| | |
| | |
Stat |
Members: 3645 Articles: 2'500'096 Articles rated: 2609
19 April 2024 |
|
| | | |
|
Article overview
| |
|
The coronal convection | Werner Curdt
; Hui Tian
; Eckart Marsch
; | Date: |
12 Jan 2011 | Abstract: | We study the hydrogen Lyman emission in various solar features - now
including Lyman-alpha observations free from geocoronal absorption - and
investigate statistically the imprint of flows and of the magnetic field on the
line profile and radiance distribution. As a new result, we found that in
Lyman-alpha rasters locations with higher opacity cluster in the cell interior,
while the network has a trend to flatter profiles. Even deeper self reversals
and larger peak distances were found in coronal hole spectra. We also compare
simultaneous Lyman-alpha and Lyman-beta profiles. There is an obvious
correspondence between asymmetry and redshift for both lines, but, most
surprisingly, the asymmetries of Lyman-alpha and Lyman-beta are opposite. We
conclude that in both cases downflows determine the line profile, in case of
Lyman-alpha by absorption and in the case of Ly-beta by emission. Our results
show that the magnetically structured atmosphere plays a dominating role in the
line formation and indicate the presence of a persisting downflow at both
footpoints of closed loops. We claim that this is the manifestation of a
fundamental mass transportation process, which Foukal back in 1978 introduced
as the ’coronal convection’. | Source: | arXiv, 1101.2365 | Services: | Forum | Review | PDF | Favorites |
|
|
No review found.
Did you like this article?
Note: answers to reviews or questions about the article must be posted in the forum section.
Authors are not allowed to review their own article. They can use the forum section.
browser claudebot
|
| |
|
|
|
| News, job offers and information for researchers and scientists:
| |