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https://olympias.lib.uoi.gr/jspui/handle/123456789/16757Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Grechnev, V. V. | en |
| dc.contributor.author | Kundu, M. R. | en |
| dc.contributor.author | Nindos, A. | en |
| dc.date.accessioned | 2015-11-24T18:33:35Z | - |
| dc.date.available | 2015-11-24T18:33:35Z | - |
| dc.identifier.issn | 0004-6264 | - |
| dc.identifier.uri | https://olympias.lib.uoi.gr/jspui/handle/123456789/16757 | - |
| dc.rights | Default Licence | - |
| dc.subject | sun : flares | en |
| dc.subject | sun : particle emission | en |
| dc.subject | sun : radio radiation | en |
| dc.subject | sun : x-rays, gamma rays | en |
| dc.subject | double-loop configuration | en |
| dc.subject | of-flight distances | en |
| dc.subject | magnetic reconnection | en |
| dc.subject | gyrosynchrotron emission | en |
| dc.subject | energetic electrons | en |
| dc.subject | bursts | en |
| dc.subject | prominence | en |
| dc.subject | distributions | en |
| dc.subject | wavelengths | en |
| dc.subject | dynamics | en |
| dc.title | A study of accelerated electrons in solar flares using microwave and X-ray observations | en |
| heal.type | journalArticle | - |
| heal.type.en | Journal article | en |
| heal.type.el | Άρθρο Περιοδικού | el |
| heal.identifier.secondary | <Go to ISI>://000235849400007 | - |
| heal.identifier.secondary | http://pasj.asj.or.jp/v58/n1/580107/580107-frame.html | - |
| heal.language | en | - |
| heal.access | campus | - |
| heal.recordProvider | Πανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιών | el |
| heal.publicationDate | 2006 | - |
| heal.abstract | We consider manifestations of accelerated electrons in microwave and hard X-ray emissions from solar flares. To meet our objectives, we discuss two events - those of 1999 March 16 and February 16. The first event is a short-duration burst, while the second is a long-duration event. An analysis of the first event leads to the conclusion that: 1) a seemingly single-loop configuration call actually be a double-loop one, and 2) it is possible that the pitch-angle distribution of the radio-emitting electrons can be anisotropic with practically no non-zero pitch angles. The second event shows seemingly intersecting flaring loops, and the formation of a post-eruptive arcade that call proceed as a series of double-loop interactions. From these and other published results, We Conclude that: 1) double-loop configurations can be responsible for flares showing diverse morphologies and time profiles; 2) the pitch-angle distribution of accelerated electrons can be Strongly anisotropic, with ail excess of small angles, contributing to a rather narrow energy range of the microwave-emitting electrons. | en |
| heal.journalName | Publications of the Astronomical Society of Japan | en |
| heal.journalType | peer reviewed | - |
| heal.fullTextAvailability | TRUE | - |
| Appears in Collections: | Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά) | |
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