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DC Field | Value | Language |
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dc.contributor.author | Lantos, P. | en |
dc.contributor.author | Alissandrakis, C. E. | en |
dc.date.accessioned | 2015-11-24T18:28:53Z | - |
dc.date.available | 2015-11-24T18:28:53Z | - |
dc.identifier.issn | 0273-1177 | - |
dc.identifier.uri | https://olympias.lib.uoi.gr/jspui/handle/123456789/16200 | - |
dc.rights | Default Licence | - |
dc.title | Evolution of the coronal plasma sheet from cycle maximum to cycle minimum observed at meter wavelengths | en |
heal.type | journalArticle | - |
heal.type.en | Journal article | en |
heal.type.el | Άρθρο Περιοδικού | el |
heal.identifier.primary | http://dx.doi.org/10.1016/0273-1177(95)00332-9 | - |
heal.identifier.secondary | http://www.sciencedirect.com/science/article/pii/0273117795003329 | - |
heal.access | campus | - |
heal.recordProvider | Πανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιών | el |
heal.publicationDate | 1995 | - |
heal.abstract | The Nan?ay Radioheliograph provides maps of the quiet solar corona around 160 MHz. In addition to coronal holes, localized emission sources and quiet sun, an unresolved component can be detected on the disk. The so-called coronal plateau corresponds to the K-corona dense regions observed on the limb and is thus located at the base of the interplanetary plasma sheet. Its evolution is studied from 1980 to 1986, during the declining phase of the cycle 21. | en |
heal.journalName | Advances in Space Research | en |
heal.journalType | peer reviewed | - |
heal.fullTextAvailability | TRUE | - |
Appears in Collections: | Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά) |
Files in This Item:
File | Description | Size | Format | |
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alissandrakis-1995-Evolution of the coronal plasma sheet from cycle maximum to cycle minimum observed at meter wavelengths.pdf | 294.54 kB | Adobe PDF | View/Open Request a copy |
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