| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1768008 | Advances in Space Research | 2005 | 5 Pages |
Abstract
The LASCO-C1 telescope was designed to perform spectral analysis of coronal structures by means of a tunable Fabry–Pérot interferometer acquiring images at different wavelengths. Results from spectral scans of the Fe xiv 5303 Å green coronal emission line are presented. Physical quantities like the ion temperature (line widths), and the flow velocity along the line of sight (Doppler shifts) are obtained over the entire corona.
Keywords
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
M. Mierla, R. Schwenn, L. Teriaca, G. Stenborg, B. Podlipnik,