Abstract—
This paper compares features of the generation of coronal mass ejections (CMEs) with the lowest, intermediate, and highest velocities in the field of view of LASCO C2 and C3 coronagraphs found from an analysis of multi-wavelength data with high temporal and spatial resolution. The dynamics of the field characteristics in the umbra of sunspots of active regions (ARs) in which variable-velocity CMEs occur are compared based on SDO/HMI vector magnetic field measurements. It is found that there are almost no noticeable changes in field characteristics in the AR sunspots in which slow CMEs occur after the onset of the eruptive event. However, there are noticeable changes in the field intensity and inclination angles of the flux tube emerging from the umbra of the sunspot in some AR sunspots in which CMEs occur after the onset of the eruptive event. Thus, for the fast CME detected on January 7, 2014, the inclination angle of the flux tube from the umbra of one of the sunspots before the flare onset reached a maximum value of ≈4°. After the flare onset, it was less than 1°.
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REFERENCES
Brueckner, G.E., Howard, R.A., and Koomen, M.J., et al., The large angle spectroscopic coronagraph (LASCO), Sol. Phys., vol. 162, p. 1995.
D’Huys, E., Seaton, D.B., Poedts, S., and Berghmans, D., Observational characteristics of coronal mass ejections without low-coronal signatures, Astrophys. J., 2014, vol. 795, id 49.
Fainshtein, V.G. and Egorov, Ya.I., Initiation of CMEs associated with filament eruption, and the nature of CME related shocks, Adv. Space Res., 2015, vol. 55, no. 3, pp. 798–807.
Gopalswamy, N., Yashiro, S., Michalek, G., et al., The SOHO/LASCO CME catalog, Earth Moon Planets, 2009, vol. 104, pp. 295–313.
Gosling, J.T., Hildner, E., MacQueen, R.M., Munro, R.H., Poland, A.I., and Ross, C.L., The speeds of coronal mass ejection events, Sol. Phys., 1976, vol. 48, pp. 389–397.
Grechnev, V.V., Uralov, A.M., Kochanov, A.A., Kuzmenko, I.V., Prosovetsky, D.V., Egorov, Y.I., Fainshtein, V.G., and Kashapova, L.K., A tiny eruptive filament as a flux-rope progenitor and driver of a large-scale CME and wave, Sol. Phys., 2016, vol. 291, no. 4, pp. 1173–1208.
Lemen, J.R., Title, A.M., and Akin, D.J., et al., The Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO), Sol. Phys., 2012, vol. 275, pp. 17–40.
MacQueen, R.M. and Fisher, R.R., The kinematics of solar inner coronal transients, Sol. Phys., 1983, vol. 89, pp. 89–102.
Pesnell, W.D., Thompson, B.J., and Chamberlin, P.C., The Solar Dynamics Observatory (SDO), Sol. Phys., 2012, vol. 275, pp. 3–15.
Schou, J., Scherrer, P.H., and Bush, R.I., et al., Design and ground calibration of the Helioseismic and Magnetic Imager (HMI) instrument on the Solar Dynamics Observatory (SDO), Sol. Phys., 2012, vol. 275, pp. 229–259.
Sheeley, N.R.,Jr., Walters, J.H., Wang, Y.-M., and Howard, R.A., Continuous tracking of coronal outflows: Two kinds of coronal mass ejections, J. Geophys. Res., 1999, vol. 104, pp. 24 767–24 768.
Tӧrӧk, T. and Kliem, B., Numerical simulations of fast and slow coronal mass ejections, Astron. Nachr., 2007, vol. 328, no. 8, pp. 743–746.
Vršnak, B., Sudar, D., and Ruždjak, D., The CME–flare relationship: Are there really two types of CMEs?, Astron. Astrophys., 2005, vol. 435, pp. 1149–1157.
Zagainova, Yu.S. and Fainshtein, V.G., How do fast impulse CMEs related to powerful flares but unrelated to eruptive filaments appear and move?, Adv. Space Res., 2015, vol. 55, no. 3, pp. 822–834.
Zagainova, Yu.S., Fainshtein, V G, Obridko, V.N., and Rudenko, G.V., Comparison of the magnetic properties of leading and following spots and the overlying ultraviolet emission, Astron. Rep., 2017a, vol. 61, no. 6, pp. 533–549.
Zagainova, Yu.S., Fainshtein, V.G., Rudenko, G.V., and Obridko, V.N., Some features of the variation of the magnetic field characteristics in the umbra of sunspots during flares and coronal mass ejections, Geomagn. Aeron. (Engl. Transl.), 2017b, vol. 57, no. 7, pp. 835–840.
ACKNOWLEDGMENTS
We are grateful to the teams of LASCO, SDO/AIA, SDO/HMI, and GOES for the opportunity to use data from these instruments. This work was supported by the Russian Foundation for Basic Research, project nos. 17-02-300 A and 15-02-01077 A. At the Institute of Solar–Terrestrial Physics of the Siberian Branch of the Russian Academy of Sciences, this work was performed with budgetary funding of Basic Research program II.16.
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Zagainova, Y.S., Fainshtein, V.G. Comparison of Features of the Generation of Coronal Mass Ejections with Variable Velocity in the Field of View of LASCO Coronagraphs. Geomagn. Aeron. 58, 966–972 (2018). https://doi.org/10.1134/S0016793218070253
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DOI: https://doi.org/10.1134/S0016793218070253