Speaker
Salvo Guglielmino
(Istituto Nazionale di Astrofisica (INAF))
Description
On 25 March 2022, during the first perihelion of the Solar Orbiter Nominal Mission, the Metis coronograph observed a fast CME at the East limb, between 05:02 and 07:02 UT.
We were able to identify the source region of the ejection in active region NOAA 12974. This was observed on the solar disk by the SDO/AIA and Hinode/XRT instruments, enabling us to study the flaring event connected with the CME. Complementary information provided by the STIX instrument allow us to estimate the amount of non-thermal energy and kinetic energy involved in the flare.
We report on this event, as a showcase of the capabilities of a synergetic approach between the multi-vantage point observations of Solar Orbiter and those of other satellite instruments.
| Submit to 'solar physics' topical issue? | Yes |
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Primary author
Salvo Guglielmino
(Istituto Nazionale di Astrofisica (INAF))
Co-authors
Prof.
Marco Romoli
(University of Florence)
Dr
Vincenzo Andretta
(INAF OACN)
Dr
Roberto Susino
(INAF OATO)
Dr
Giuliana Russano
(INAF OACN)
Dr
Paolo Romano
(INAF)
Dr
Daniele Spadaro
(INAF OACT)
Prof.
Michele Piana
(University of Genoa)
Dr
Paolo Massa
(Western Kentucky University)
Ms
Anna Volpara
(University of Genoa)
Dr
Sabrina Guastavino
(University of Genoa)
Prof.
Anna Maria Massone
(University of Genoa)
