Results 81 to 90 of about 1,337 (185)
An intrinsic limitation of empirical models of the magnetopause location is a predefined magnetopause shape and assumed functional dependences on relevant parameters.
M. Aghabozorgi Nafchi +7 more
doaj +1 more source
Estimating the subsolar magnetopause position from soft X-ray images using a low-pass image filter
The Lunar Environment heliospheric X-ray Imager (LEXI) and Solar wind Magnetosphere Ionosphere Link Explorer (SMILE) missions will image the Earth’s dayside magnetopause and cusps in soft X-rays after their respective launches in the near future, to ...
Hyangpyo Kim +11 more
doaj +1 more source
Experimental and numerical investigation of plasma parameters in the magnetosheath
We investigate the behaviour of the plasma parameters in the magnetosheath in a case when Interball-1 satellite stayed in the magnetosheath, crossing the tail magnetopause.
Dobreva Polya +4 more
doaj +1 more source
The Electric Properties of the Magnetopause Boundary Layer
The magnetopause plays a pivotal role in the coupling among solar wind, the magnetosheath, and the magnetosphere. By analyzing magnetopause crossing events using MMS, we reveal a local non-neutrality of electric charges in the magnetopause boundary layer
Lai Gao +4 more
doaj +1 more source
Observations of the Crustal Mini-magnetopause Reconnection at Mars
Magnetopause reconnection is a fundamental mechanism for mass and energy transfer in terrestrial planetary systems. Unlike Earth, Mars lacks a global magnetic field and instead has localized crustal magnetic fields, which can create structures ...
Xinzhi Qiu +6 more
doaj +1 more source
Occurrence of Kelvin–Helmholtz Instability at Lunar Distance Magnetopause: ARTEMIS Observation
Kelvin–Helmholtz waves can be observed frequently at the near-Earth magnetopause and play an important role in the transport of particles, momentum, and energy from the solar wind to the magnetosphere.
J. Y. Feng +7 more
doaj +1 more source
A linear perturbation analysis of magnetopause motion in the Newton-Busemann limit
The response of the magnetopause surface to time-varying solar wind dynamic pressure is examined. We argue that to a first approximation the magnetopause surface may be considered as analogous to an elastic membrane.
M. P. Freeman +2 more
doaj
Dawn-dusk Asymmetrical Distribution of Saturn's Cusp. [PDF]
Xu Y +12 more
europepmc +1 more source
Impact of ICME sheath planarity on Earth's outer radiation belt. [PDF]
Ghag K +9 more
europepmc +1 more source
Energy transfer across magnetopause under dawn-dusk IMFs. [PDF]
Zhang HX, Lu JY, Wang M.
europepmc +1 more source

