On the Relationship Between a CME Associated Waves Observed on 5 March 2000
| dc.creator | Raouafi, N. -E. | |
| dc.creator | Tripathi, D. | |
| dc.date | 2008-01-05 | |
| dc.date.accessioned | 2026-07-07T08:52:46Z | |
| dc.date.available | 2026-07-07T08:52:46Z | |
| dc.description | We study the relationship between different wave phenomena associated with a coronal mass ejection (CME) observed on 05 Mar. 2000. EIT waves were observed in the images recorded by EIT at 195 Å. The white-light LASCO/C2 images show clear deflection and propagation of a kink along with the CME. Spectroscopic observations recorded by the UVCS reveals excessive line broadening in the two O {\sc{vi}} lines (1032 and 1037 Å). Moreover very hot lines such as Si {\sc{xii}} and Mg {\sc{x}} were observed. Interestingly, the EIT wave, the streamer deflection and the intensity modulation along the slit were all propagating North-East. Spatial and temporal correlations show that the streamer deflection and spectral line broadening are highly likely to be due to a CME-driven shock wave and that the EIT wave is the signature of a CME-driven shock wave in the lower corona. | |
| dc.description | 8 pages, 4 figures | |
| dc.identifier | https://arxiv.org/abs/0801.0766 | |
| dc.identifier | http://arxiv.org/abs/0801.0766 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/145392 | |
| dc.subject | Astrophysics | |
| dc.title | On the Relationship Between a CME Associated Waves Observed on 5 March 2000 | |
| dc.type | text |