Results 11 to 20 of about 6,760 (227)
Observations of a new foreshock region upstream of a foreshock bubble's shock [PDF]
Earth's foreshock is a region within the solar wind upstream of Earth's bow shock filled with backstreaming solar wind particles reflected at the shock.
Vassilis Angelopoulos, Heli Hietala
exaly +4 more sources
Helium in the Earth's foreshock: a global Vlasiator survey [PDF]
The foreshock is a region of space upstream of the Earth's bow shock extending along the interplanetary magnetic field (IMF). It is permeated by shock-reflected ions and electrons, low-frequency waves, and various plasma transients.
M. Battarbee +21 more
doaj +3 more sources
On the edge of the foreshock: model-data comparisons [PDF]
We present the results of a global hybrid code simulation for the solar wind-interaction with the Earth's magnetosphere during an interval of steady radial IMF.
D. G. Sibeck +3 more
doaj +4 more sources
Characterization of Foreshock Plasma Populations at Mercury
Observations of foreshock plasma populations at Mercury are presented utilizing measurements from the Fast Imaging Plasma Spectrometer aboard the Mercury Surface, Space Environment, Geochemistry, and Ranging spacecraft.
A. N. Glass +5 more
semanticscholar +2 more sources
The statistics of foreshock cavities: results of a Cluster survey [PDF]
We use Cluster magnetic field, thermal ion, and energetic particle observations upstream of the Earth's bow shock to investigate the occurrence patterns of foreshock cavities. Such cavities are thought to form when bundles of magnetic field connect to
L. Billingham +2 more
doaj +4 more sources
Statistical study of foreshock cavitons [PDF]
In this work we perform a statistical analysis of 92 foreshock cavitons observed with the Cluster spacecraft 1 during the period 2001–2006. We analyze time intervals during which the spacecraft was located in the Earth's foreshock with durations ...
P. Kajdič +7 more
doaj +2 more sources
Ion Acceleration Inside Foreshock Transients [PDF]
AbstractRecent observations upstream of Earth's bow shock have revealed that foreshock transients can not only accelerate solar wind ions by reflection at their upstream boundaries but may also accelerate ions inside them. Evidence for the latter comes from comparisons of ion spectra inside and outside the cores, and from evidence of leakage of ...
Terry Z. Liu +4 more
core +5 more sources
Oxygen foreshock of Mars [PDF]
AbstractMars Express (MEX) has operated for more than 10 years in the environment of Mars, providing solar wind ion observations from the Analyzer of Space Plasmas and Energetic Atoms experiment's Ion Mass Analyser (IMA). On 21 September 2008, MEX/IMA detected foreshock-like discrete distributions of oxygen ions at around 1keV in the solar wind ...
Yamauchi, M. +5 more
openaire +2 more sources
Impact of Foreshock Transients on the Flank Magnetopause and Magnetosphere and the Ionosphere
Mesoscale (on the scales of a few minutes and a few RE) magnetosheath and magnetopause perturbations driven by foreshock transients have been observed in the flank magnetotail.
Chih-Ping Wang +3 more
doaj +2 more sources
3-D global hybrid simulations of magnetospheric response to foreshock processes
It has been suggested that ion foreshock waves originating in the solar wind upstream of the quasi-parallel (Q-||) shock can impact the planetary magnetosphere leading to standing shear Alfvén waves, i.e., the field line resonances (FLRs). In this paper,
Feng Shi +4 more
doaj +2 more sources

