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 |
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| Date: | 2012 |
| Main Authors: | , , , , , , , |
| Format: | Article |
| Language: | English |
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Головна астрономічна обсерваторія НАН України
2012
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| 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 |
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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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