Search results for "UV radiation – Sun"

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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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Analysis of a multi-wavelength time-resolved observation of a coronal loop

2005

Several items on the diagnostics and interpretation of coronal loop observations are under debate. In this work, we analyze a well-defined loop system detected in a time-resolved observation in several spectral bands. The dataset includes simultaneous images in the TRACE 171 A, 195 A and 284 A bands, and Yohkoh/SXT, and two rasters taken with SoHO/CDS in twelve relevant lines. The loop is initially best visible in the TRACE 195 A filter band, and later in the 171 A filter band, with correspondence with the CDS raster images at log T \~ 6.0-6.1. We have taken as pixel-by-pixel background the latest TRACE, Yohkoh and CDS images where the loop has faded out. We examine the loop morphology evol…

PhysicsBackground subtractionbusiness.industryAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsSpectral bandsCoronal loopAstrophysicsLight curveSpectral lineRatio distributionLoop (topology)corona – Sun : X-rays gamma raysOpticsUV radiation – SunSpace and Planetary ScienceFilter (video)business
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