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https://olympias.lib.uoi.gr/jspui/handle/123456789/16785Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Klimchuk, S. Patsourakos | en |
| dc.contributor.author | S. K. Antiochos | en |
| dc.contributor.author | J. A. | en |
| dc.date.accessioned | 2015-11-24T18:33:42Z | - |
| dc.date.available | 2015-11-24T18:33:42Z | - |
| dc.identifier.issn | 0004-637X | - |
| dc.identifier.uri | https://olympias.lib.uoi.gr/jspui/handle/123456789/16785 | - |
| dc.rights | Default Licence | - |
| dc.title | A Model for Bright Extreme-Ultraviolet Knots in Solar Flare Loops | en |
| heal.type | journalArticle | - |
| heal.type.en | Journal article | en |
| heal.type.el | Άρθρο Περιοδικού | el |
| heal.identifier.secondary | http://stacks.iop.org/0004-637X/614/i=2/a=1022 | - |
| heal.access | campus | - |
| heal.recordProvider | Πανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιών | el |
| heal.publicationDate | 2004 | - |
| heal.abstract | EUV observations often indicate the presence of bright knots in flare loops. The temperature of the knot plasma is of the order of 1 MK, and the knots themselves are usually localized somewhere near the loop tops. We propose a model in which the formation of EUV knots is due to the spatial structure of the nonflare active region heating. We present the results of a series of one-dimensional hydrodynamic, flare-loop simulations, which include both an impulsive flare heating and a background, active region heating. The simulations demonstrate that the formation of the observed knots depends critically on the spatial distribution of the background heating during the decay phase. In particular, the heating must be localized far from the loop apex and have a magnitude comparable to the local radiative losses of the cooling loop. Our results, therefore, provide strong constraints on both coronal heating and postflare conditions. | en |
| heal.journalName | The Astrophysical Journal | en |
| heal.journalType | peer reviewed | - |
| heal.fullTextAvailability | TRUE | - |
| Appears in Collections: | Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά) | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| patsourakos-2004-A Model for Bright Extreme-Ultraviolet Knots in Solar Flare Loops.pdf | 244.92 kB | Adobe PDF | View/Open |
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