Results 11 to 20 of about 1,762,916 (284)
Geomagnetic storms driven by ICME- and CIR-dominated solar wind. [PDF]
, 2006 The interaction of the solar wind and the Earth's magnetosphere is complex and the phenomenology of the interaction is very different for solar wind dominated by interplanetary coronal mass ejections (ICMEs) compared to solar wind dominated by corotating
Liemohn, M. W. +8 more
core +5 more sources
Solar wind dependence of ion parameters in the earth's magnetospheric region calculated from CLUSTER observations [PDF]
, 2008 Moments calculated from the ion distributions (~0–40 keV) measured by the Cluster Ion Spectrometry (CIS) instrument are combined with data from the Cluster Flux Gate Magnetometer (FGM) instrument and used to characterise the bulk properties of the plasma
Denton, M. H., Taylor, M. G. G. T.
core +5 more sources
Voyager 2 observation of the multifractal spectrum in the heliosphere and the heliosheath [PDF]
Nonlinear Processes in Geophysics, 2013 We look in detail at the multifractal scaling of the fluctuations in the interplanetary magnetic field strength as measured onboard Voyager 2 in the entire heliosphere and even in the heliosheath.
W. M. Macek, A. Wawrzaszek
doaj +1 more source
Neutral solar wind generated by lunar exospheric dust at the terminator [PDF]
Journal of Geophysical Research: Space Physics, 2009 We calculate the flux of neutral solar wind observed on the lunar surface at the terminator due to solar wind protons penetrating exospheric dust grains with (1) radii greater than 0.1 μm and (2) radii greater than 0.01 μm. For grains with radii larger than 0.1 μm, the ratio of the neutral solar wind flux produced by exospheric dust to the incident ...
Collier, Michael R., Stubbs, Timothy J.
openaire +2 more sources
The Astrophysical Journal, 2023 We present a time-dependent, three-dimensional single-fluid model for the transport of magnetohydrodynamic (MHD) turbulence that is self-consistently evolving with a dynamic large-scale solar wind in the outer heliosphere.
Jens Kleimann +3 more
doaj +1 more source
A two-component transport model for solar wind fluctuations: Waves plus quasi-2D turbulence [PDF]
, 2010 We present a model for the transport of solar wind fluctuations, based on the assumption that they can be well-represented using two distinct components: a quasi-2D turbulence piece and a wave-like piece.
Matthaeus, William H. +3 more
core +1 more source
Unexpected sites of efficient stochastic acceleration in the inner heliosheath [PDF]
Annales Geophysicae, 2007 Up until the recent past, it was generally believed that the solar wind termination shock (TS) is the favourite site to accelerate ions from the keV- to the MeV- energy levels by means of Fermi-1 processes.
S. V. Chalov +3 more
doaj +1 more source
Mediation of the solar wind termination shock by non-thermal ions [PDF]
Nature, 2008 Broad regions on both sides of the solar wind termination shock are populated by high intensities of non-thermal ions and electrons. The pre-shock particles in the solar wind have been measured by the spacecraft Voyager 1 (refs 1-5) and Voyager 2 (refs 3, 6).
Decker, R. B. +7 more
openaire +3 more sources
Solar cycle dependence of scaling in solar wind fluctuations [PDF]
, 2008 In this review we collate recent results for the statistical scaling properties of fluctuations in the solar wind with a view to synthesizing two descriptions: that of evolving MHD turbulence and that of a scaling signature of coronal origin that ...
B. Hnat +6 more
core +2 more sources
The influence of solar wind variability on magnetospheric ULF wave power [PDF]
, 2015 Magnetospheric ultra-low frequency (ULF) oscillations in the Pc 4–5 frequency range play an important role in the dynamics of Earth's radiation belts, both by enhancing the radial diffusion through incoherent interactions and through the coherent drift ...
Murphy, KR +7 more
core +2 more sources