Results 51 to 60 of about 3,269,942 (182)
Solar and Stellar Coronal Mass Ejections - a review of the Cool Stars 21 splinter session
Coronal mass ejections (CMEs) are the most energetic phenomena related to magnetic activity and, by impacting the interplanetary space, they can be the source of severe planetary disturbances. Solar CMEs and their sources, such as flares and filament/prominence eruptions, have been intensively observed and studied over decades.
Chifu, Iulia +3 more
openaire +1 more source
Observing Solar Coronal Mass Ejections from Space [PDF]
In this contribution to the panel discussion of the IAU Symposium 388 Solar and Stellar Coronal Mass Ejections , I concentrate on white-light observations of solar coronal mass ejections (CMEs) from space and specifically address the following aspects ...
Lamy, Philippe
core +3 more sources
Editorial to the Special Issue “Propagation of Coronal Mass Ejections”
Coronal mass ejections (CMEs) and their associated shocks are one of the main drivers of heliosphere variability, causing both interplanetary and planetary perturbations [...
Fang Shen, Mateja Dumbović
core +1 more source
The insect stinger is among the best‐known venom‐delivery structures, yet its valvilli—paired flaps within the valve chamber—remain poorly understood. Using micro‐CT, histology, serial block‐face SEM and CLSM in the ant Diacamma nr. indicum, we show that the valvilli are not uniformly flexible flaps but are materially differentiated structures with ...
Alexandre Casadei‐Ferreira +6 more
wiley +1 more source
Abstract Variations in the solar wind, particularly those associated with interplanetary coronal mass ejections (ICMEs) and high‐speed streams (HSSs), drive geomagnetic disturbances that produce rapid changes in the ground magnetic field. These variations, commonly quantified by the time derivative of the horizontal magnetic field dBH/dt $\left({\text ...
José P. Marchezi +8 more
wiley +1 more source
Magnetospheric preconditioning under northward IMF: evidence from the study of coronal mass ejection and corotating interaction region geoeffectiveness [PDF]
Motivated by recent observations and simulations of the formation of a cold and dense plasma sheet in the tail of the magnetosphere under northward interplanetary magnetic field (IMF) and of the direct influence of the plasma sheet density on the ring ...
Pulkkinen, T. I. +4 more
core +4 more sources
Diagnosis of Coronal Mass Ejections through Local and Global Dimmings
Coronal dimmings are localized sharp reductions in soft X-ray and extreme ultraviolet (EUV) emission at the early expansion phase of coronal mass ejections (CMEs). Such local dimmings have global responses, known as Sun-as-a-star or global dimmings. Here,
Tao Ding, Jun Zhang, Ting Li
doaj +1 more source
Cosmic Ray Anisotropy Generated by the June 22nd 2015 Interplanetary Events
Abstract On 22 June 2015, the near Earth interplanetary space was perturbed by a series of high‐speed streamers and interplanetary coronal mass ejections associated with an active region and two low‐latitude coronal holes. The interaction of these disturbances gave rise to the complex solar wind structure observed at 1 au.
A. Lara, K. P. Arunbabu, T. Niembro
wiley +1 more source
Sun-as-a-star analyses serve as a bridge for comparative studies on solar and stellar activities. To investigate the typical Sun-as-a-star H α temporal spectral characteristics in solar eruption source regions, we analyzed five different types of solar ...
Xiaofeng Liu +8 more
doaj +1 more source
Major Space Weather Risks Identified via Coupled Physics‐Engineering‐Economic Modeling
Abstract Space weather poses an important but under‐quantified threat to society. While severe geomagnetic storms are recognized as potential global catastrophes, their socio‐economic impacts remain poorly quantified. We present a novel physics‐engineering‐economic framework that links geophysical drivers to power grid geoelectric fields, transformer ...
Edward J. Oughton +7 more
wiley +1 more source

