Fine structure of the solar atmosphere from near-limb observations in three wavelengths
| dc.contributor.author | Georgakilas, A. A. | en |
| dc.contributor.author | Dara, H. | en |
| dc.contributor.author | Zachariadis, T. | en |
| dc.contributor.author | Alissandrakis, C. E. | en |
| dc.contributor.author | Koutchmy, S. | en |
| dc.date.accessioned | 2015-11-24T18:28:27Z | |
| dc.date.available | 2015-11-24T18:28:27Z | |
| dc.identifier.issn | 0038-0938 | - |
| dc.identifier.uri | https://olympias.lib.uoi.gr/jspui/handle/123456789/16142 | |
| dc.rights | Default Licence | - |
| dc.subject | contrasts | en |
| dc.subject | faculae | en |
| dc.title | Fine structure of the solar atmosphere from near-limb observations in three wavelengths | en |
| heal.abstract | We analyze a time series of high-resolution observations near the limb, in the continuum, in the Mg b(1) line (-0.4 Angstrom off line center), and in the wings of H alpha (+0.75 Angstrom). The observations were obtained with a CCD camera at the Vacuum Tower telescope of the Sacramento Peak Observatory. We study the association of facular points, as they appear at different heights of the solar atmosphere (continuum, b(1) - 0.4 Angstrom, H alpha + 0.75 Angstrom) with the feet of fine dark mottles. | en |
| heal.access | campus | - |
| heal.fullTextAvailability | TRUE | - |
| heal.identifier.secondary | <Go to ISI>://A1997XL73000018 | - |
| heal.journalName | Solar Physics | en |
| heal.journalType | peer reviewed | - |
| heal.language | en | - |
| heal.publicationDate | 1997 | - |
| 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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