Results 31 to 40 of about 334,315 (204)

Coordinated ground-based, low altitude satellite and Cluster observations on global and local scales during a transient post-noon sector excursion of the magnetospheric cusp [PDF]

open access: yes, 2001
On 14 January 2001, the four Cluster spacecraft passed through the northern magnetospheric mantle in close conjunction to the EISCAT Svalbard Radar (ESR) and approached the post-noon dayside magnetopause over Greenland between 13:00 and 14:00 UT.
Eglitis, P.   +58 more
core   +5 more sources

Auroral vortex street formed by the magnetosphere–ionosphere coupling instability [PDF]

open access: yesAnnales Geophysicae, 2015
By performing three-dimensional magnetohydrodynamic simulations including Alfvén eigenmode perturbations most unstable to the ionospheric feedback effects, we examined the auroral vortex street that often appears just before substorm onset.
Y. Hiraki
doaj   +1 more source

Magnetosphere dynamics during the 14 November 2012 storm inferred from TWINS, AMPERE, Van Allen Probes, and BATS-R-US–CRCM [PDF]

open access: yesAnnales Geophysicae, 2018
During the 14 November 2012 geomagnetic storm, the Van Allen Probes spacecraft observed a number of sharp decreases (dropouts) in particle fluxes for ions and electrons of different energies.
N. Buzulukova   +10 more
doaj   +1 more source

Observational evidence of ring current in the magnetosphere of Mercury [PDF]

open access: yesNature Communications, 2022
Abstract The magnetic gradient and curvature drift of energetic ions can form a longitudinal electric current around a planet known as the ring current, that has been observed in the intrinsic magnetospheres of Earth, Jupiter, and Saturn.
J.-T. Zhao   +11 more
openaire   +3 more sources

Morphology of the ring current derived from magnetic field observations [PDF]

open access: yesAnnales Geophysicae, 2004
Our examination of the 20 years of magnetospheric magnetic field data from ISEE, AMPTE/CCE and Polar missions has allowed us to quantify how the ring current flows and closes in the magnetosphere at a variety of disturbance levels.
G. Le, C. T. Russell, K. Takahashi
doaj   +1 more source

Current instabilities in the pulsar magnetosphere [PDF]

open access: yesProceedings of the International Astronomical Union, 2010
AbstractPulsars are rotating neutron stars with strong magnetic dipole fields (B = 104 − 109T), and high induced surface potentials (ca. 1014V). A strong charged particle current is driven out of the polar cap. It returns along an equatorial current sheet.
Axel Jessner   +2 more
openaire   +1 more source

Instability of the magnetosphere-ionosphere convection and formation of auroral arcs [PDF]

open access: yesAnnales Geophysicae, 1994
In this paper we study an instability of the plasma moving towards the Earth near the inner plasma sheet boundary. We include both the interchange instability of the plasma sheet and the magnetosphere-ionosphere interaction instability caused by an ...
A. E. Kozlovsky, W. B. Lyatsky
doaj   +1 more source

Event-oriented modelling of magnetic fields and currents during storms [PDF]

open access: yes, 2004
P(論文)We model the magnetospheric magnetic field during two storms, moderate and intense, using the event-oriented modelling technique which includes the representations of the magnetic field arising from the various magnetospheric current systems.
Ejiri, Masaki   +5 more
core   +1 more source

Current controversies in magnetospheric physics [PDF]

open access: yesReviews of Geophysics, 2001
The scientific ascent of humankind comes in two forms: incremental progress with traditional thinking, and paradigm transition. The latter typically engenders intense debate, often long lasting, before the transition of the paradigm is deemed acceptable.
openaire   +1 more source

Ionospheric control of the magnetosphere: conductance [PDF]

open access: yesAnnales Geophysicae, 2004
It is well known that the ionosphere plays a role in determining the global state of the magnetosphere. The ionosphere allows magnetospheric currents to close, thereby allowing magnetospheric convection to occur.
A. J. Ridley   +2 more
doaj   +1 more source

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