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All issues Volume 5 (2015) J. Space Weather Space Clim., 5 (2015) A20 References
Issue
J. Space Weather Space Clim.
Volume 5, 2015
Statistical Challenges in Solar Information Processing
Article Number A20
Number of page(s) 12
DOI https://doi.org/10.1051/swsc/2015021
Published online 07 July 2015
  • Billings, D.E. A guide to the solar corona. Academic Press, New York, 150, 1966. [Google Scholar]
  • Burlaga, L., R. Fitzenreiter, R. Lepping, K. Ogilvie, A. Szabo, et al. A magnetic cloud containing prominence material – January 1997. J. Geophys. Res., 103, 277, 1998. [NASA ADS] [CrossRef] [Google Scholar]
  • Burlaga, L.F.E. Magnetic Clouds. In: R. Schwenn, and E. Marsch, Editors, Physics of the Inner Heliosphere II, Springer, Berlin, 1–2, 1991. [CrossRef] [Google Scholar]
  • Cargill, P.J. On the aerodynamic drag force acting on interplanetary coronal mass ejections. Sol. Phys., 221, 135–149, 2004. [NASA ADS] [CrossRef] [Google Scholar]
  • Cargill, P.J., J. Chen, D.S. Spicer, and S.T. Zalesak. Magnetohydrodynamic simulations of the motion of magnetic flux tubes through a magnetized plasma. J. Geophys. Res., 101, 4855–4870, 1996. [Google Scholar]
  • Colaninno, R.C., A. Vourlidas, and C.C. Wu. Quantitative comparison of methods for predicting the arrival of coronal mass ejections at Earth based on multiview imaging. J. Geophys. Res., 118, 6866–6879, 2013. [Google Scholar]
  • Crooker, N.U., and T.S. Horbury. Solar imprint on ICMEs, their magnetic connectivity, and heliospheric evolution. Space Sci. Rev., 123, 93–109, 2006. [Google Scholar]
  • Davies, J.A., R.A. Harrison, A.P. Rouillard, N.R. Sheeley, C.H. Perry, et al. A synoptic view of solar transient evolution in the inner heliosphere using the Heliospheric Imagers on STEREO. Geophys. Res. Lett., 36, L02102, 2009. [NASA ADS] [CrossRef] [Google Scholar]
  • Davies, J.A., R.A. Harrison, C.H. Perry, C. Möstl, N. Lugaz, et al. A self-similar expansion model for use in solar wind transient propagation studies. Astrophys. J., 750, 23, 2012. [Google Scholar]
  • Davies, J.A., C.H. Perry, R.M.G.M. Trines, R.A. Harrison, N. Lugaz, C. Möstl, Y.D. Liu, and K. Steed. Establishing a stereoscopic technique for determining the kinematic properties of solar wind transients based on a generalised self-similarly expanding circular geometry. Astrophys. J., 777, 167, 2013. [Google Scholar]
  • Davis, C.J., J.A. Davies, M. Lockwood, A.P. Rouillard, C.J. Eyles, and R.A. Harrison. Stereoscopic imaging of an Earth-impacting solar coronal mass ejection: a major milestone for the STEREO mission. Geophys. Res. Lett., 36, L08102, 2009. [Google Scholar]
  • Davis, C.J., J. Kennedy, and J.A. Davies. Assessing the accuracy of CME Speed and trajectory estimates from STEREO observations through a comparison of independent methods. Sol. Phys., 263, 209–222, 2010. [NASA ADS] [CrossRef] [Google Scholar]
  • DeForest, C.E., T.A. Howard, and S.J. Tappin. Observations of detailed structure in the solar wind at 1 AU with STEREO/HI-2. Astrophys. J., 738, 103, 2011. [Google Scholar]
  • Eyles, C.J., R.A. Harrison, C.J. Davis, N.R. Waltham, B.M. Shaughnessy, et al. The heliospheric imagers onboard the STEREO mission. Sol. Phys., 254, 387–445, 2009. [NASA ADS] [CrossRef] [Google Scholar]
  • Forsyth, R.J., V. Bothmer, C. Cid, N.U. Crooker, T.S. Horbury, et al. ICMEs in the inner heliosphere: origin, evolution and propagation effects. report of working group G. Space Sci. Rev., 123, 383–416, 2006. [NASA ADS] [CrossRef] [Google Scholar]
  • Gloeckler, G., J. Cain, F.M. Ipavich, E.O. Tums, P. Bedini, et al. Investigation of the composition of solar and interstellar matter using solar wind and pickup ion measurements with SWICS and SWIMS on the ACE spacecraft. Space Sci. Rev., 86, 497–539, 1998. [NASA ADS] [CrossRef] [Google Scholar]
  • Gopalswamy, N., Y. Hanaoka, T. Kosugi, R.P. Lepping, J.T. Steinberg, et al. On the relationship between coronal mass ejections and magnetic clouds. Geophys. Res. Lett., 25, 2485–2488, 1998. [NASA ADS] [CrossRef] [Google Scholar]
  • Gopalswamy, N., A. Dal Lago, S. Yashiro, and S. Akiyama. The expansion and radial speeds of coronal mass ejections. Central European Astrophysical Bulletin, 33, 115–124, 2009. [Google Scholar]
  • Harrison, R.A., J.A. Davies, C. Möstl, Y. Liu, M. Temmer, et al. An analysis of the origin and propagation of the multiple coronal mass ejections of 2010 August 1. Astrophys. J., 750, 45, 2012. [Google Scholar]
  • Howard, R.A., J.D. Moses, A. Vourlidas, J.S. Newmark, D.G. Socker, et al. Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI). Space Sci. Rev., 136, 67–115, 2008. [NASA ADS] [CrossRef] [Google Scholar]
  • Howard, T.A. Three-dimensional reconstruction of coronal mass ejections using heliospheric imager data. J. Atmos. Sol. Terr. Phys., 73, 1242–1253, 2011. [NASA ADS] [CrossRef] [Google Scholar]
  • Howard, T.A., and C.E. DeForest. Inner heliospheric flux rope evolution via imaging of coronal mass ejections. Astrophys. J., 746, 64, 2012. [Google Scholar]
  • Howard, T.A., and S.J. Tappin. Interplanetary coronal mass ejections observed in the heliosphere: 1. review of theory. Space Sci. Rev., 147, 31–54, 2009. [Google Scholar]
  • Howard, T.A., D.F. Webb, S.J. Tappin, D.R. Mizuno, and J.C. Johnston. Tracking halo coronal mass ejections from 0–1 AU and space weather forecasting using the solar mass ejection imager (SMEI). J. Geophys. Res., 111, A04105, 2006. [Google Scholar]
  • Illing, R.M.E., and A.J. Hundhausen. Observation of a coronal transient from 1.2 to 6 solar radii. J. Geophys. Res., 90, 275–282, 1985. [Google Scholar]
  • Joshi, A.D., and N. Srivastava. Kinematics of two eruptive prominences observed by EUVI/STEREO. Astrophys. J., 730, 104, 2011. [NASA ADS] [CrossRef] [Google Scholar]
  • Kahler, S.W., and D.F. Webb. V arc interplanetary coronal mass ejections observed with the solar mass ejection imager. J. Geophys. Res., 112, A09103, 2007. [Google Scholar]
  • Klein, L.W., and L.F. Burlaga. Interplanetary magnetic clouds at 1 AU. J. Geophys. Res., 87, 613–624, 1982. [Google Scholar]
  • Lemen, J.R., A.M. Title, D.J. Akin, P.F. Boerner, C. Chou, et al. The atmospheric imaging assembly (AIA) on the solar dynamics observatory (SDO). Sol. Phys., 275, 17–40, 2012. [NASA ADS] [CrossRef] [Google Scholar]
  • Lepping, R.P., L.F. Burlaga, and J.A. Jones. Magnetic field structure of interplanetary magnetic clouds at 1 AU. J. Geophys. Res., 95, 11957–11965, 1990. [NASA ADS] [CrossRef] [Google Scholar]
  • Lepri, S.T., and T.H. Zurbuchen. Direct observational evidence of filament material within interplanetary coronal mass ejections. Astrophys. J. Lett., 723, L22–L27, 2010. [CrossRef] [Google Scholar]
  • Liu, Y., J.A. Davies, J.G. Luhmann, A. Vourlidas, S.D. Bale, and R.P. Lin. Geometric triangulation of imaging observations to track coronal mass ejections continuously out to 1 AU. Astrophys. J. Lett., 710, L82–L87, 2010a. [Google Scholar]
  • Liu, Y., A. Thernisien, J.G. Luhmann, A. Vourlidas, J.A. Davies, R.P. Lin, and S.D. Bale. Reconstructing coronal mass ejections with coordinated imaging and in situ observations: global structure, kinematics, and implications for space weather forecasting. Astrophys. J., 722, 1762–1777, 2010b. [Google Scholar]
  • Liu, Y., J.G. Luhmann, S.D. Bale, and R.P. Lin. Solar source and heliospheric consequences of the 2010 April 3 coronal mass ejection: a comprehensive view. Astrophys. J., 734, 84, 2011. [CrossRef] [Google Scholar]
  • Liu, Y.D., J.G. Luhmann, N. Lugaz, C. Möstl, J.A. Davies, S.D. Bale, and R.P. Lin. On sun-to-earth propagation of coronal mass ejections. Astrophys. J., 769, 45, 2013. [Google Scholar]
  • Lopez, R.E. Solar cycle invariance in solar wind proton temperature relationships. J. Geophys. Res., 92, 11189–11194, 1987. [CrossRef] [Google Scholar]
  • Lugaz, N. Accuracy and limitations of fitting and stereoscopic methods to determine the direction of coronal mass ejections from heliospheric imagers observations. Sol. Phys., 267, 411–429, 2010. [CrossRef] [Google Scholar]
  • Lugaz, N., A. Vourlidas, and I.I. Roussev. Deriving the radial distances of wide coronal mass ejections from elongation measurements in the heliosphere – application to CME-CME interaction. Ann. Geophys., 27, 3479–3488, 2009. [NASA ADS] [CrossRef] [Google Scholar]
  • Lugaz, N., J.N. Hernandez-Charpak, I.I. Roussev, C.J. Davis, A. Vourlidas, and J.A. Davies. Determining the azimuthal properties of coronal mass ejections from multi-spacecraft remote-sensing observations with STEREO SECCHI. Astrophys. J., 715, 493–499, 2010. [CrossRef] [Google Scholar]
  • Manoharan, P.K. Evolution of coronal mass ejections in the inner heliosphere: a study using white-light and scintillation images. Sol. Phys., 235, 345–368, 2006. [NASA ADS] [CrossRef] [Google Scholar]
  • Michalek, G., N. Gopalswamy, and S. Yashiro. Expansion speed of coronal mass ejections. Sol. Phys., 260, 401–406, 2009. [CrossRef] [Google Scholar]
  • Mierla, M., B. Inhester, C. Marqué, L. Rodriguez, S. Gissot, A.N. Zhukov, D. Berghmans, and J. Davila. On 3D reconstruction of coronal mass ejections: I. method description and application to SECCHI-COR data. Sol. Phys., 259, 123–141, 2009. [NASA ADS] [CrossRef] [Google Scholar]
  • Mishra, W., and N. Srivastava. Estimating the arrival time of earth-directed coronal mass ejections at in situ spacecraft using COR and HI observations from STEREO. Astrophys. J., 772, 70, 2013. [CrossRef] [Google Scholar]
  • Mishra, W., and N. Srivastava. Morphological and kinematic evolution of three interacting coronal mass ejections of 2011 February 13–15. Astrophys. J., 794, 64, 2014. [CrossRef] [Google Scholar]
  • Mishra, W., N. Srivastava, and J.A. Davies. A comparison of reconstruction methods for the estimation of coronal mass ejections kinematics based on SECCHI/HI observations. Astrophys. J., 784, 135, 2014. [NASA ADS] [CrossRef] [Google Scholar]
  • Mishra, W., N. Srivastava, and D. Chakrabarty. Evolution and consequences of interacting CMEs of 9–10 November 2012 using STEREO/SECCHI and in situ observations. Sol. Phys., 290, 527–552, 2015. [Google Scholar]
  • Möstl, C., and J.A. Davies. Speeds and arrival times of solar transients approximated by self-similar expanding circular fronts. Sol. Phys., 285, 411–423, 2013. [NASA ADS] [CrossRef] [Google Scholar]
  • Möstl, C., T. Rollett, N. Lugaz, C.J. Farrugia, J.A. Davies, et al. Arrival time calculation for interplanetary coronal mass ejections with circular fronts and application to STEREO observations of the 2009 February 13 eruption. Astrophys. J., 741, 34, 2011. [Google Scholar]
  • Ogilvie, K.W., D.J. Chornay, R.J. Fritzenreiter, F. Hunsaker, J. Keller, et al. SWE, a comprehensive plasma instrument for the Wind spacecraft. Space Sci. Rev., 71, 55–77, 1995. [NASA ADS] [CrossRef] [Google Scholar]
  • Poomvises, W., J. Zhang, and O. Olmedo. Coronal mass ejection propagation and expansion in three-dimensional space in the heliosphere based on Stereo/SECCHI observations. Astrophys. J. Lett., 717, L159–L163, 2010. [Google Scholar]
  • Riley, P., R. Lionello, Z. Mikić, and J. Linker. Using global simulations to relate the three-part structure of coronal mass ejections to in situ signatures. Astrophys. J., 672, 1221–1227, 2008. [Google Scholar]
  • Rouillard, A.P., J.A. Davies, R.J. Forsyth, A. Rees, C.J. Davis, et al. First imaging of corotating interaction regions using the STEREO spacecraft. Geophys. Res. Lett., 35, L1011, 2008. [Google Scholar]
  • Schwenn, R., A. dal Lago, E. Huttunen, and W.D. Gonzalez. The association of coronal mass ejections with their effects near the Earth. Ann. Geophys., 23, 1033–1059, 2005. [NASA ADS] [CrossRef] [Google Scholar]
  • Sharma, R., and N. Srivastava. Presence of solar filament plasma detected in interplanetary coronal mass ejections by in situ spacecraft. J. Space Weather Space Clim., 2 (26), A10, 2012. [CrossRef] [EDP Sciences] [Google Scholar]
  • Sharma, R., N. Srivastava, D. Chakrabarty, C. Möstl, and Q. Hu. Interplanetary and geomagnetic consequences of 5 January 2005 CMEs associated with eruptive filaments. J. Geophys. Res., 118, 3954–3967, 2013. [Google Scholar]
  • Sheeley, N.R., J.H. Walters, Y.-M. Wang, and R.A. Howard. Continuous tracking of coronal outflows: two kinds of coronal mass ejections. J. Geophys. Res., 104, 24739–24768, 1999. [Google Scholar]
  • Sheeley Jr., N.R., A.D. Herbst, C.A. Palatchi, Y.-M. Wang, R.A. Howard, et al. Heliospheric images of the solar wind at Earth. Astrophys. J., 675, 853–862, 2008. [Google Scholar]
  • Skoug, R.M., S.J. Bame, W.C. Feldman, J.T. Gosling, D.J. McComas, et al. A prolonged He+ enhancement within a coronal mass ejection in the solar wind. Geophys. Res. Lett., 26, 161–164, 1999. [NASA ADS] [CrossRef] [Google Scholar]
  • Stone, E.C., A.M. Frandsen, R.A. Mewaldt, E.R. Christian, D. Margolies, J.F. Ormes, and F. Snow. The advanced composition explorer. Space Sci. Rev., 86, 1–22, 1998. [Google Scholar]
  • Tappin, S.J., A. Buffington, M.P. Cooke, C.J. Eyles, P.P. Hick, et al. Tracking a major interplanetary disturbance with SMEI. Geophys. Res. Lett., 31, L02802, 2004. [CrossRef] [Google Scholar]
  • Thompson, W.T. 3D triangulation of a Sun-grazing comet. Icarus, 200, 351–357, 2009. [NASA ADS] [CrossRef] [Google Scholar]
  • Vršnak, B., T. Žic, T.V. Falkenberg, C. Möstl, S. Vennerstrom, and D. Vrbanec. The role of aerodynamic drag in propagation of interplanetary coronal mass ejections. A&A, 512, A43, 2010. [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
  • Vršnak, B., T. Žic, D. Vrbanec, M. Temmer, T. Rollett, et al. Propagation of interplanetary coronal mass ejections: the drag-based model. Sol. Phys., 285, 295–315, 2013. [Google Scholar]
  • Webb, D.F., and A.J. Hundhausen. Activity associated with the solar origin of coronal mass ejections. Sol. Phys., 108, 383–401, 1987. [NASA ADS] [CrossRef] [Google Scholar]
  • Zurbuchen, T.H., and I.G. Richardson. In-situ solar wind and magnetic field signatures of interplanetary coronal mass ejections. Space Sci. Rev., 123, 31–43, 2006. [NASA ADS] [CrossRef] [Google Scholar]

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