Prominence fine structure II: Diagnostics |
| |
| Authors: | J B Zirker S Koutchmy |
| |
| Institution: | (1) National Solar Observatory/Sacramento Peak, National Optical Astronomy Observatories, 88349 Sunspot, NM, U.S.A.;(2) Institut d'Astrophysique, CNRS, Paris, France |
| |
| Abstract: | A random-clustering model of prominence fine-structure has been applied to observations of prominence H spectra. The model yields an estimate of the number of unresolved elements that form an individual resolved feature, and sets limits on their velocity and H profile dispersions. |
| |
| Keywords: | |
| 本文献已被 SpringerLink 等数据库收录！ |
|
