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https://olympias.lib.uoi.gr/jspui/handle/123456789/17490Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Nistico, G. | en |
| dc.contributor.author | Bothmer, V. | en |
| dc.contributor.author | Patsourakos, S. | en |
| dc.contributor.author | Zimbardo, G. | en |
| dc.date.accessioned | 2015-11-24T18:39:42Z | - |
| dc.date.available | 2015-11-24T18:39:42Z | - |
| dc.identifier.issn | 0992-7689 | - |
| dc.identifier.uri | https://olympias.lib.uoi.gr/jspui/handle/123456789/17490 | - |
| dc.rights | Default Licence | - |
| dc.subject | solar physics, astrophysics, and astronomy | en |
| dc.subject | corona and transition region | en |
| dc.subject | ultraviolet emissions | en |
| dc.subject | space plasma physics | en |
| dc.subject | magnetic reconnection | en |
| dc.subject | x-ray jets | en |
| dc.subject | magnetic reconnection | en |
| dc.subject | polar jets | en |
| dc.subject | h-alpha | en |
| dc.subject | parameters | en |
| dc.subject | telescope | en |
| dc.subject | secchi | en |
| dc.subject | model | en |
| dc.title | Observational features of equatorial coronal hole jets | en |
| heal.type | journalArticle | - |
| heal.type.en | Journal article | en |
| heal.type.el | Άρθρο Περιοδικού | el |
| heal.identifier.secondary | <Go to ISI>://000276173600001 | - |
| heal.identifier.secondary | http://www.ann-geophys.net/28/687/2010/angeo-28-687-2010.pdf | - |
| heal.language | en | - |
| heal.access | campus | - |
| heal.recordProvider | Πανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιών | el |
| heal.publicationDate | 2010 | - |
| heal.abstract | Collimated ejections of plasma called "coronal hole jets" are commonly observed in polar coronal holes. However, such coronal jets are not only a specific features of polar coronal holes but they can also be found in coronal holes appearing at lower heliographic latitudes. In this paper we present some observations of "equatorial coronal hole jets" made up with data provided by the STEREO/SECCHI instruments during a period comprising March 2007 and December 2007. The jet events are selected by requiring at least some visibility in both COR1 and EUVI instruments. We report 15 jet events, and we discuss their main features. For one event, the uplift velocity has been determined as about 200 km s(-1), while the deceleration rate appears to be about 0.11 km s(-2), less than solar gravity. The average jet visibility time is about 30 min, consistent with jet observed in polar regions. On the basis of the present dataset, we provisionally conclude that there are not substantial physical differences between polar and equatorial coronal hole jets. | en |
| heal.journalName | Annales Geophysicae | en |
| heal.journalType | peer reviewed | - |
| heal.fullTextAvailability | TRUE | - |
| Appears in Collections: | Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά) | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| Nistico-2010-Observational featur.pdf | 5.65 MB | Adobe PDF | View/Open |
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