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UNIVERSITY OF BUCHAREST
FACULTY OF PHYSICS Guest
2024-11-22 1:23 |
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Conference: Bucharest University Faculty of Physics 2012 Meeting
Section: Atomic and Molecular Physics; Astrophysics
Title:
Preliminary results on coronal jet contribution to the slow solar wind flux
Authors:
S.RADU (2), A.R.PARASCHIV (3,1), D. DRAGOMIRESCU (2), L. STAN (2), D.C.TALPEANU (2), C.IVAN (2), Daniela A.LACATUS (3,1), Marilena MIERLA (3,1)
Affiliation:
(1) Research Center for Atomic Physics and Astrophysics, Faculty of Physics, University of Bucharest, Str. Atomistilor 405, RO-077125, Magurele, Romania.
(2) Faculty of Physics, University of Bucharest, Str. Atomistilor 405, RO-077125, Magurele, Romania.
(3) Institute of Geodynamics of the Romanian Academy, Str. Jean-Louis Calderon 19-21, RO-020032, Bucharest, Romania.
E-mail
radu.sbt@gmail.com, paraschiv_alin_razvan@yahoo.com
Keywords:
Sun, jets, corona, solar wind
Abstract:
The slow solar wind is a continuous flux of charged particles that are ejected from the Sun`s corona. Coronal jets are proposed as a possible source candidate. A sample of events, from an existing catalog was analyzed, and ejected jet mass has been estimated.First results are now presented. In the future all the catalog will be analysed, in order to obtain the average jet particle flux. The results will be compared with other measurements in order to assess the total coronal jet contribution to the slow solar wind flux.
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