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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Опубліковано в: :Advances in Astronomy and Space Physics
Дата:2012
Автори: Paraschiv, A.R., Dragomirescu, D., Stan, L., Talpeanu, D.C., Ivan, C., Radu, S., Lacatus, D.A., Mierla, M.
Формат: Стаття
Мова:Англійська
Опубліковано: Головна астрономічна обсерваторія НАН України 2012
Онлайн доступ:https://nasplib.isofts.kiev.ua/handle/123456789/119191
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Цитувати: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.

Репозитарії

Digital Library of Periodicals of National Academy of Sciences of Ukraine
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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.
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.
collection DSpace DC
container_title Advances in Astronomy and Space Physics
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.
first_indexed 2025-12-07T19:54:28Z
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language English
last_indexed 2025-12-07T19:54:28Z
publishDate 2012
publisher Головна астрономічна обсерваторія НАН України
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
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 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_short Coronal jet contribution to the slow Solar wind flux: preliminary results
title_sort coronal jet contribution to the slow solar wind flux: preliminary results
url https://nasplib.isofts.kiev.ua/handle/123456789/119191
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AT talpeanudc coronaljetcontributiontotheslowsolarwindfluxpreliminaryresults
AT ivanc coronaljetcontributiontotheslowsolarwindfluxpreliminaryresults
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