Steepening of waves at the duskside magnetopause
Surface waves at the magnetopause flanks typically feature steeper, i.e., more inclined leading (antisunward facing) than trailing (sunward facing) edges. This is expected for Kelvin‐Helmholtz instability (KHI) amplified waves.
F. Plaschke +17 more
doaj +1 more source
Flux Transfer Events at a Reconnection‐Suppressed Magnetopause: Cassini Observations at Saturn [PDF]
J. M. Jasinski +7 more
openalex +1 more source
On the Collisionless Asymmetric Magnetic Reconnection Rate
A prediction of the steady state reconnection electric field in asymmetric reconnection is obtained by maximizing the reconnection rate as a function of the opening angle made by the upstream magnetic field on the weak magnetic field (magnetosheath) side.
Yi‐Hsin Liu +5 more
doaj +1 more source
Thick escaping magnetospheric ion layer in magnetopause reconnection with MMS observations
The structure of asymmetric magnetopause reconnection is explored with multiple point and high‐time‐resolution ion velocity distribution observations from the Magnetospheric Multiscale mission.
T. Nagai +22 more
doaj +1 more source
Large-Scale Statistical Survey of Magnetopause Reconnection [PDF]
Samantha Piatt
openalex +1 more source
Concerning the location of magnetopause merging as a function of the magnetopause current strength [PDF]
I. I. Alexeev +2 more
openalex +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
Mercury’s Bow Shock and Magnetopause Variations According to MESSENGER Data
Using data from the MESSENGER spacecraft magnetometer that describes the magnetopause and the bow shock crossing points of the Mercury’s magnetosphere, we have calculated the parameters of the paraboloids of revolution approximating the obtained points ...
Dmitry Nevsky +2 more
doaj +1 more source
Characterization of Alfvenic fluctuations in the magnetopause boundary layer [PDF]
L. Rezeau +4 more
openalex +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

