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| Content Provider | Springer Nature Link |
|---|---|
| Author | Pohjolainen, S. Driel Gesztelyi, L. Culhane, J. L. Maharan, P. K. Elliott, H. A. |
| Copyright Year | 2007 |
| Abstract | We explore the relationship among three coronal mass ejections (CMEs), observed on 28 October 2003, 7 November 2004, and 20 January 2005, the type II burst-associated shock waves in the corona and solar wind, as well as the arrival of their related shock waves and magnetic clouds at 1 AU. Using six different coronal/interplanetary density models, we calculate the speeds of shocks from the frequency drifts observed in metric and decametric radio wave data. We compare these speeds with the velocity of the CMEs as observed in the plane-of-the-sky white-light observations and calculated with a cone model for the 7 November 2004 event. We then follow the propagation of the ejecta using Interplanetary Scintillation measurements, which were available for the 7 November 2004 and 20 January 2005 events. Finally, we calculate the travel time of the interplanetary shocks between the Sun and Earth and discuss the velocities obtained from the different data. This study highlights the difficulties in making velocity estimates that cover the full CME propagation time. |
| Starting Page | 167 |
| Ending Page | 188 |
| Page Count | 22 |
| File Format | |
| ISSN | 00380938 |
| Journal | Solar Physics |
| Volume Number | 244 |
| Issue Number | 1-2 |
| e-ISSN | 1573093X |
| Language | English |
| Publisher | Springer Netherlands |
| Publisher Date | 2007-09-27 |
| Publisher Place | Dordrecht |
| Access Restriction | One Nation One Subscription (ONOS) |
| Subject Keyword | Coronal mass ejections Initiation and propagation Interplanetary Plasma physics Radio bursts Dynamic spectrum Meter-wavelengths and longer Type II Radio scintillation Astrophysics Extraterrestrial Physics, Space Sciences Astronomy |
| Content Type | Text |
| Resource Type | Article |
| Subject | Astronomy and Astrophysics Space and Planetary Science |
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