亲密
发表于 2025-3-30 09:08:10
Hyperasymptotic Perturbation Theorye consistent with observational measurements, it will mean positive identification of the magnetic morphology that surrounds certain quiescent filaments, which will lead to a better understanding of how they form and why they erupt.
嘲弄
发表于 2025-3-30 14:48:17
J. Litva,A. Sandhu,K. Cho,T. Loormation to constrain CME models and probe various processes during the initial propagation of CMEs in the low corona, but also offer a possible cost-effective and low-risk means of space-weather monitoring.
parsimony
发表于 2025-3-30 18:17:23
Coronal Cavity Survey: Morphological Clues to Eruptive Magnetic Topologies,tween cavity shape, aspect ratio, and propensity for eruption. We find that cavities with a teardrop-shaped morphology are more likely to erupt, and we discuss the implications of this morphology for magnetic topologies associated with CME models. We provide the full details of the survey for broad scientific use as supplemental material.
龙卷风
发表于 2025-3-31 00:30:05
Polarimetric Properties of Flux Ropes and Sheared Arcades in Coronal Prominence Cavities,e consistent with observational measurements, it will mean positive identification of the magnetic morphology that surrounds certain quiescent filaments, which will lead to a better understanding of how they form and why they erupt.
Immobilize
发表于 2025-3-31 02:05:34
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光滑
发表于 2025-3-31 08:21:58
he topical issue also contains contributions from researchers not present at the workshop..This volume is aimed at researchers and graduate students active in solar physics..Originally published in .Solar Physics., Vol. 288, Issue 2, 2013 and Vol. 289, Issue 8, 2014..978-1-4939-4983-0978-1-4939-2038-9
Vertebra
发表于 2025-3-31 10:22:50
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orthopedist
发表于 2025-3-31 14:30:08
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召集
发表于 2025-3-31 20:15:18
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DEBT
发表于 2025-4-1 01:41:30
Transactional Aspects of Workflows,ven if one integrates for several minutes to reach the required signal-to-noise ratio, and despite the rapidly changing intensity in the model (just as in observations). This variability of the intensity is often used as an argument against transition region magnetic diagnostics, which requires expo