Radial evolution of the April 2020 stealth coronal mass ejection between 0.8 and 1 AU
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Published:2021-12
Issue:
Volume:656
Page:A1
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ISSN:0004-6361
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Container-title:Astronomy & Astrophysics
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language:
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Short-container-title:A&A
Author:
Freiherr von Forstner Johan L.ORCID, Dumbović MatejaORCID, Möstl Christian, Guo JingnanORCID, Papaioannou AthanasiosORCID, Elftmann Robert, Xu ZigongORCID, Christoph Terasa Jan, Kollhoff Alexander, Wimmer-Schweingruber Robert F., Rodríguez-Pacheco JavierORCID, Weiss Andreas J., Hinterreiter Jürgen, Amerstorfer Tanja, Bauer Maike, Belov Anatoly V., Abunina Maria A.ORCID, Horbury TimothyORCID, Davies Emma E.ORCID, O’Brien Helen, Allen Robert C.ORCID, Bruce Andrews G., Berger Lars, Boden Sebastian, Cernuda Cangas IgnacioORCID, Eldrum Sandra, Espinosa Lara FranciscoORCID, Gómez Herrero RaúlORCID, Hayes John R., Ho George C.ORCID, Kulkarni Shrinivasrao R.ORCID, Jeffrey Lees W., Martín César, Mason Glenn M.ORCID, Pacheco DanielORCID, Prieto Mateo ManuelORCID, Ravanbakhsh Ali, Rodríguez Polo OscarORCID, Sánchez Prieto SebastiánORCID, Schlemm Charles E., Seifert Helmut, Tyagi Kush, Yedla MaheshORCID
Abstract
Aims. We present observations of the first coronal mass ejection (CME) observed by the Solar Orbiter spacecraft on April 19, 2020 and the associated Forbush decrease (FD) measured by the High Energy Telescope (HET). This CME is a multi-spacecraft event that was also seen near Earth the following day.
Methods. We highlight the capabilities of the HET for observing small short-term variations of the galactic cosmic ray count rate using its single detector counters. We applied the analytical ForbMod model to the FD measurements to reproduce the Forbush decrease at both locations. Input parameters for the model were derived from both in situ and remote-sensing observations of the CME.
Results. The very slow (∼350 km s−1) stealth CME caused an FD with an amplitude of 3% in the low-energy cosmic ray measurements at HET and 2% in a comparable channel of the Cosmic Ray Telescope for the Effects of Radiation (CRaTER) on board the Lunar Reconnaissance Orbiter, as well as a 1% decrease in neutron monitor measurements. Significant differences are observed in the expansion behavior of the CME at different locations, which may be related to influence of the following high speed solar wind stream. Under certain assumptions, ForbMod is able to reproduce the observed FDs in low-energy cosmic ray measurements from HET as well as CRaTER, however, with the same input parameters, the results do not agree with the FD amplitudes at higher energies measured by neutron monitors on Earth. We study these discrepancies and provide possible explanations.
Conclusions. This study highlights the notion that the novel measurements of Solar Orbiter can be coordinated with observations from other spacecraft to improve our understanding of space weather in the inner heliosphere. Multi-spacecraft observations combined with data-based modeling are also essential for understanding the propagation and evolution of CMEs, in addition to their space weather impacts.
Funder
Chinese Academy of Sciences CNSA EU H2020 Croatian Science Foundation National Observatory of Athens NASA Russian Science Foundation Austrian Science Fund Deutsches Zentrum für Luft- und Raumfahrt e.V. ESA
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by
19 articles.
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