0000000000298233

AUTHOR

A. M. Malvezzi

showing 2 related works from this author

First light observations of the solar wind in the outer corona with the Metis coronagraph

2021

In this work, we present an investigation of the wind in the solar corona that has been initiated by observations of the resonantly scattered ultraviolet emission of the coronal plasma obtained with UVCS-SOHO, designed to measure the wind outflow speed by applying Doppler dimming diagnostics. Metis on Solar Orbiter complements the UVCS spectroscopic observations that were performed during solar activity cycle 23 by simultaneously imaging the polarized visible light and the H I Lyman-α corona in order to obtain high spatial and temporal resolution maps of the outward velocity of the continuously expanding solar atmosphere. The Metis observations, taken on May 15, 2020, provide the first H I …

010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaSolar windFOS: Physical sciencesAstrophysics01 natural sciencesWind speedlaw.inventionsymbols.namesakeSun: corona – solar wind – Sun: UV radiationlaw0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsCoronagraphSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesPhysics[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]Sun: coronaAstronomy and AstrophysicsPlasmaSolar wind Sun: corona Sun: UV radiationSun: UV radiationCoronaSolar windAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceTemporal resolutionPhysics::Space PhysicssymbolsOutflowDoppler effect
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The first coronal mass ejection observed in both visible-light and UV HI Ly-α channels of the Metis coronagraph on board Solar Orbiter

2021

Context.The Metis coronagraph on board Solar Orbiter offers a new view of coronal mass ejections (CMEs), observing them for the first time with simultaneous images acquired with a broad-band filter in the visible-light interval and with a narrow-band filter around the H ILy-αline at 121.567 nm, the so-called Metis UV channel.Aims.We show the first Metis observations of a CME, obtained on 16 and 17 January 2021. The event was also observed by the EUI/FSI imager on board Solar Orbiter, as well as by other space-based coronagraphs, such as STEREO-A/COR2 and SOHO/LASCO/C2, whose images are combined here with Metis data.Methods.Different images are analysed here to reconstruct the 3D orientation…

Physics010504 meteorology & atmospheric sciences[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]Sun: coronaSun: coronal mass ejections (CMEs)Astronomy and AstrophysicsAstrophysicsAlpha (navigation)Sun: UV radiation01 natural scienceslaw.inventionOn boardOrbiterSpace and Planetary Sciencelaw0103 physical sciencesCoronal mass ejectionMetis010303 astronomy & astrophysicsCoronagraphSun: atmosphere0105 earth and related environmental sciencesVisible spectrumSun: atmosphere – Sun: corona – Sun: UV radiation – Sun: coronal mass ejections (CMEs)
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