Results 11 to 20 of about 6,080 (232)
Neural Distribution-Guided Botulinum Toxin Injection for Platysma muscle: A Split-Neck Comparison With Conventional Technique. [PDF]
ABSTRACT Background The platysma muscle plays a pivotal role in the formation of vertical neck bands and contributes to lower facial descent, making it a prime target for botulinum toxin type A (BoNT‐A) in aesthetic neck rejuvenation. Conventional protocols typically involve injecting across the entire muscle, necessitating a high number of injection ...
Yi KH +5 more
europepmc +2 more sources
A summary of observational records on periodicities above the rotational period in the Jovian magnetosphere [PDF]
The Jovian magnetosphere is a very dynamic system. The plasma mass-loading from the moon Io and the fast planetary rotation lead to regular release of mass from the Jovian magnetosphere and to a change of the magnetic topology.
E. A. Kronberg +3 more
doaj +1 more source
Early Stages of Galilean Moon Formation in a Water-depleted Environment
A key feature of the Galilean satellite system is its monotonic decrease in bulk density with growing distance from Jupiter, indicating an ice mass fraction that is zero in the innermost moon Io and about half in the outer moons Ganymede and Callisto ...
Olivier Mousis +5 more
doaj +1 more source
Electron cyclotron harmonic waves in Jovian magnetosphere as seen by Juno
Electron cyclotron harmonic (ECH) waves along with whistler mode waves are suggested to be responsible for causing the persistent diffuse aurora in Jupiter.
J. Joseph +5 more
doaj +1 more source
On the location of the Io plasma torus: Voyager 1 observations [PDF]
The Voyager 1 outbound ultraviolet observations of the Io plasma torus are used to determine the location of the ansae, to obtain a third viewing angle of this structure in the Jovian magnetosphere. At an angle of −114° with respect to the Sun–Jupiter
M. Volwerk
doaj +1 more source
Whistler-mode chorus waves are regarded as an important acceleration mechanism contributing to the formation of relativistic and ultra-relativistic electrons in the Jovian radiation belts.
BinBin Ni +8 more
doaj +1 more source
Observation of Turbulent Magnetohydrodynamic Cascade in the Jovian Magnetosheath
We present the first estimation of the energy cascade rate in Jupiter’s magnetosheath (MS). We use in situ observations from the Jovian Auroral Distributions Experiment and the magnetometer investigation instruments on board the Juno spacecraft, in ...
N. Andrés +8 more
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Wave-particle interactions triggered by whistler-mode chorus waves are an important contributor to the Jovian radiation belt electron dynamics. While the sensitivity of chorus-driven electron scattering to the ambient magnetospheric and wave parameters ...
Jing Huang +6 more
doaj +1 more source
AbstractThis paper reviews a new astrophysical subject: seismology of the giant planets. Seismology is dedicated to the sounding of the interior structure of any object; on the other hand, the interiors of the Jovian planets need to be constrained, in order to improve our knowledge of their structure and of their evolution, as well as the ...
openaire +1 more source
We present preliminary results of a new global Magnetohydrodynamics (MHD) simulation model of the Jovian magnetosphere. The model incorporates mass loading from Jupiter's satellite Io, the planet's fast corotation, and electrostatic coupling between its ...
YuXian Wang +4 more
doaj +1 more source

