Results 1 to 10 of about 196,114 (210)
Using Mars Atmosphere and Volatile EvolutioN Magnetometer observations, we report the first statistical study of ultralow frequency (ULF) waves at the Martian foreshock.
Nahuel Andrés +5 more
doaj +1 more source
Mercury’s plasma environment after BepiColombo’s third flyby
Understanding Mercury’s magnetosphere is crucial for advancing our comprehension of how the solar wind interacts with the planetary magnetospheres. Despite previous missions, several gaps remain in our knowledge of Mercury’s plasma environment.
Lina Z. Hadid +24 more
doaj +1 more source
Statistical Distributions of Plasma Density and Pressure in the Jovian Plasma Sheet
The Jovian plasma sheet is a key region of the Jovian magnetosphere populated by a mix of warm and hot plasma. It is the main channel for radial transport of mass and energy in the Jovian magnetosphere and provides a favorable environment for magnetic ...
Haobo Fu +7 more
doaj +1 more source
Determining the State of Jupiter’s Magnetosphere Using In Situ and Remote Sensing Observations
While Jupiter’s magnetosphere is primarily governed by internal processes, variations in solar wind conditions can significantly modulate magnetospheric energy.
J. W. Sun +11 more
doaj +1 more source
A Simulation Study of an HFA-like Event at Mars
Hot flow anomalies (HFAs) are transient structures at planetary bow shocks characterized by hot, tenuous plasma. At Mars, where no global dipole field exists, such events interact with the induced magnetosphere in a unique and poorly understood way. This
Maodong Yan +4 more
doaj +1 more source
Saturn’s Recurrent Auroral Flashes in the Equinoctial Campaign
The past decades of Cassini’s investigation around Saturn have revealed the frequent occurrence of ∼1 hr quasiperiodic (QP) signatures in the in situ magnetic field and plasma measurements and plasma wave observations. Saturn’s aurora, as the response to
Tianshu Qin +4 more
doaj +1 more source
STRUCTURE AND DYNAMICS OF PLANETARY MAGNETOSPHERES
The interactions between the ambient plasmas and the objects of the Solar System result in variable exchanges both in time and space of mass, momentum and energy within different types of magnetospheres. The characterization of the sources, the general circulation and the losses of the magnetospheric plasmas as well as the identification of the ...
openaire +1 more source
Triggering the Magnetopause Reconnection by Solar Wind Discontinuities
Magnetic reconnection is one of the most universal processes in space plasma that is responsible for charged particle acceleration and the mixing and heating of plasma populations.
Alexander Lukin +6 more
doaj +1 more source
Radial Evolution of Turbulence Spectra on the Jovian Magnetosheath Flanks: Juno Observations
The Jovian magnetosheath provides a unique environment for examining the radial evolution of magnetosheath turbulence due to its large spatial extent.
Hui Li +3 more
doaj +1 more source
Double Layers in the Martian Magnetosheath
The observation of electrostatic double layers in Martian magnetosheath plasma is reported, based on medium-frequency (100 Hz–32 kHz) electric field data recorded by the Langmuir Probe and Waves on board the Mars Atmosphere and Volatile Evolution ...
Sahil Pandey +4 more
doaj +1 more source

