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| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | PrekaPapadema, P. | en |
| dc.contributor.author | Alissandrakis, C. E. | en |
| dc.contributor.author | Dennis, B. R. | en |
| dc.contributor.author | Kundu, M. R. | en |
| dc.date.accessioned | 2015-11-24T18:40:29Z | - |
| dc.date.available | 2015-11-24T18:40:29Z | - |
| dc.identifier.issn | 0038-0938 | - |
| dc.identifier.uri | https://olympias.lib.uoi.gr/jspui/handle/123456789/17629 | - |
| dc.rights | Default Licence | - |
| dc.title | Modeling of a microwave burst emission | en |
| heal.type | journalArticle | - |
| heal.type.en | Journal article | en |
| heal.type.el | Άρθρο Περιοδικού | el |
| heal.identifier.secondary | <Go to ISI>://A1997XL73000029 | - |
| heal.language | en | - |
| heal.access | campus | - |
| heal.recordProvider | Πανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιών | el |
| heal.publicationDate | 1997 | - |
| heal.abstract | We applied model computations on a microwave burst observed with the Westerbork Synthesis Radio Telescope (WSRT) at 6 cm. We used additional data from H alpha, soft and hard X-rays in order to reproduce the flaring loop and to compute the microwave total intensity and circular polarization. We examined both cases of thin and thick target. The computations show a large emission source in an optically thick loop. We compare our results with the observation. | en |
| heal.journalName | Solar Physics | en |
| heal.journalType | peer reviewed | - |
| heal.fullTextAvailability | TRUE | - |
| Appears in Collections: | Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά) | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| allissandrakis-1997-Modeling of a microwave burst emission.pdf | 571.44 kB | Adobe PDF | View/Open Request a copy |
This item is licensed under a Creative Commons License
