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https://olympias.lib.uoi.gr/jspui/handle/123456789/16470Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Vourlidas, A. | en |
| dc.contributor.author | Howard, R. A. | en |
| dc.contributor.author | Esfandiari, E. | en |
| dc.contributor.author | Patsourakos, S. | en |
| dc.contributor.author | Yashiro, S. | en |
| dc.contributor.author | Michalek, G. | en |
| dc.date.accessioned | 2015-11-24T18:31:27Z | - |
| dc.date.available | 2015-11-24T18:31:27Z | - |
| dc.identifier.issn | 0004-637X | - |
| dc.identifier.uri | https://olympias.lib.uoi.gr/jspui/handle/123456789/16470 | - |
| dc.rights | Default Licence | - |
| dc.subject | methods: statistical | en |
| dc.subject | sun: activity | en |
| dc.subject | sun: corona | en |
| dc.subject | sun: coronal mass ejections (cmes) | en |
| dc.subject | spaced data | en |
| dc.subject | lasco | en |
| dc.subject | brightness | en |
| dc.subject | energetics | en |
| dc.subject | interplanetary | en |
| dc.subject | distributions | en |
| dc.subject | calibration | en |
| dc.subject | parameters | en |
| dc.subject | density | en |
| dc.subject | speeds | en |
| dc.title | Comprehensive Analysis of Coronal Mass Ejection Mass and Energy Properties over a Full Solar Cycle | en |
| heal.type | journalArticle | - |
| heal.type.en | Journal article | en |
| heal.type.el | Άρθρο Περιοδικού | el |
| heal.identifier.primary | Doi 10.1088/0004-637x/722/2/1522 | - |
| heal.identifier.secondary | <Go to ISI>://000284075400042 | - |
| heal.identifier.secondary | http://iopscience.iop.org/0004-637X/722/2/1522/pdf/0004-637X_722_2_1522.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 | The LASCO coronagraphs, in continuous operation since 1995, have observed the evolution of the solar corona and coronal mass ejections (CMEs) over a full solar cycle with high-quality images and regular cadence. This is the first time that such a data set becomes available and constitutes a unique resource for the study of CMEs. In this paper, we present a comprehensive investigation of the solar cycle dependence on the CME mass and energy over a full solar cycle (1996-2009) including the first in-depth discussion of the mass and energy analysis methods and their associated errors. Our analysis provides several results worthy of further studies. It demonstrates the possible existence of two event classes: "normal" CMEs reaching constant mass for > 10 R(circle dot) and "pseudo"-CMEs which disappear in the C3 field of view. It shows that the mass and energy properties of CME reach constant levels and therefore should be measured only above similar to 10R(circle dot). The mass density (g/R(circle dot)(2)) of CMEs varies relatively little (< order of magnitude) suggesting that the majority of the mass originates from a small range in coronal heights. We find a sudden reduction in the CME mass in mid-2003 which may be related to a change in the electron content of the large-scale corona and we uncover the presence of a 6 month periodicity in the ejected mass from 2003 onward. | en |
| heal.journalName | Astrophysical Journal | en |
| heal.journalType | peer reviewed | - |
| heal.fullTextAvailability | TRUE | - |
| Appears in Collections: | Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά) | |
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