| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 5374414 | Chemical Physics | 2012 | 4 Pages |
Abstract
⺠Classical solar atmospheric models are too warm for observations at mm wavelengths. ⺠Dynamic models are in agreement with the spatially averaged mm observational data. ⺠Mm interferometric observations confirm the complex structure of the chromosphere. ⺠Mm interferometric observations confirm the presence of chromospheric dynamics.
Keywords
Related Topics
Physical Sciences and Engineering
Chemistry
Physical and Theoretical Chemistry
Authors
V.G. Nagnibeda, M.A. Loukitcheva,