Speaker
Mr
Angelos Michailidis
(University of Ioannina)
Description
Abstract: Jets are collimated plasma eruptions found on the solar surface having sizes from few arcseconds to a fraction of the solar radius. We study cases of solar jets observed with Metis coronagraph on Solar Orbiter (SO), in combination with imagers as AIA on SDO or EUI on SO along with other coronagraphs such as LASCO/C2 on SOHO and COR2 on STEREO-A.
We characterize the jets geometry calculating the solar magnetic field with the PFSS model. The three-dimension shape of the jets is calculated using triangulation methods that combine images from different satellites.
The velocity of the jets is compared with calculations of the solar wind in the heliosphere.
Authors
Mr
Angelos Michailidis
(University of Ioannina)
Dr
Giulianna Russano
(INAF Astronomical Observatory of Capodimonte)
Mrs
Preity Sukla Sahani
(INAF Astronomical Observatory of Capodimonte)
Dr
Costis Gontikakis
(Research Center for Astronomy and Applied Mathematics, Academy of Athens)
Dr
Vincenzo Andretta
(INAF Astronomical Observatory of Capodimonte)
Prof.
Ioannis Daglis
(National Kapodistrian University of Athens)
Prof.
Nektarios Vlahakis
(National and Kapodistrian University of Athens)
