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Canada-AB-CZAR Azienda Directories
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Azienda News:
- [2412. 04219] Ionospheric conductances at the giant planets of the Solar . . .
We perform a comparative study of Hall and Pedersen conductivities and conductances in the four giant planets of our Solar System - Jupiter, Saturn, Uranus and Neptune
- FG: Comparative Planetary Magnetospheric Processes - gem
Studying all the processes is an overwhelming and unrealistic task, so we propose the following key comparative topics that directly relate to the active GEM focus groups: 1) comparative magnetotail dynamics and their effects on the transport of mass, momentum, energy, and magnetic flux; 2) comparative planetary radiation belts and ring
- Comparative Planetary Magnetospheric Processes
Earth’s magnetosphere experiences varying solar wind input, but other parameters, which are important for understand magnetospheres, such as plasma sources, rotation rate, magnetic field magnitude, size of magnetosphere change only very little or not at all
- Solar and Space Physics: A Science for a Technological Society
Identifying the factors that control solar wind and ionospheric contributions to magnetospheric populations is fundamental to determining the dynamics of the magnetosphere, ionosphere, and atmosphere, their coupling, and the response to solar wind variability
- Current Systems in Planetary Magnetospheres and Ionospheres
The interaction of planets with the solar wind produces a diversity of current systems, yet these can be classified into only a few different types, which include ionospheric currents, currents carried by magnetospheric boundaries like the magnetopause or ionopause, magnetotail currents, and currents flowing inside the magnetospheres, like ring
- PLANETARY MAGNETOSPHERES A COMPARATIVE VIEW - NASA Technical Reports . . .
some interesting differences in magnetospheric dynamics as compared to the Earth When magnetic merging between the interplanetary field and a planetary magnetic field is a factor,, the size of the front portion of the magnetosphere can be significantly affected
- GIANT PLANET IONOSPHERES AND THERMOSPHERES: THE IMPORTANCE OF ION . . .
All of the Solar System’s giant planets have magnetic fields of various strengths, and in-teractions with their space environments are thus mediated by their respective magnetospheres This article concentrates on the consequences of magnetosphere-atmosphere interactions for the physical conditions of the thermosphere and ionosphere
- Comparative Study on Planetary Magnetosphere in the Solar System - MDPI
The magnetospheric responses to solar wind of Mercury, Earth, Jupiter and Uranus are compared via magnetohydrodynamic (MHD) simulations The tilt angle of each planetary field and the polarity of solar wind are also considered
- Dynamics of the Magnetosphere and its Coupling to the Ionosphere on . . .
Topics include solar-terrestrial interactions, magnetospheric physics, and magnetosphere-ionosphere coupling Presentations will mainly be from the four-satellite Interball system, including joint studies with the US and Japanese ISTP satellites 14 SUBJECT TERMS 15 NUMBER OF PAGES 16 PRICE CODE N A 17 SECURITY CLASSIFICATION 18
- Frontiers | Simulating the Responses of the Magnetosphere–Ionosphere . . .
We investigate in detail the transitional change of the y-component of the geomagnetic field and compare it to the scenario under southward IMF conditions, and find that the latter case reacts in a much simpler manner and the responses are faster globally
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