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pro vyhledávání: '"Dhuri, Dattaraj B."'
Proton auroras are widely observed on the dayside of Mars, identified as a significant intensity enhancement in the hydrogen Lyman alpha (121.6 nm) emission between 110 - 150 km altitudes. Solar wind protons penetrating as energetic neutral atoms int
Externí odkaz:
http://arxiv.org/abs/2309.08195
For the past several decades, numerous attempts have been made to model the climate of Mars with extensive studies focusing on the planet's dynamics and the understanding of its climate. While physical modeling and data assimilation approaches have m
Externí odkaz:
http://arxiv.org/abs/2309.01424
Auroras are emissions in a planetary atmosphere caused by its interactions with the surrounding plasma environment. They have been observed in most planets and some moons of the solar system. Since their first discovery in 2005, Mars auroras have bee
Externí odkaz:
http://arxiv.org/abs/2209.15229
Solar magnetic activity produces extreme solar flares and coronal mass ejections, which pose grave threats to electronic infrastructure and can significantly disrupt economic activity. It is therefore important to appreciate the triggers of explosive
Externí odkaz:
http://arxiv.org/abs/2209.09944
For the first time, the Emirates Mars Infrared Spectrometer (EMIRS) instrument on board the Emirates Mars Mission (EMM) "Hope", is providing us with the temperature measurements of Mars at all local times covering most of the planet. As a result, it
Externí odkaz:
http://arxiv.org/abs/2204.12850
Magnetic flux generated within the solar interior emerges to the surface, forming active regions (ARs) and sunspots. Flux emergence may trigger explosive events, such as flares and coronal mass ejections and therefore understanding emergence is usefu
Externí odkaz:
http://arxiv.org/abs/2009.06287
Solar flares are explosions in the solar atmosphere that release intense bursts of short-wavelength radiation and are capable of producing severe space-weather consequences. Flares release free energy built up in coronal fields, which are rooted in a
Externí odkaz:
http://arxiv.org/abs/2005.13333
Publikováno v:
Published in Proceedings of the National Academy of Sciences of the United States of America (PNAS) May, 2019
Solar flares - bursts of high-energy radiation responsible for severe space-weather effects - are a consequence of the occasional destabilization of magnetic fields rooted in active regions (ARs). The complexity of AR evolution is a barrier to a comp
Externí odkaz:
http://arxiv.org/abs/1905.10167
We analyse a linear lattice Boltzmann (LB) formulation for simulation of linear acoustic wave propagation in heterogeneous media. We employ the single-relaxation-time Bhatnagar-Gross-Krook (BGK) as well as the general multi-relaxation-time (MRT) coll
Externí odkaz:
http://arxiv.org/abs/1704.03172
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