI science teams; the NASA’s STEREO/SECCHI science and instrument teams; the teams operating LASCO on SOHO, STEREO/WAVES, Wind/WAVES, the GOES satellites, and the Space Weather Services Culgoora Solar Observatory for the data used here. SOHO is a project of international cooperation between ESA and NASA. We thank the ACE SWEPAM, SWICS, and MAG instrument teams and the ACE Science Center for providing the ACE data. We are grateful to the team maintaining the CME Catalogs at the CDAW Data Center by NASA and the Catholic University of America in cooperation with the Naval Research Laboratory.

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  1. Institute of Solar-Terrestrial Physics SB RAS, Lermontov St. 126A, Irkutsk, 664033, Russia

    V. V. Grechnev

  2. Institute of Applied Astronomy RAS, Kutuzov Emb. 10, St. Petersburg, 191187, Russia

    I. V. Kuzmenko

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  1. V. V. Grechnev
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Grechnev, V.V., Kuzmenko, I.V. A Geoeffective CME Caused by the Eruption of a Quiescent Prominence on 29 September 2013. Sol Phys 295, 55 (2020). https://doi.org/10.1007/s11207-020-01619-x

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