Abstract
We present a study of the complex event consisting of several solar wind transients detected by the Advanced Composition Explorer (ACE) on 4 – 7 August 2011, which caused a geomagnetic storm with \(\mathit{Dst}=-110~\mbox{nT}\). The supposed coronal sources, three flares and coronal mass ejections (CMEs), occurred on 2 – 4 August 2011 in active region (AR) 11261. To investigate the solar origin and formation of these transients, we study the kinematic and thermodynamic properties of the expanding coronal structures using the Solar Dynamics Observatory/Atmospheric Imaging Assembly (SDO/AIA) EUV images and differential emission measure (DEM) diagnostics. The Helioseismic and Magnetic Imager (HMI) magnetic field maps were used as the input data for the 3D magnetohydrodynamic (MHD) model to describe the flux rope ejection (Pagano, Mackay, and Poedts, 2013b). We characterize the early phase of the flux rope ejection in the corona, where the usual three-component CME structure formed. The flux rope was ejected with a speed of about \(200~\mbox{km}\,\mbox{s}^{-1}\) to the height of \(0.25~\mbox{R}_{\odot}\). The kinematics of the modeled CME front agrees well with the Solar Terrestrial Relations Observatory (STEREO) EUV measurements. Using the results of the plasma diagnostics and MHD modeling, we calculate the ion charge ratios of carbon and oxygen as well as the mean charge state of iron ions of the 2 August 2011 CME, taking into account the processes of heating, cooling, expansion, ionization, and recombination of the moving plasma in the corona up to the frozen-in region. We estimate a probable heating rate of the CME plasma in the low corona by matching the calculated ion composition parameters of the CME with those measured in situ for the solar wind transients. We also consider the similarities and discrepancies between the results of the MHD simulation and the observations.
Similar content being viewed by others
Notes
References
Akmal, A., Raymond, J.C., Vourlidas, A., Thompson, B., Ciaravella, A., Ko, Y.-K., Uzzo, M., Wu, R.: 2001, SOHO observations of a coronal mass ejection. Astrophys. J. 553, 922. DOI . ADS .
Arge, C.N., Pizzo, V.J.: 2000, Improvement in the prediction of solar wind conditions using near-real time solar magnetic field updates. J. Geophys. Res. 105, 10465. DOI . ADS .
Borgazzi, A., Lara, A., Echer, E., Alves, M.V.: 2009, Dynamics of coronal mass ejections in the interplanetary medium. Astron. Astrophys. 498, 885. DOI . ADS .
Bothmer, V., Schwenn, R.: 1998, The structure and origin of magnetic clouds in the solar wind. Ann. Geophys. 16, 1. DOI . ADS .
Brueckner, G.E., Howard, R.A., Koomen, M.J., Korendyke, C.M., Michels, D.J., Moses, J.D., Socker, D.G., Dere, K.P., Lamy, P.L., Llebaria, A., Bout, M.V., Schwenn, R., Simnett, G.M., Bedford, D.K., Eyles, C.J.: 1995, The Large Angle Spectroscopic Coronagraph (LASCO). Solar Phys. 162, 357. DOI . ADS .
Cargill, P.J.: 2004, On the aerodynamic drag force acting on interplanetary coronal mass ejections. Solar Phys. 221, 135. DOI . ADS .
Cargill, P.J., Chen, J., Spicer, D.S., Zalesak, S.T.: 1996, Magnetohydrodynamic simulations of the motion of magnetic flux tubes through a magnetized plasma. J. Geophys. Res. 101, 4855. DOI . ADS .
Cheng, X., Zhang, J., Liu, Y., Ding, M.D.: 2011, Observing flux rope formation during the impulsive phase of a solar eruption. Astrophys. J. Lett. 732, L25. DOI . ADS .
Cheng, X., Zhang, J., Saar, S.H., Ding, M.D.: 2012, Differential emission measure analysis of multiple structural components of coronal mass ejections in the inner corona. Astrophys. J. 761, 62. DOI . ADS .
Cheng, X., Zhang, J., Ding, M.D., Liu, Y., Poomvises, W.: 2013, The driver of coronal mass ejections in the low corona: A flux rope. Astrophys. J. 763, 43. DOI . ADS .
Ciaravella, A., Raymond, J.C., Reale, F., Strachan, L., Peres, G.: 2001, 1997 December 12 helical coronal mass ejection. II. Density, energy estimates, and hydrodynamics. Astrophys. J. 557, 351. DOI . ADS .
Colaninno, R.C., Vourlidas, A.: 2009, First determination of the true mass of coronal mass ejections: A novel approach to using the two STEREO viewpoints. Astrophys. J. 698, 852. DOI . ADS .
Colaninno, R.C., Vourlidas, A.: 2015, Using multiple-viewpoint observations to determine the interaction of three coronal mass ejections observed on 2012 March 5. Astrophys. J. 815, 70. DOI . ADS .
Cremades, H., Bothmer, V.: 2004, On the three-dimensional configuration of coronal mass ejections. Astron. Astrophys. 422, 307. DOI . ADS .
DeForest, C.E., Howard, T.A., McComas, D.J.: 2013, Tracking coronal features from the low corona to Earth: A quantitative analysis of the 2008 December 12 coronal mass ejection. Astrophys. J. 769, 43. DOI . ADS .
Dere, K.P.: 2007, Ionization rate coefficients for the elements hydrogen through zinc. Astron. Astrophys. 466, 771. DOI . ADS .
Dere, K.P., Landi, E., Young, P.R., Del Zanna, G., Landini, M., Mason, H.E.: 2009, CHIANTI – an atomic database for emission lines. IX. ionization rates, recombination rates, ionization equilibria for the elements hydrogen through zinc and updated atomic data. Astron. Astrophys. 498, 915. DOI . ADS .
Feldman, U., Landi, E., Schwadron, N.A.: 2005, On the sources of fast and slow solar wind. J. Geophys. Res. 110, A07109. DOI . ADS .
Fisk, L.A., Schwadron, N.A., Zurbuchen, T.H.: 1998, On the slow solar wind. Space Sci. Rev. 86, 51. DOI . ADS .
Gibb, G.P.S., Mackay, D.H., Green, L.M., Meyer, K.A.: 2014, Simulating the formation of a sigmoidal flux rope in AR10977 from SOHO/MDI magnetograms. Astrophys. J. 782, 71. DOI . ADS .
Gopalswamy, N., Lara, A., Lepping, R.P., Kaiser, M.L., Berdichevsky, D., St. Cyr, O.C.: 2000, Interplanetary acceleration of coronal mass ejections. Geophys. Res. Lett. 27, 145. DOI . ADS .
Gopalswamy, N., Mäkelä, P., Xie, H., Akiyama, S., Yashiro, S.: 2009a, CME interactions with coronal holes and their interplanetary consequences. J. Geophys. Res. 114, A00A22. DOI . ADS .
Gopalswamy, N., Mäkelä, P., Xie, H., Akiyama, S., Yashiro, S.: 2009b, CME interactions with coronal holes and their interplanetary consequences. J. Geophys. Res. 114, A00A22. DOI . ADS .
Gopalswamy, N., Mäkelä, P., Xie, H., Yashiro, S.: 2013, Testing the empirical shock arrival model using quadrature observations. Space Weather 11, 661. DOI . ADS .
Goryaev, F.F., Parenti, S., Urnov, A.M., Oparin, S.N., Hochedez, J.-F., Reale, F.: 2010, An iterative method in a probabilistic approach to the spectral inverse problem. Differential emission measure from line spectra and broadband data. Astron. Astrophys. 523, A44. DOI . ADS .
Gosling, J.T.: 1990, Coronal Mass Ejections and Magnetic Flux Ropes in Interplanetary Space, AGU Monograph Ser. 58, 343. ADS .
Gruesbeck, J.R., Lepri, S.T., Zurbuchen, T.H., Antiochos, S.K.: 2011, Constraints on coronal mass ejection evolution from in situ observations of ionic charge states. Astrophys. J. 730, 103. DOI . ADS .
Howard, R.A., Moses, J.D., Vourlidas, A., Newmark, J.S., Socker, D.G., Plunkett, S.P., et al.: 2008, Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI). Space Sci. Rev. 136, 67. DOI . ADS .
Hundhausen, A.J., Gilbert, H.E., Bame, S.J.: 1968, Ionization state of the interplanetary plasma. J. Geophys. Res. 73, 5485. DOI .
Jian, L.K., MacNeice, P.J., Taktakishvili, A., Odstrcil, D., Jackson, B., Yu, H.S., Riley, P., Sokolov, I.V., Evans, R.M.: 2015, Validation for solar wind prediction at Earth: Comparison of coronal and heliospheric models installed at the CCMC. Space Weather 13, 316. DOI .
Kilpua, E.K.J., Luhmann, J.G., Jian, L.K., Russell, C.T., Li, Y.: 2014, Why have geomagnetic storms been so weak during the recent solar minimum and the rising phase of cycle 24? J. Atmos. Solar-Terr. Phys. 107, 12. DOI . ADS .
Ko, Y.-K., Fisk, L.A., Geiss, J., Gloeckler, G., Guhathakurta, M.: 1997, An empirical study of the electron temperature and heavy ion velocities in the south polar coronal hole. Solar Phys. 171, 345. ADS .
Kumar, A., Rust, D.M.: 1996, Interplanetary magnetic clouds, helicity conservation, and current-core flux-ropes. J. Geophys. Res. 101, 15667. DOI . ADS .
Lara, A., Borgazzi, A.I.: 2009, Dynamics of interplanetary CMEs and associated type II bursts. In: Gopalswamy, N., Webb, D.F. (eds.) Universal Heliophysical Processes, IAU Symp. 257, 287. DOI . ADS .
Lee, J.-Y., Raymond, J.C., Ko, Y.-K., Kim, K.-S.: 2009, Three-dimensional structure and energy balance of a coronal mass ejection. Astrophys. J. 692, 1271. DOI . ADS .
Lemen, J.R., Title, A.M., Akin, D.J., Boerner, P.F., Chou, C., Drake, J.F., et al.: 2012, The Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO). Solar Phys. 275, 17. DOI . ADS .
Lepri, S.T., Laming, J.M., Rakowski, C.E., von Steiger, R.: 2012, Spatially dependent heating and ionization in an ICME observed by both ACE and Ulysses. Astrophys. J. 760, 105. DOI . ADS .
Lugaz, N., Farrugia, C.J., Davies, J.A., Möstl, C., Davis, C.J., Roussev, I.I., Temmer, M.: 2012, The deflection of the two interacting coronal mass ejections of 2010 May 23 – 24 as revealed by combined in situ measurements and heliospheric imaging. Astrophys. J. 759, 68. DOI . ADS .
Lynch, B.J., Reinard, A.A., Mulligan, T., Reeves, K.K., Rakowski, C.E., Allred, J.C., Li, Y., Laming, J.M., MacNeice, P.J., Linker, J.A.: 2011, Ionic composition structure of coronal mass ejections in axisymmetric magnetohydrodynamic models. Astrophys. J. 740, 112. DOI . ADS .
Mackay, D.H., Green, L.M., van Ballegooijen, A.: 2011, Modeling the dispersal of an active region: Quantifying energy input into the corona. Astrophys. J. 729, 97. DOI . ADS .
Mäkelä, P., Gopalswamy, N., Xie, H., Mohamed, A.A., Akiyama, S., Yashiro, S.: 2013, Coronal hole influence on the observed structure of interplanetary CMEs. Solar Phys. 284, 59. DOI . ADS .
Manoharan, P.K.: 2010, Ooty interplanetary scintillation – Remote-sensing observations and analysis of coronal mass ejections in the heliosphere. Solar Phys. 265, 137. DOI . ADS .
Mays, M.L., Taktakishvili, A., Pulkkinen, A., MacNeice, P.J., Rastätter, L., Odstrcil, D., Jian, L.K., Richardson, I.G., LaSota, J.A., Zheng, Y., Kuznetsova, M.M.: 2015, Ensemble modeling of CMEs using the WSA-ENLIL+Cone model. Solar Phys. 290, 1775. DOI . ADS .
McNeice, P., Elliot, B., Acebal, A.: 2011, Validation of community models. Space Weather 9, S10003. DOI .
Mohamed, A.A., Gopalswamy, N., Yashiro, S., Akiyama, S., Mäkelä, P., Xie, H., Jung, H.: 2012, The relation between coronal holes and coronal mass ejections during the rise, maximum, and declining phases of Solar Cycle 23. J. Geophys. Res. 117, A01103. DOI . ADS .
Möstl, C., Farrugia, C.J., Kilpua, E.K.J., Jian, L.K., Liu, Y., Eastwood, J.P., Harrison, R.A., Webb, D.F., Temmer, M., Odstrcil, D., Davies, J.A., Rollett, T., Luhmann, J.G., Nitta, N., Mulligan, T., Jensen, E.A., Forsyth, R., Lavraud, B., de Koning, C.A., Veronig, A.M., Galvin, A.B., Zhang, T.L., Anderson, B.J.: 2012, Multi-point shock and flux rope analysis of multiple interplanetary coronal mass ejections around 2010 August 1 in the inner heliosphere. Astrophys. J. 758, 10. DOI . ADS .
Nindos, A., Patsourakos, S., Vourlidas, A., Tagikas, C.: 2015, How common are hot magnetic flux ropes in the low solar corona? A statistical study of EUV observations. Astrophys. J. 808, 117. DOI . ADS .
Nolte, J.T., Roelof, E.C.: 1973, Large-scale structure of the interplanetary medium, I: High coronal source longitude of the quiet-time solar wind. Solar Phys. 33, 241. DOI . ADS .
Odstrčil, D.: 1994, Interactions of solar wind streams and related small structures. J. Geophys. Res. 99, 17. DOI . ADS .
Odstrčil, D., Pizzo, V.J.: 1999, Three-dimensional propagation of CMEs in a structured solar wind flow: 1. CME launched within the streamer belt. J. Geophys. Res. 104, 483. DOI . ADS .
Odstrčil, D., Dryer, M., Smith, Z.: 1996, Propagation of an interplanetary shock along the heliospheric plasma sheet. J. Geophys. Res. 101, 19973. DOI . ADS .
Owens, M., Cargill, P.: 2004, Predictions of the arrival time of coronal mass ejections at 1AU: an analysis of the causes of errors. Ann. Geophys. 22, 661. DOI . ADS .
Pagano, P., Mackay, D.H., Poedts, S.: 2013a, Effect of gravitational stratification on the propagation of a CME. Astron. Astrophys. 560, A38. DOI . ADS .
Pagano, P., Mackay, D.H., Poedts, S.: 2013b, Magnetohydrodynamic simulations of the ejection of a magnetic flux rope. Astron. Astrophys. 554, A77. DOI . ADS .
Pagano, P., Mackay, D.H., Poedts, S.: 2014, Simulating AIA observations of a flux rope ejection. Astron. Astrophys. 568, A120. DOI . ADS .
Pagano, P., Reale, F., Orlando, S., Peres, G.: 2007, MHD evolution of a fragment of a CME core in the outer solar corona. Astron. Astrophys. 464, 753. DOI . ADS .
Pagano, P., Raymond, J.C., Reale, F., Orlando, S.: 2008, Modeling magnetohydrodynamics and non-equilibrium SoHO/UVCS line emission of CME shocks. Astron. Astrophys. 481, 835. DOI . ADS .
Pizzo, V., Millward, G., Parsons, A., Biesecker, D., Hill, S., Odstrcil, D.: 2011, Wang–Sheeley–Arege–Enlil cone model transitions to operations. Space Weather 9, S033004. DOI .
Porth, O., Xia, C., Hendrix, T., Moschou, S.P., Keppens, R.: 2014, MPI-AMRVAC for solar and astrophysics. Astron. Astrophys. Suppl. 214, 4. DOI . ADS .
Reinard, A.A., Lynch, B.J., Mulligan, T.: 2012, Composition structure of interplanetary coronal mass ejections from multispacecraft observations, modeling, and comparison with numerical simulations. Astrophys. J. 761, 175. DOI . ADS .
Richardson, I.G., Cane, H.V.: 2004, The fraction of interplanetary coronal mass ejections that are magnetic clouds: Evidence for a solar cycle variation. Geophys. Res. Lett. 31, L18804. DOI . ADS .
Richardson, I.G., Cane, H.V.: 2010, Near-Earth interplanetary coronal mass ejections during Solar Cycle 23 (1996 – 2009): Catalog and summary of properties. Solar Phys. 264, 189. DOI . ADS .
Schou, J., Scherrer, P.H., Bush, R.I., Wachter, R., Couvidat, S., Rabello-Soares, M.C., Bogart, R.S., Hoeksema, J.T., Liu, Y., Duvall, T.L., Akin, D.J., Allard, B.A., Miles, J.W., Rairden, R., Shine, R.A., Tarbell, T.D., Title, A.M., Wolfson, C.J., Elmore, D.F., Norton, A.A., Tomczyk, S.: 2012, Design and ground calibration of the Helioseismic and Magnetic Imager (HMI) instrument on the Solar Dynamics Observatory (SDO). Solar Phys. 275, 229. DOI . ADS .
Shi, T., Wang, Y., Wan, L., Cheng, X., Ding, M., Zhang, J.: 2015, Predicting the arrival time of coronal mass ejections with the graduated cylindrical shell and drag force model. Astrophys. J. 806, 271. DOI . ADS .
Stone, E.C., Frandsen, A.M., Mewaldt, R.A., Christian, E.R., Margolies, D., Ormes, J.F., Snow, F.: 1998, The advanced composition explorer. Space Sci. Rev. 86, 1. DOI . ADS .
Temmer, M., Vršnak, B., Rollett, T., Bein, B., de Koning, C.A., Liu, Y., Bosman, E., Davies, J.A., Möstl, C., Žic, T., Veronig, A.M., Bothmer, V., Harrison, R., Nitta, N., Bisi, M., Flor, O., Eastwood, J., Odstrcil, D., Forsyth, R.: 2012, Characteristics of kinematics of a coronal mass ejection during the 2010 August 1 CME–CME interaction event. Astrophys. J. 749, 57. DOI . ADS .
Urnov, A.M., Goryaev, F., Oparin, S.: 2012, On spectroscopic diagnostics of hot optically thin plasmas. In: Shevelko, V., Tawara, H. (eds.) Atomic Processes in Basic and Applied Physics, Springer Series on Atomic, Optical, and Plasma Physics 68, 249. DOI . ADS .
Urnov, A.M., Goryaev, F.F., Bertschinger, G., Kunze, H.J., Marchuk, O.: 2007, On the verification of atomic data for \(K_{\alpha}\) radiation spectra from the TEXTOR tokamak. JETP Lett. 85, 374. DOI .
Vršnak, B.: 2001, Deceleration of coronal mass ejections. Solar Phys. 202, 173. DOI . ADS .
Vršnak, B., Žic, T.: 2007, Transit times of interplanetary coronal mass ejections and the solar wind speed. Astron. Astrophys. 472, 937. DOI . ADS .
Vršnak, B., Vrbanec, D., Čalogović, J.: 2008, Dynamics of coronal mass ejections. The mass-scaling of the aerodynamic drag. Astron. Astrophys. 490, 811. DOI . ADS .
Vršnak, B., Ruždjak, D., Sudar, D., Gopalswamy, N.: 2004, Kinematics of coronal mass ejections between 2 and 30 solar radii. What can be learned about forces governing the eruption? Astron. Astrophys. 423, 717. DOI . ADS .
Vršnak, B., Žic, T., Falkenberg, T.V., Möstl, C., Vennerstrom, S., Vrbanec, D.: 2010, The role of aerodynamic drag in propagation of interplanetary coronal mass ejections. Astron. Astrophys. 512, A43. DOI . ADS .
Vršnak, B., Žic, T., Vrbanec, D., Temmer, M., Rollett, T., Möstl, C., Veronig, A., Čalogović, J., Dumbović, M., Lulić, S., Moon, Y.-J., Shanmugaraju, A.: 2013, Propagation of interplanetary coronal mass ejections: The drag-based model. Solar Phys. 285, 295. DOI . ADS .
Wang, Y.-M.: 2012, Semiempirical models of the slow and fast solar wind. Space Sci. Rev. 172, 123. DOI . ADS .
Webb, D.F., Howard, T.A.: 2012, Coronal mass ejections: Observations. Living Rev. Solar Phys. 9, 3. DOI . ADS .
Wood, B.E., Wu, C.-C., Rouillard, A.P., Howard, R.A., Socker, D.G.: 2012, A coronal hole’s effects on coronal mass ejection shock morphology in the inner heliosphere. Astrophys. J. 755, 43. DOI . ADS .
Yiğit, E., Frey, H.U., Moldwin, M.B., Immel, T.J., Ridley, A.J.: 2016, Hemispheric differences in the response of the upper atmosphere to the August 2011 geomagnetic storm: A simulation study. J. Atmos. Solar-Terr. Phys. 141, 13. DOI . ADS .
Zhang, J., Cheng, X., Ding, M.-D.: 2012, Observation of an evolving magnetic flux rope before and during a solar eruption. Nat. Commun. 3, 747. DOI . ADS .
Zhao, L., Zurbuchen, T.H., Fisk, L.A.: 2009, Global distribution of the solar wind during solar cycle 23: ACE observations. Geophys. Res. Lett. 36, L14104. DOI . ADS .
Zhao, L., Landi, E., Zurbuchen, T.H., Fisk, L.A., Lepri, S.T.: 2014, The evolution of 1 AU equatorial solar wind and its association with the morphology of the heliospheric current sheet from Solar Cycles 23 to 24. Astrophys. J. 793, 44. DOI . ADS .
Zurbuchen, T.H., Richardson, I.G.: 2006, In-situ solar wind and magnetic field signatures of interplanetary coronal mass ejections. Space Sci. Rev. 123, 31. DOI . ADS .
Acknowledgements
The authors are grateful to Jie Zhang and Nat Gopalswamy as the ISEST coordinators for supporting our studies of coronal sources of ICMEs. We thank Ian Richardson and Hilary Cane for their list of Near-Earth Interplanetary Coronal Mass Ejections,Footnote 7 CDAW Data Centre,Footnote 8 and CACTus software package,Footnote 9 which we used in our investigations. The authors thank the GOES, SDO/AIA, and ACE research teams for their open data policy. We are grateful for the opportunity to use the results of the simulation obtained by the WSA-Enlil Cone and DBM models.Footnote 10 This project has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No. 647214). We acknowledge the use of the open source ( gitorious.org/amrvac ) MPI-AMRVAC software, relying on coding efforts from C. Xia, O. Porth, and R. Keppens. The computational work for this article was carried out on the joint STFC and SFC (SRIF) funded clusters at the University of St Andrews (Scotland, UK). The work is partially supported by RFBR grants 17-02-00787, 14-02-00945 and the P7 Program of the Russian Academy of Sciences.
Author information
Authors and Affiliations
Corresponding author
Ethics declarations
Disclosure of Potential Conflicts of Interest
The authors declare that they have no conflicts of interest.
Additional information
Earth-affecting Solar Transients
Guest Editors: Jie Zhang, Xochitl Blanco-Cano, Nariaki Nitta, and Nandita Srivastava
Electronic Supplementary Material
Below are the links to the electronic supplementary material.
Rights and permissions
About this article
Cite this article
Rodkin, D., Goryaev, F., Pagano, P. et al. Origin and Ion Charge State Evolution of Solar Wind Transients during 4 – 7 August 2011. Sol Phys 292, 90 (2017). https://doi.org/10.1007/s11207-017-1109-0
Received:
Accepted:
Published:
DOI: https://doi.org/10.1007/s11207-017-1109-0