Results 41 to 50 of about 20,122 (200)
Accretion, Outflows, and Winds of Magnetized Stars
Many types of stars have strong magnetic fields that can dynamically influence the flow of circumstellar matter. In stars with accretion disks, the stellar magnetic field can truncate the inner disk and determine the paths that matter can take to flow ...
A. Brandenburg +192 more
core +1 more source
Excitation of Alfvén waves by modulated HF heating of the ionosphere, with application to FAST observations [PDF]
During the operation of the EISCAT high power facility (heater) at Tromsø, Norway, on 8 October 1998, the FAST spacecraft made electric field and particle observations in the inner magnetosphere at 0.39 Earth radii above the heated ionospheric ...
E. Kolesnikova +5 more
doaj +1 more source
Line and continuum radiative transfer modelling of AA Tau [PDF]
We present photometric and spectroscopic models of the Classical T Tauri star AA Tau. Photometric and spectroscopic variability present in observations of AA Tau is attributed to a magnetically induced warp in the accretion disc, periodically occulting ...
Bouvier, J., Esau, C. F., Harries, T. J.
core +4 more sources
We examined rapid variations in the electron zebra stripe patterns, specifically at L = 1.5, over a three‐month duration, using twin Van Allen Probes within Earth's inner magnetosphere. During geomagnetically quiet intervals, these stripes exhibit a peak‐
Megha Pandya +4 more
doaj +1 more source
Electric Current Approach Studying Both Auroral Substorms and Solar Flares Together
Auroral substorms and solar flares are basically various manifestations of electromagnetic energy dissipation processes, so it is useful to consider both phenomena in terms of a chain of processes, consisting of power supply (dynamo), transmission ...
Syun-Ichi Akasofu
doaj +1 more source
Constraining the Origin of Magnetar Flares [PDF]
Sudden relaxation of the magnetic field in the core of a magnetar produces mechanical energy primarily in the form of shear waves which propagate to the surface and enter the magnetosphere as relativistic Alfv\'en waves.
Link, Bennett
core +1 more source
Observational features of charge distribution in Earth’s inner magnetosphere
Understanding the motion of charged particles in the electromagnetic field in the inner magnetosphere is essential for space science and space weather. Charge accumulation can occur due to the dipole magnetic and convective electric fields in this region.
Lai Gao +11 more
doaj +1 more source
Latitudinal dependence of ground VLF transmitter wave power in the inner magnetosphere
In this study, we use approximately 3 years of observations from the Exploration of energization and Radiation in Geospace (ERG/Arase) satellite to statistically study the meridional distribution of wave power from very-low-frequency (VLF) ground ...
Zhiyang Xia +10 more
doaj +1 more source
Anti-particles in the inner magnetosphere: energetic positron population
Se analiza la generación de antipartículas atrapadas en el cinturón interior de la magnetosfera. Dichas partículas podrían tener flujos en exceso de los flujos interestelares generados por rayos cósmicos.
I. M. Martin +3 more
doaj +1 more source
Electron pitch-angle diffusion: resonant scattering by waves vs. nonadiabatic effects [PDF]
In this paper we investigate the electron pitch-angle diffusion coefficients in the night-side inner magnetosphere around the geostationary orbit (L ~ 7) due to magnetic field deformation.
A. V. Artemyev +7 more
doaj +1 more source

