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

• Veröffentlicht in: Advances in Astronomy and Space Physics
• Datum: 2012
• Hauptverfasser: Paraschiv, A.R., Dragomirescu, D., Stan, L., Talpeanu, D.C., Ivan, C., Radu, S., Lacatus, D.A., Mierla, M.
• Format: Artikel
• Sprache: English
• Veröffentlicht: Головна астрономічна обсерваторія НАН України 2012
• Online Zugang: https://nasplib.isofts.kiev.ua/handle/123456789/119191
• Назва журналу: Digital Library of Periodicals of National Academy of Sciences of Ukraine
• Zitieren: 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.

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...