| | |
| | |
Stat |
Members: 3645 Articles: 2'504'928 Articles rated: 2609
26 April 2024 |
|
| | | |
|
Article overview
| |
|
Molecular absorption in transition region spectral lines | Donald Schmit
; Davina Innes
; Thomas Ayres
; Hardi Peter
; Werner Curdt
; Sarah Jaeggli
; | Date: |
5 Sep 2014 | Abstract: | Aims: We present observations from the Interface Region Imaging Spectrograph
(IRIS) of absorption features from a multitude of cool atomic and molecular
lines within the profiles of Si IV transition region lines. Many of these
spectral lines have not previously been detected in solar spectra. Methods: We
examined spectra taken from deep exposures of plage on 12 October 2013. We
observed unique absorption spectra over a magnetic element which is bright in
transition region line emission and the ultraviolet continuum. We compared the
absorption spectra with emission spectra that is likely related to
fluorescence. Results: The absorption features require a population of sub-5000
K plasma to exist above the transition region. This peculiar stratification is
an extreme deviation from the canonical structure of the chromosphere-corona
boundary . The cool material is not associated with a filament or discernible
coronal rain. This suggests that molecules may form in the upper solar
atmosphere on small spatial scales and introduces a new complexity into our
understanding of solar thermal structure. It lends credence to previous
numerical studies that found evidence for elevated pockets of cool gas in the
chromosphere. | Source: | arXiv, 1409.1702 | 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 Mozilla/5.0 AppleWebKit/537.36 (KHTML, like Gecko; compatible; ClaudeBot/1.0; +claudebot@anthropic.com)
|
| |
|
|
|
| News, job offers and information for researchers and scientists:
| |