Coronal jet contribution to the slow Solar wind flux: preliminary results

The solar wind is a continuous flux of charged particles that are ejected from the Sun's atmosphere. The sources of this flux have not been clearly identiffed yet. Coronal jets are proposed as a possible candidate. They are small collimated ejections of plasma seen in white-light coronagraph im...

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Published in:Advances in Astronomy and Space Physics
Date:2012
Main Authors: Paraschiv, A.R., Dragomirescu, D., Stan, L., Talpeanu, D.C., Ivan, C., Radu, S., Lacatus, D.A., Mierla, M.
Format: Article
Language:English
Published: Головна астрономічна обсерваторія НАН України 2012
Online Access:https://nasplib.isofts.kiev.ua/handle/123456789/119191
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Journal Title:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Cite this:Coronal jet contribution to the slow Solar wind flux: preliminary results / A.R. Paraschiv, D. Dragomirescu, L. Stan, D.C. Talpeanu, C. Ivan, S. Radu, D.A. Lacatus, M. Mierla // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 2. — С. 161-163. — Бібліогр.: 20 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
id nasplib_isofts_kiev_ua-123456789-119191
record_format dspace
spelling Paraschiv, A.R.
Dragomirescu, D.
Stan, L.
Talpeanu, D.C.
Ivan, C.
Radu, S.
Lacatus, D.A.
Mierla, M.
2017-06-04T19:40:12Z
2017-06-04T19:40:12Z
2012
Coronal jet contribution to the slow Solar wind flux: preliminary results / A.R. Paraschiv, D. Dragomirescu, L. Stan, D.C. Talpeanu, C. Ivan, S. Radu, D.A. Lacatus, M. Mierla // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 2. — С. 161-163. — Бібліогр.: 20 назв. — англ.
2227-1481
https://nasplib.isofts.kiev.ua/handle/123456789/119191
The solar wind is a continuous flux of charged particles that are ejected from the Sun's atmosphere. The sources of this flux have not been clearly identiffed yet. Coronal jets are proposed as a possible candidate. They are small collimated ejections of plasma seen in white-light coronagraph images. Using an existing catalogue, a sample of events during the period 2007-2008 was analysed, and ejected particle flux has been estimated. First results are now presented. As future work, all the jets contained in the catalogue will be analysed in order to obtain the average particle flux. The results will be compared to in-situ measurements in order to assess the coronal jet contribution to the solar wind.
The authors are grateful to Prof. Dr. E. Barna, Prof. Dr. S. Antohe, Prof. Dr. Al. Jipa and the University of Bucharest for providing financial support. A. R. Paraschiv would like to thank Prof. Dr. I. Lazanu for guidance and productive discussions. A. R. Paraschiv and D. A. Lacatus thank the University of Bucharest for funding this research. The authors acknowledge the STEREO/SECCHI consortium for providing the data.
en
Головна астрономічна обсерваторія НАН України
Advances in Astronomy and Space Physics
Coronal jet contribution to the slow Solar wind flux: preliminary results
Article
published earlier
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
title Coronal jet contribution to the slow Solar wind flux: preliminary results
spellingShingle Coronal jet contribution to the slow Solar wind flux: preliminary results
Paraschiv, A.R.
Dragomirescu, D.
Stan, L.
Talpeanu, D.C.
Ivan, C.
Radu, S.
Lacatus, D.A.
Mierla, M.
title_short Coronal jet contribution to the slow Solar wind flux: preliminary results
title_full Coronal jet contribution to the slow Solar wind flux: preliminary results
title_fullStr Coronal jet contribution to the slow Solar wind flux: preliminary results
title_full_unstemmed Coronal jet contribution to the slow Solar wind flux: preliminary results
title_sort coronal jet contribution to the slow solar wind flux: preliminary results
author Paraschiv, A.R.
Dragomirescu, D.
Stan, L.
Talpeanu, D.C.
Ivan, C.
Radu, S.
Lacatus, D.A.
Mierla, M.
author_facet Paraschiv, A.R.
Dragomirescu, D.
Stan, L.
Talpeanu, D.C.
Ivan, C.
Radu, S.
Lacatus, D.A.
Mierla, M.
publishDate 2012
language English
container_title Advances in Astronomy and Space Physics
publisher Головна астрономічна обсерваторія НАН України
format Article
description The solar wind is a continuous flux of charged particles that are ejected from the Sun's atmosphere. The sources of this flux have not been clearly identiffed yet. Coronal jets are proposed as a possible candidate. They are small collimated ejections of plasma seen in white-light coronagraph images. Using an existing catalogue, a sample of events during the period 2007-2008 was analysed, and ejected particle flux has been estimated. First results are now presented. As future work, all the jets contained in the catalogue will be analysed in order to obtain the average particle flux. The results will be compared to in-situ measurements in order to assess the coronal jet contribution to the solar wind.
issn 2227-1481
url https://nasplib.isofts.kiev.ua/handle/123456789/119191
citation_txt Coronal jet contribution to the slow Solar wind flux: preliminary results / A.R. Paraschiv, D. Dragomirescu, L. Stan, D.C. Talpeanu, C. Ivan, S. Radu, D.A. Lacatus, M. Mierla // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 2. — С. 161-163. — Бібліогр.: 20 назв. — англ.
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first_indexed 2025-12-07T19:54:28Z
last_indexed 2025-12-07T19:54:28Z
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