Forward Modeling of Coronal Mass Ejection Flux Ropes in the Inner Heliosphere with 3DCORE. [PDF]
Space Weather, 2018 Möstl C +9 more
europepmc +2 more sources
Protean Manifestations of Systemic Lupus Erythematosus With Antiphospholipid Syndrome: A Case Report of a Rare Variant of Libman-Sack's Endocarditis and Optic Perineuritis. [PDF]
ACR Open RheumatolACR Open Rheumatology, Volume 8, Issue 4, April 2026.
Harata M, Abel A, Jin Y.
europepmc +2 more sources
On the Construction of Phenomenological Coronal Mass Ejection Models
Space Weather, 2021 We consider recently developed 3DCORE coronal mass ejection (CME) model. We find that the magnetic field of 3DCORE violates both Maxwellian equations: the one for absence of magnetic monopoles and the other one for Faraday induction (“frozen‐in ...
D. V. Peregoudov
doaj +1 more source
Earth-affecting solar transients: a review of progresses in solar cycle 24
Progress in Earth and Planetary Science, 2021 This review article summarizes the advancement in the studies of Earth-affecting solar transients in the last decade that encompasses most of solar cycle 24. It is a part of the effort of the International Study of Earth-affecting Solar Transients (ISEST)
Jie Zhang +18 more
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Redefining the boundaries of interplanetary coronal mass ejections from observations at the ecliptic plane [PDF]
, 2016 On 2015 January 6-7, an interplanetary coronal mass ejection (ICME) was observed at L1. This event, which can be associated with a weak and slow coronal mass ejection, allows us to discuss on the differences between the boundaries of the magnetic cloud ...
Cid, C. +3 more
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Simulation study on the propagation process of coronal mass ejection
地球与行星物理论评, 2022 Coronal mass ejection (CME) is a kind of space weather phenomenon caused by the intense activity of the sun. Important issues of concern to the space weather community include understanding the propagation and evolution of a particular CME in the corona ...
Mengxuan Ma, Fang Shen, Yousheng Liu
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Proton beam velocity distributions in an interplanetary coronal mass ejection [PDF]
Annales Geophysicae, 2009 The plasma and magnetic-field instruments on the Helios 2 spacecraft, which was on 3 April 1979 located at 0.68 AU, detected an interplanetary coronal mass ejection (ICME) that revealed itself by the typical signature of magnetic field rotation.
E. Marsch, S. Yao, C.-Y. Tu
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Coronal Mass Ejections: Observations [PDF]
Living Reviews in Solar Physics, 2012 Solar eruptive phenomena embrace a variety of eruptions, including flares, solar energetic particles, and radio bursts. Since the vast majority of these are associated with the eruption, development, and evolution of coronal mass ejections (CMEs), we focus on CME observations in this review. CMEs are a key aspect of coronal and interplanetary dynamics.
David F. Webb, Timothy A. Howard
openaire +2 more sources
Journal of Space Weather and Space Climate, 2019 A three-dimensional time-dependent, numerical magnetohydrodynamic simulation is performed to investigate the propagation of a coronal mass ejection that occurred on 12 December 2008.
Zhang Man, Feng Xue Shang, Yang Li Ping
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Planar magnetic structures in coronal mass ejection-driven sheath regions [PDF]
Annales Geophysicae, 2016 Planar magnetic structures (PMSs) are periods in the solar wind during which interplanetary magnetic field vectors are nearly parallel to a single plane.
E. Palmerio +3 more
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