Determining the parameters of coronal mass ejections using the method of MHD modeling ejection evolutions |
| |
| Authors: | N A Barkhatov E G Zhulina E A Kalinina |
| |
| Institution: | (1) Institute for Scientific Research, Boston College, Chestnut Hill, MA, USA;(2) Air Force Research Laboratory, Space Vehicles Directorate, Hanscom AFB, MA, USA;(3) Air Force Research Laboratory, National Solar Observatory, Sunspot, NM, USA;(4) Exploration Physics International, Inc., Huntsville, AL, USA;(5) Cooperative Institute for Research in Environmental Sciences, University of Colorado, Boulder, CO, USA;(6) Space Weather Prediction Center, National Oceanic and Atmospheric Administration, Boulder, CO, USA;(7) Center for Astrophysics and Space Science, University of California-San Diego, La Jolla, CA, USA;(8) Space Physics Division, Space Science and Technology Dept., Rutherford Appleton Laboratory, Chilton, Didcot, Oxfordshire, UK;(9) Space Science Division, Code 7663, Naval Research Laboratory, Washington, DC, USA |
| |
| Abstract: | The initial parameters of disturbing fluxes of coronal mass ejections (CMEs) such as loop, front, spike, multiple structure
ejection, and structureless ejection, which cannot be determined from direct observations, are determined using the data on
the interplanetary coronal mass ejections (ICMEs) registered on the Helios and Pioneer Venus Orbiter spacecraft in the vicinity
of Venus. The method of MHD modeling the modified initial parameters of CMEs has been used for this purpose. The ICME parameters
have been analyzed in order to determine the types of the solar sources of the considered plasma flows. |
| |
| Keywords: | |
| 本文献已被 SpringerLink 等数据库收录！ |
|
