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2017 AGU Chapman Conference on Dayside Magnetosphere Interactions
2017 AGU Chapman Conference Dayside Magnetosphere Interactions
2017/3/10
This conference will address the processes by which solar wind mass, momentum, and energy enter the magnetosphere. Regions of interest include the foreshock, bow shock, magnetosheath, magnetopause, an...
AXIOM: Advanced X-ray Imaging Of the Magnetosphere
X-rays. Space telescope. Space plasma instrumentation Magnetometer Techniques:Imaging spectroscopy plasma field analysers
2011/9/27
Planetary plasma and magnetic field environments can be studied by in situ measurements or by remote sensing. While the former provide precise information about plasma behaviour, instabilities and dyn...
Varying disc-magnetosphere coupling as the origin of pulse profile variability in SAX J1808.4-3658
accretion accretion discs – pulsars:individual:SAX J1808.4–3658 – stars:neu-tron – X-rays:binaries
2011/9/26
Accreting millisecond pulsars show significant variability of their pulse profiles, especially at low accretion rates. On the other hand, their X-ray spectra are remarkably similar with not much varia...
Formation of "Lightnings" in a Neutron Star Magnetosphere and the Nature of RRATs
neutron stars, pulsars, rotating radio transients.
2011/9/15
The connection between the radio emission from “lightnings” produced by the absorption of high-energy photons from the cosmic gamma-ray background in a neutron star magnetosphere and radio bursts from...
Origin And Evolution Of Energetic Particle Populations In The Magnetosphere
Constant current ions electrons magnetosphere ionosphere solar wind
2017/3/23
There is a constant flow of electrons ions and into and out of the magnetosphere and the intricacies of the magnetosphere determine the paths that these particles take through it. Although the plasma ...
Magnetosphere-Ionosphere Coupling Through E-region Turbulence: Anomalous Conductivities and Frictional Heating
Anomalous Conductivities Frictional Heating
2017/3/22
Global magnetospheric MHD codes using ionospheric conductances based on laminar
models systematically overestimate the cross-polar cap potential during storm time by
up to a factor of two. At these ...
Conjectured chaotic nature of the ionosphere-magnetosphere coupling in a reconfigurating magnetosphere
Conjectured chaotic nature ionosphere-magnetosphere coupling reconfigurating magnetosphere
2009/11/16
During substorms the magnetic field configuration changes in time; stretching of the magnetosphere during growth phase is followed by its collapse after the onset of the expansion phase. In this study...
Evaluation on the analogy between the dynamic magnetosphere and a forced and/or self-organized critical system
Evaluation on the analogy dynamic magnetosphere self-organized critical system
2009/11/12
The dissipation power and size of auroral blobs are investigated in detail to examine the possible analogy between the dynamic magnetosphere and a forced and/or self-organized critical system. The dis...
Large amplitude solitary waves in and near the Earth’s magnetosphere,magnetopause and bow shock:Polar and Cluster observations
Large amplitude solitary waves Earth’s magnetosphere magnetopause bow shock
2009/11/11
Solitary waves with large electric fields (up to 100's of mV/m) have been observed throughout the magnetosphere and in the bow shock. We discuss observations by Polar at high altitudes ( ~ 4-8 RE ), d...
Testing the hypothesis of the Earth's magnetosphere behaving like an avalanching system
hypothesis Earth's magnetosphere avalanching system
2009/11/11
The global auroral dissipation power as observed by the imager on the Polar spacecraft is used as a proxy for the power dissipation of the Earth's magnetosphere to examine whether or not the magnetosp...
Mitigation of energetic electrons in the magnetosphere by amplified whistler wave under double cyclotron resonances
energetic electrons magnetosphere amplified whistler wave double cyclotron resonances
2009/11/2
An optimal approach reducing the population of MeV electrons in the magnetosphere is presented. Under a double resonance condition, whistler wave is simultaneously in cyclotron resonance with keV and ...
The effect of upstream turbulence and its anisotropy on the efficiency of solar wind–magnetosphere coupling
upstream turbulence anisotropy efficiency of solar wind magnetosphere coupling
2009/11/2
The importance of space weather and its forecasting is growing as interest in studying geoeffective processes in the Sun – solar wind – magnetosphere – ionosphere coupled system is increasing. This pa...
Solar wind interaction with the Earth's magnetosphere:the role of reconnection in the presence of a large scale sheared flow
Solar wind interaction Earth's magnetosphere role of reconnection large scale sheared flow
2009/10/30
The Earth's magnetosphere and solar wind environment is a laboratory of excellence for the study of the physics of collisionless magnetic reconnection. At low latitude magnetopause, magnetic reconnect...
Azimuthal field perturbations in the jovian magnetosphere：ulysses observations
jovian magnetosphere ulysses observations Azimuthal field perturbations
2009/6/4
Azimuthal field perturbations in the jovian magnetosphere：ulysses observations。
Magnetic turbulence in and around the Earth's magnetosphere
Magnetic turbulence Earth's magnetosphere
2009/5/27
Magnetic turbulence is found in most space plasmas, including the geospace environment. Recent spacecraft observations of magnetic turbulence in the ion foreshock, in the magnetosheath, in the polar ...