Results 91 to 100 of about 11,368 (206)
The objective of this study was to evaluate body development, growth performance, ingestive behavior, and physiological responses of Nelore and crossbred calves during the cow‐calf phase. Thirty beef calves were divided into four groups according to their genotype: Nelore (NE; eight animals), Nelore × Senepol (NS; eight animals), Nelore × Montana (NM ...
Lidianny S. Amorim +9 more
wiley +1 more source
Magnetic Topology and Loop Statistics in Observed Coronal Holes Using Potential Field Modeling
Potential field source surface (PFSS) models are widely used to study the solar corona and form the basis for solar wind forecasting, yet they often fail to reproduce observed properties of coronal holes.
Stephan G. Heinemann +2 more
doaj +1 more source
Optoelectronic Interfaces for Nongenetic Modulation of Excitable Tissues
This review summarizes recent advances in nongenetic optoelectronic technologies for the modulation of excitable biotissues, covering material selection, device design, and working principles, as well as characterization methods. Representative applications in in vitro and in vivo models of the cardiac, central, and peripheral nervous systems are ...
Qi Wang, Jinghua Li
wiley +1 more source
ARCANE–Early Detection of Interplanetary Coronal Mass Ejections
Abstract Interplanetary coronal mass ejections (ICMEs) are major drivers of space weather disturbances, posing risks to both technological infrastructure and human activities. Automatic detection of ICMEs in solar wind in situ data is essential for early warning systems.
Hannah T. Rüdisser +4 more
wiley +1 more source
We investigate the thermal properties of a solar flare by the observations of the soft X-ray Telescope on board Hinode and the Atmospheric Imaging Assembly (AIA) on board the Solar Dynamics Observatory. Our analysis reveals a tenuous but hot plasma cloud
Xiaoyan Xie +7 more
doaj +1 more source
Solar Flares as Cascades of Reconnecting Magnetic Loops
A model for the solar coronal magnetic field is proposed where multiple directed loops evolve in space and time. Loops injected at small scales are anchored by footpoints of opposite polarity moving randomly on a surface.
A.-L. Barabási +18 more
core +1 more source
On the Intermittency of Hot Plasma Loops in the Solar Corona
A recent analysis has suggested that the heating of plasma loops in the solar corona depends not just on the Poynting flux but also on processes yet to be identified.
Philip G. Judge, N. Paul M. Kuin
doaj +1 more source
Damped transverse oscillations of interacting coronal loops
Damped transverse oscillations of magnetic loops are routinely observed in the solar corona. This phenomenon is interpreted as standing kink magnetohydrodynamic waves, which are damped by resonant absorption owing to plasma inhomogeneity across the ...
Luna, Manuel, Soler, Roberto
core +1 more source
Magnetic Waves In Solar Coronal Loops
Final presentations of the Center for Astrophysics HEA/SSP Solar Summer Intern Program.
openaire +1 more source

