Results 41 to 50 of about 12,575 (260)
Numerical simulations of a flux rope ejection
Coronal mass ejections (CMEs) are the most violent phenomena observed on the Sun. One of the most successful models to explain CMEs is the flux rope ejection model, where a magnetic flux rope is expelled from the solar corona after a long phase along ...
Pagano, P. +6 more
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Current sheets in the Sun’s corona [PDF]
Current sheets play an important role in the Sun’s atmosphere, especially in coronal heating events and solar flares. They may form in response to motions of the magnetic footpoints in the solar surface or following a loss of equilibrium.
openaire +1 more source
This review aims to provide a broad understanding for interdisciplinary researchers in engineering and clinical applications. It addresses the development and control of magnetic actuation systems (MASs) in clinical surgeries and their revolutionary effects in multiple clinical applications.
Yingxin Huo +3 more
wiley +1 more source
From the Sun to the Earth: The 13 May 2005 Coronal Mass Ejection [PDF]
We report the results of a multi-instrument, multi-technique, coordinated study of the solar eruptive event of 13 May 2005. We discuss the resultant Earth-directed (halo) coronal mass ejection (CME), and the effects on the terrestrial space environment ...
Chashei, I. V. +111 more
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Fleeting Small-scale Surface Magnetic Fields Build the Quiet-Sun Corona
Arch-like loop structures filled with million Kelvin hot plasma form the building blocks of the quiet-Sun corona. Both high-resolution observations and magnetoconvection simulations show the ubiquitous presence of magnetic fields on the solar surface on ...
E. R. Priest +55 more
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ABSTRACT Congenital heart disease (CHD) and dermatologic conditions such as lymphedema and acquired melanocytic nevi (AMN) are common in Turner Syndrome (TS). We hypothesized that abnormalities of cranial neural crest cell derivatives drive the skin and heart manifestations of TS. We conducted joint cardiac and skin examinations of volunteers at a 2023
Sarah Elsaim +8 more
wiley +1 more source
SWIFF : space weather integrated forecasting framework [PDF]
This research has received funding from the European Commission’s FP7 Program with the grant agreement SWIFF (Project No. 2633430, swiff.eu). The KU Leuven simulations were conducted on the computational resources provided by the PRACE Tier-0 Project No.
Viviane Pierrard +84 more
core +1 more source
Development and application of a global magnetic field evolution model for the solar corona
Magnetic fields are fundamental to the structure and dynamics of the Sun’s corona. Observations show them to be locally complex, with highly sheared and twisted fields visible in solar filaments/prominences.
Yeates, Anthony Robinson
core
On the topology of global coronal magnetic fields
This thesis considers the magnetic topology of the global solar corona. To understand the magnetic topology we use the magnetic skeleton which provides us with a robust description of the magnetic field.
Edwards, Sarah J.
core
Der Beitrag geht der Frage nach, wie die Corona-Krise den Nachhaltigkeitsprozess transformiert. Die Effekte der Corona-Krise werden dabei im Kontext der verschiedenen, sich derzeit überlagernden globalen Krisen und Umbruchsprozesse diskutiert.
Brand, Karl-Werner
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