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Magneto-Acoustic Energetics Study of the Seismically Active Flare of 15 February 2011

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Abstract

Multi-wavelength studies of energetic solar flares with seismic emissions have revealed interesting common features between them. We studied the first GOES X-class flare of Solar Cycle 24, as detected by the Solar Dynamics Observatory (SDO). For context, seismic activity from this flare (SOL2011-02-15T01:55-X2.2, in NOAA AR 11158) has been reported by Kosovichev (Astrophys. J. Lett., 734, L15, 2011) and Zharkov et al. (Astrophys. J. Lett., 741, L35, 2011). Based on Dopplergram data from the Helioseismic and Magnetic Imager (HMI), we applied standard methods of local helioseismology in order to identify the seismic sources in this event. RHESSI hard X-ray data are used to check the correlation between the location of the seismic sources and the particle-precipitation sites in during the flare. Using HMI magnetogram data, the temporal profile of fluctuations in the photospheric line-of-sight magnetic field is used to estimate the magnetic-field change in the region where the seismic signal was observed. This leads to an estimate of the work done by the Lorentz-force transient on the photosphere of the source region. In this instance, this is found to be a significant fraction of the acoustic energy in the attendant seismic emission, suggesting that Lorentz forces can contribute significantly to the generation of sunquakes. However, there are regions in which the signature of the Lorentz force is much stronger, but from which no significant acoustic emission emanates.

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Notes

  1. Because B los varies considerably across the source region, the mean of B losΔB los can be considerably different from the product of the means used as a proxy in Equation (7). The error could be of order 100 %. However, we think that it is unlikely to be anything like an order of magnitude.

References

  • Beşliu-Ionescu, D., Donea, A.-C., Cally, P., Lindsey, C.: 2006, Significant acoustic activity in AR10720 on January 15, 2005. Rom. Astron. J. 16, 203.

    Google Scholar 

  • Donea, A.-C., Lindsey, C.: 2005, Seismic emission from the solar flares of 2003 October 28 and 29. Astrophys. J. 630, 1168 – 1183. doi: 10.1086/432155 .

    Article  ADS  Google Scholar 

  • Donea, A.-C., Braun, D.C., Lindsey, C.: 1999, Seismic images of a solar flare. Astrophys. J. Lett. 513, L143 – L146. doi: 10.1086/311915 .

    Article  ADS  Google Scholar 

  • Donea, A.-C., Lindsey, C., Braun, D.C.: 2000, Stochastic seismic emission from acoustic glories and the quiet Sun. Solar Phys. 192, 321 – 333. doi: 10.1023/A:1005280327665 .

    Article  ADS  Google Scholar 

  • Donea, A.-C., Besliu-Ionescu, D., Cally, P.S., Lindsey, C., Zharkova, V.V.: 2006, Seismic emission from A M9.5-class solar flare. Solar Phys. 239, 113 – 135. doi: 10.1007/s11207-006-0108-3 .

    Article  ADS  Google Scholar 

  • Fisher, G.H., Bercik, D.J., Welsch, B.T., Hudson, H.S.: 2012, Global forces in eruptive solar flares: The Lorentz force acting on the solar atmosphere and the solar interior. Solar Phys. 277, 59 – 76. doi: 10.1007/s11207-011-9907-2 .

    Article  ADS  Google Scholar 

  • Hudson, H.S.: 2000, Implosions in coronal transients. Astrophys. J. Lett. 531, L75 – L77. doi: 10.1086/312516 .

    Article  ADS  Google Scholar 

  • Hudson, H.S., Fisher, G.H., Welsch, B.T.: 2008, Flare energy and magnetic field variations. In: Howe, R., Komm, R.W., Balasubramaniam, K.S., Petrie, G.J.D. (eds.) Subsurface and Atmospheric Influences on Solar Activity CS-383, Astron. Soc. Pacific, San Francisco, 221.

    Google Scholar 

  • Hurford, G.J., Schmahl, E.J., Schwartz, R.A., Conway, A.J., Aschwanden, M.J., Csillaghy, A., Dennis, B.R., Johns-Krull, C., Krucker, S., Lin, R.P., McTiernan, J., Metcalf, T.R., Sato, J., Smith, D.M.: 2002, The RHESSI imaging concept. Solar Phys. 210, 61 – 86. doi: 10.1023/A:1022436213688 .

    Article  ADS  Google Scholar 

  • Kosovichev, A.G.: 2011, Helioseismic response to the X2.2 solar flare of 2011 February 15. Astrophys. J. Lett. 734, L15. doi: 10.1088/2041-8205/734/1/L15 .

    Article  ADS  Google Scholar 

  • Kosovichev, A.G., Zharkova, V.V.: 1998, X-ray flare sparks quake inside Sun. Nature 393, 317 – 318. doi: 10.1038/30629 .

    Article  ADS  Google Scholar 

  • Lindsey, C., Braun, D.C.: 2000, Basic principles of solar acoustic holography (Invited Review). Solar Phys. 192, 261 – 284. doi: 10.1023/A:1005227200911 .

    Article  ADS  Google Scholar 

  • Martínez-Oliveros, J.C., Moradi, H., Donea, A.-C.: 2008, Seismic emissions from a highly impulsive M6.7 solar flare. Solar Phys. 251, 613 – 626. doi: 10.1007/s11207-008-9122-y .

    Article  ADS  Google Scholar 

  • Martínez-Oliveros, J.C., Moradi, H., Besliu-Ionescu, D., Donea, A.-C., Cally, P.S., Lindsey, C.: 2007, From gigahertz to millihertz: A multiwavelength study of the acoustically active 14 August 2004 M7.4 solar flare. Solar Phys. 245, 121 – 139. doi: 10.1007/s11207-007-9004-8 .

    Article  ADS  Google Scholar 

  • Moradi, H., Donea, A.-C., Lindsey, C., Besliu-Ionescu, D., Cally, P.S.: 2007, Helioseismic analysis of the solar flare-induced sunquake of 2005 January 15. Mon. Not. Roy. Astron. Soc. 374, 1155 – 1163. doi: 10.1111/j.1365-2966.2006.11234.x .

    Article  ADS  Google Scholar 

  • Schou, J., Borrero, J.M., Norton, A.A., Tomczyk, S., Elmore, D., Card, G.L.: 2012, Polarization Calibration of the Helioseismic and Magnetic Imager (HMI) onboard the Solar Dynamics Observatory (SDO). Solar Phys. 275, 327 – 355. doi: 10.1007/s11207-010-9639-8 .

    Article  ADS  Google Scholar 

  • Sudol, J.J., Harvey, J.W.: 2005, Longitudinal magnetic field changes accompanying solar flares. Astrophys. J. 635, 647 – 658. doi: 10.1086/497361 .

    Article  ADS  Google Scholar 

  • Zharkov, S., Green, L.M., Matthews, S.A., Zharkova, V.V.: 2011, 2011 February 15: Sunquakes produced by flux rope eruption. Astrophys. J. Lett. 741, L35. doi: 10.1088/2041-8205/741/2/L35 .

    Article  ADS  Google Scholar 

  • Zharkova, V.V.: 2008, The mechanisms of particle kinetics and dynamics leading to seismic emission and sunquakes. Solar Phys. 251, 665 – 666. doi: 10.1007/s11207-008-9266-9 .

    Article  ADS  Google Scholar 

  • Zharkova, V.V., Zharkov, S.I.: 2007, On the origin of three seismic sources in the proton-rich flare of 2003 October 28. Astrophys. J. 664, 573 – 585. doi: 10.1086/518731 .

    Article  ADS  Google Scholar 

  • Zharkova, V.V., Zharkov, S.I., Ipson, S.S., Benkhalil, A.K.: 2005, Toward magnetic field dissipation during the 23 July 2002 solar flare measured with Solar and Heliospheric Observatory/Michelson Doppler Imager (SOHO/MDI) and Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSIgr). J. Geophys. Res. 110(A9), 8104. doi: 10.1029/2004JA010934 .

    Article  Google Scholar 

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Acknowledgements

The Berkeley group was supported by NASA under contract NNX11AP05G. Special thanks to K.D. Leka and Graham Barnes for their helpful comments and discussion to improve the ideas presented in this work.

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Correspondence to J. D. Alvarado-Gómez.

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Advances in European Solar Physics

Guest Editors: Valery M. Nakariakov, Manolis K. Georgoulis, and Stefaan Poedts

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Alvarado-Gómez, J.D., Buitrago-Casas, J.C., Martínez-Oliveros, J.C. et al. Magneto-Acoustic Energetics Study of the Seismically Active Flare of 15 February 2011. Sol Phys 280, 335–345 (2012). https://doi.org/10.1007/s11207-012-0009-6

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