Results 101 to 110 of about 1,320 (193)
Comparison of Solar Wind Current Sheets in the Inner Heliosphere
The solar wind is filled with intense current sheets (magnetic field discontinuities) that host multiple instabilities and may undergo magnetic reconnection, a basic process for plasma heating and charged particle acceleration.
Zijin Zhang +4 more
doaj +1 more source
Scale and Time Dependence of Alfvénicity in the Solar Wind as Observed by the Parker Solar Probe
Alfvénicity is a well-known property, common in the solar wind, characterized by a high correlation between magnetic and velocity fluctuations. Data from the Parker Solar Probe (PSP) enable the study of this property closer to the Sun than ever before ...
Panisara Thepthong +6 more
doaj +1 more source
Distribution and Anisotropy of the Energy Transfer Rate in the Solar Wind Turbulence
The distribution of the energy transfer rate is critical for the interpretation of the intermittent energy cascade in the solar wind turbulence. However, the true observational distribution of the energy transfer rate in the solar wind and its anisotropy
Honghong Wu +4 more
doaj +1 more source
Induced magnetosphere of Mars responds fast to interplanetary magnetic field rotation. [PDF]
Lin R +13 more
europepmc +1 more source
Multiwavelength Multipoint Observations of the October 28, 2021 Type III Radio Burst. [PDF]
Martinez Oliveros JC +8 more
europepmc +1 more source
Shock-induced magnetic reconnection in the Venusian magnetotail. [PDF]
Zhang M +8 more
europepmc +1 more source
Plasma acceleration and boundary compression in the magnetosheath of Mars under low-Alfvén-Mach-number solar wind. [PDF]
Qiao F +20 more
europepmc +1 more source
Mars' induced magnetosphere can form under radial interplanetary magnetic field. [PDF]
Lin R +16 more
europepmc +1 more source

