Dissipative Pulsar Magnetosphere [PDF]
Journal of Cosmology and Astroparticle Physics, 2008 Dissipative axisymmetric pulsar magnetosphere is calculated by a direct numerical simulation of the Strong-Field Electrodynamics equations. The magnetic separatrix disappears, it is replaced by a region of enhanced dissipation.
Andrei Gruzinov +2 more
core +2 more sources
BLACK HOLE MAGNETOSPHERES [PDF]
The Astrophysical Journal, 2014 10 pages, 4 figures, recommended for publication in the Astrophysical ...
Antonios Nathanail, Ioannis Contopoulos
openaire +3 more sources
Organization of the magnetosphere during substorms [PDF]
, 2011 The change in degree of organization of the magnetosphere during substorms is investigated by analyzing various geomagnetic indices, as well as interplanetary magnetic field z-component and solar wind flow speed.
Abarbanel +44 more
core +2 more sources
The Astrophysical Journal Letters, 2023 Mars’s magnetosphere is hybrid, having contributions from both an induced magnetosphere like Venus and the localized crustal magnetic fields. However, the planetary fields also include large-scale, more global components.
Shaosui Xu +12 more
doaj +1 more source
Ionospheric conductance distribution and MHD wave structure: observation and model [PDF]
Annales Geophysicae, 1998 The ionosphere influences magnetohydrodynamic waves in the magnetosphere by damping because of Joule heating and by varying the wave structure itself.
F. Budnik +3 more
doaj +1 more source
Noise, Regression Dilution Bias, and Solar-Wind/Magnetosphere Coupling Studies
Frontiers in Astronomy and Space Sciences, 2022 Using numerical experiments, the effects of noise in the solar-wind and magnetospheric data on fits to the data are examined. In particular, the impact of noise amplitude on the functional forms of best-fit solar-wind driver functions is explored.
Joseph E. Borovsky
doaj +1 more source
Geophysical Monograph Series, Page i-xiv., 2021 Exploring the links between Large Igneous Provinces and dramatic environmental impact
An emerging consensus suggests that Large Igneous Provinces (LIPs) and Silicic LIPs (SLIPs) are a significant driver of dramatic global environmental and biological changes, including mass extinctions.
wiley +1 more source
A three-dimensional model for the radio emission of magnetic chemically peculiar stars [PDF]
, 2004 In this paper we present a three-dimensional numerical model for the radio emission of Magnetic Chemically Peculiar stars, on the hypothesis that energetic electrons emit by the gyrosynchrotron mechanism. For this class of radio stars, characterized by a
Buemi, C. S. +4 more
core +2 more sources
The Geoeffectiveness of Solar Wind Current Sheets and Its Modulation by Foreshock Ions
Geophysical Research Letters, 2022 We examined the evolution of 34 solar wind bifurcated current sheets in the magnetosheath and their magnetospheric responses, using the in‐situ observations of the THEMIS probes and the GOES satellites.
Boyi Wang +3 more
doaj +1 more source
A Statistical Investigation of Factors Influencing the Magnetotail Twist at Mars
Geophysical Research Letters, 2022 The Martian magnetotail exhibits a highly twisted configuration, shifting in response to changes in polarity of the interplanetary magnetic field's (IMF) dawn‐dusk (BY) component.
Gina A. DiBraccio +14 more
doaj +1 more source