Fine structure of the solar chromosphere: Arch-shaped mottles
| dc.contributor.author | Zachariadis, T. G. | en |
| dc.contributor.author | Georgakilas, A. A. | en |
| dc.contributor.author | Koutchmy, S. | en |
| dc.contributor.author | Alissandrakis, C. E. | en |
| dc.date.accessioned | 2015-11-24T18:28:26Z | |
| dc.date.available | 2015-11-24T18:28:26Z | |
| dc.identifier.issn | 0038-0938 | - |
| dc.identifier.uri | https://olympias.lib.uoi.gr/jspui/handle/123456789/16141 | |
| dc.rights | Default Licence | - |
| dc.subject | evolution | en |
| dc.title | Fine structure of the solar chromosphere: Arch-shaped mottles | en |
| heal.abstract | We analyze a time series of high resolution observations near the solar limb, obtained in H alpha and the Mg bl line. We identified arch-shaped dark mottles, which are thin, faint H alpha structures observable under very good seeing conditions, best seen in H alpha + 0.75 Angstrom. Their mean length is about 15", their mean height about 6'' and indicative lifetimes is of the order of 5 min. They show negative (away from the observer) line-of-sight velocities. A possible interpretation is that material flows from the apex towards the feet of the arches. | en |
| heal.access | campus | - |
| heal.fullTextAvailability | TRUE | - |
| heal.identifier.secondary | <Go to ISI>://000078944000004 | - |
| heal.identifier.secondary | http://www.springerlink.com/content/t552333u52992861/fulltext.pdf | - |
| heal.journalName | Solar Physics | en |
| heal.journalType | peer reviewed | - |
| heal.language | en | - |
| heal.publicationDate | 1999 | - |
| heal.recordProvider | Πανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιών | el |
| heal.type | journalArticle | - |
| heal.type.el | Άρθρο Περιοδικού | el |
| heal.type.en | Journal article | en |
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