Comparison of the extent and mass of CME events in the interplanetary medium using IPS and SMEI Thomson scattering observations
作者： B. V. Jackson , P. P. Hick , A. Buffington , M. M. Bisi , M. Kojima
DOI: 10.1080/10556790701612221
关键词:
摘要: The Solar-Terrestrial Environment Laboratory (STELab), Japan, interplanetary scintillation (IPS) g-level and velocity measurements can be used to give the extent of CME disturbances in medium arising from scattering radio waves distant point-like natural sources through intervening medium. In addition, white-light Thomson-scattering observations Solar Mass Ejection Imager (SMEI) have recorded inner heliospheric response several hundred CMEs. work described here compares details difference three-dimensional (3D) reconstructions for these two data sets well-observed 28 October 2003 halo seen LASCO; this passed Earth on 29 SMEI at same elongations as IPS observations. analysis employs a 3D tomographic reconstruction technique that obtains perspective views outward-flowing solar wind observed Earth, iteratively fitting kinematic density model, when av...
harvard.edu
sci-hub.se 参考文章(24)
Michael K. Bird, Peter Edenhofer, Remote Sensing Observations of the Solar Corona Physics of the Inner Heliosphere I. pp. 13- 97 ,(1990) , 10.1007/978-3-642-75361-9_2
Bernard V. Jackson, P. Paul Hick, Three-Dimensional Tomography of Interplanetary Disturbances Astrophysics and space science library. ,vol. 314, pp. 355- 386 ,(2004) , 10.1007/1-4020-2814-8_17
E.A. Jensen, M.K. Bird, S.W. Asmar, L. Iess, J.D. Anderson, C.T. Russell, The Cassini solar Faraday rotation experiment Advances in Space Research. ,vol. 36, pp. 1587- 1594 ,(2005) , 10.1016/J.ASR.2005.09.039
Ruth M Skoug, JT Gosling, John T Steinberg, DJ McComas, CW Smith, NF Ness, Q Hu, LF Burlaga, Extremely high speed solar wind: 29–30 October 2003 Journal of Geophysical Research. ,vol. 109, ,(2004) , 10.1029/2004JA010494
Munetoshi Tokumaru, Masayoshi Kojima, Ken'ichi Fujiki, Masahiro Yamashita, Atsushi Yokobe, Toroidal-shaped interplanetary disturbance associated with the halo coronal mass ejection event on 14 July 2000 Journal of Geophysical Research. ,vol. 108, pp. 1220- ,(2003) , 10.1029/2002JA009574
E. W. Cliver, L. Svalgaard, The 1859 Solar–Terrestrial Disturbance And the Current Limits of Extreme Space Weather Activity Solar Physics. ,vol. 224, pp. 407- 422 ,(2004) , 10.1007/S11207-005-4980-Z
Munetoshi Tokumaru, Masayoshi Kojima, Ken’ichi Fujiki, Masahiro Yamashita, Bernard V. Jackson, The source and propagation of the interplanetary disturbance associated with the full-halo coronal mass ejection on 28 October 2003 Journal of Geophysical Research. ,vol. 112, ,(2007) , 10.1029/2006JA012043
Bernard V. Jackson, Andrew Buffington, P. P. Hick, Cindy X. Wang, Low resolution three dimensional reconstruction of CMEs using solar mass ejection imager (SMEI) data Proceedings of SPIE. ,vol. 5901, pp. 590101- ,(2005) , 10.1117/12.616329
Z. HOUMINER, Corotating Plasma Streams revealed by Interplanetary Scintillation Nature. ,vol. 231, pp. 165- 167 ,(1971) , 10.1038/PHYSCI231165A0
G. E. Brueckner, R. A. Howard, M. J. Koomen, C. M. Korendyke, D. J. Michels, J. D. Moses, D. G. Socker, K. P. Dere, P. L. Lamy, A. Llebaria, M. V. Bout, R. Schwenn, G. M. Simnett, D. K. Bedford, C. J. Eyles, The Large Angle Spectroscopic Coronagraph (LASCO): Visible light coronal imaging and spectroscopy Solar Physics. ,vol. 162, pp. 17- 34 ,(1995) , 10.1007/BF00733434