Results 161 to 170 of about 932,549 (275)

Small-amplitude Compressible Magnetohydrodynamic Turbulence Modulated by Collisionless Damping in Earth’s Magnetosheath: Observation Matches Theory

open access: yesThe Astrophysical Journal
Plasma turbulence is a ubiquitous dynamical process that transfers energy across many spatial and temporal scales and affects energetic particle transport.
Siqi Zhao   +4 more
doaj   +1 more source

Formation of H+ PUI Tails Downstream of Distant Interplanetary Shocks

open access: yesThe Astrophysical Journal
New Horizons’ Solar Wind Around Pluto (SWAP) instrument has observed interplanetary shocks from ∼20 to 60 au from the Sun. Different studies have analyzed the effects of these shocks on the solar wind ion (SWI) and interstellar pickup ion (PUI ...
E. J. Zirnstein   +11 more
doaj   +1 more source

Mode Composition Shapes Magnetic Anisotropy in Solar Wind Turbulence

open access: yesThe Astrophysical Journal
Turbulence is a ubiquitous process that transfers energy across many spatial and temporal scales, thereby influencing particle transport and heating. Recent progress has improved our understanding of the anisotropy of turbulence with respect to the mean ...
Siqi Zhao   +3 more
doaj   +1 more source

A Brief Review of Interplanetary Physics Research Progress in Mainland China during 2020–2022

open access: yesChinese Journal of Space Science, 2022
Xinhua ZHAO   +7 more
openaire   +1 more source

Editorial: Magnetic Flux Ropes: From the Sun to the Earth and Beyond

open access: yesFrontiers in Astronomy and Space Sciences, 2020
Rui Liu   +6 more
doaj   +1 more source

Impact of ICME sheath planarity on Earth's outer radiation belt. [PDF]

open access: yesSci Rep
Ghag K   +9 more
europepmc   +1 more source

Quantifying the evolution of interplanetary coronal mass ejections by coupling physics-based and data-driven modeling

open access: yes, 2022
Coronal mass ejections (CMEs) are considered to be one of the main drivers of space weather. They consist of large-scale eruptions of magnetised plasma, originating predominantly from active regions in the low solar corona and are extremely common events. During solar maxima, they occur on a daily basis, at times exceeding 10 events per day.
openaire   +1 more source

IMAP's Role in Understanding Particle Injection and Energization Throughout the Heliosphere. [PDF]

open access: yesSpace Sci Rev
Cohen CMS   +30 more
europepmc   +1 more source

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