Results 31 to 40 of about 290,306 (312)
Dynamics of the Magnetotail Plasma Sheet Current
Magnetospheric plasma can be investigated as a continuum by adopting magnetic field B and plasma flow u as primary parameters in the Bu paradigm or as a collection of individual particles by adopting electric field E and electrical current j as primary ...
Anthony Tat Yin Lui
doaj +1 more source
RADIATING CURRENT SHEETS IN THE SOLAR CHROMOSPHERE [PDF]
An MHD model of a Hydrogen plasma with flow, an energy equation, NLTE ionization and radiative cooling, and an Ohm's law with anisotropic electrical conduction and thermoelectric effects is used to self-consistently generate atmospheric layers over a $50$ km height range.
Goodman, Michael L., Judge, Philip G.
openaire +2 more sources
Transition from substorm growth to substorm expansion phase as observed with a radial configuration of ISTP and Cluster spacecraft [PDF]
International audienceTransition from the growth phase to the substorm expansion during a well-isolated substorm with a strong growth phase is investigated using a unique radial (THEMIS-like) spacecraft constellation near midnight, including the probing ...
Sergeev, V.A. +36 more
core +1 more source
Optimal Energy Growth in Current Sheets [PDF]
In this paper, we investigate the possibility of transient growth in the linear perturbation of current sheets. The resistive magnetohydrodynamic (MHD) operator for a background field consisting of a current sheet is non-normal, meaning that associated eigenvalues and eigenmodes can be very sensitive to perturbation. In a linear stability analysis of a
MacTaggart, David, Stewart, Peter
openaire +2 more sources
The heliospheric current sheet [PDF]
The heliospheric current sheet (HCS) is the boundary between open oppositely directed magnetic field lines which commonly originate as the outward extension of the solar magnetic dipole. The dipole tilt, the rotation of the Sun, and the outward propagation of the solar wind cause peaks and valleys in the current sheet which spiral outward.
openaire +1 more source
Galactic cosmic ray modulation near the heliospheric current sheet
Galactic cosmic rays (GCRs) are modulated by the heliospheric magnetic field (HMF) both over decadal time scales (due to long-term, global HMF variations), and over time scales of a few hours (associated with solar wind structures such as coronal mass ...
Owens, M. J. +7 more
core +1 more source
South-north asymmetry of field-aligned currents in the magnetotail observed by Cluster [PDF]
We statistically investigated features of the field-aligned current (FAC) distribution in plasma sheet boundary layers between 17 and 19 RE in the magnetotail using the curlometer technique to calculate the current from four-point magnetic field ...
Lahiff, A. D. +86 more
core +1 more source
Current Sheet Statistics in the Magnetosheath
The magnetosheath (MSH) plasma turbulence depends on the structure and properties of the bow shock (BS). Under quasi-parallel (Q||) and quasi-perpendicular (Q⊥) BS configurations the electromagnetic field and plasma quantities possess quite distinct ...
Emiliya Yordanova +4 more
doaj +1 more source
Cluster as current sheet surveyor in the magnetotail [PDF]
A novel analysis technique is presented to estimate the current sheet thickness unambiguously and directly, without associating time series data with spatial structure.
Y. Narita, R. Nakamura, W. Baumjohann
doaj +1 more source
“Matreshka” model of multilayered current sheet [PDF]
Current sheets are one of the key elements of the Earth's magnetosphere, determining the magnetic energy storage and release. An analytical self‐consistent model of multicomponent thin current sheets, where the plasma consists of ions of both solar wind and ionospheric origin, is presented. The influence of the electron population is taken into account
Zelenyi, L.M. +5 more
openaire +4 more sources

