Zobrazeno 1 - 10
of 50
pro vyhledávání: '"Horaites, Konstantinos"'
Autor:
Grandin, Maxime, Luttikhuis, Thijs, Battarbee, Markus, Cozzani, Giulia, Zhou, Hongyang, Turc, Lucile, Pfau-Kempf, Yann, George, Harriet, Horaites, Konstantinos, Gordeev, Evgeny, Ganse, Urs, Papadakis, Konstantinos, Alho, Markku, Tesema, Fasil, Suni, Jonas, Dubart, Maxime, Tarvus, Vertti, Palmroth, Minna
The precipitation of charged particles from the magnetosphere into the ionosphere is one of the crucial coupling mechanisms between these two regions of geospace and is associated with multiple space weather effects, such as global navigation satelli
Externí odkaz:
http://arxiv.org/abs/2301.06578
We provide evidence that the sunward-propagating half of the solar wind electron halo distribution evolves without scattering in the inner heliosphere. We assume the particles conserve their total energy and magnetic moment, and perform a "Liouville
Externí odkaz:
http://arxiv.org/abs/2204.06532
We develop a kinetic theory for {the electron strahl, a beam of energetic electrons which propagate} from the sun along the Parker-spiral-shaped magnetic field lines. By assuming a Maxwellian electron distribution function in the near-sun region wher
Externí odkaz:
http://arxiv.org/abs/1908.01902
We propose a kinetic model describing the formation of the strahl and halo electron populations in the solar wind. We demonstrate that the suprathermal electrons propagating from the sun along the Parker-spiral magnetic field lines are progressively
Externí odkaz:
http://arxiv.org/abs/1811.01098
In this work, we analyze the kinetic stability of a solar wind electron distribution composed of core and strahl subpopulations. The core is modeled by a drifting Maxwellian distribution, while the strahl is modeled by an analytic function recently d
Externí odkaz:
http://arxiv.org/abs/1805.04603
Autor:
Horaites, Konstantinos, Boldyrev, Stanislav, Wilson III, Lynn B., Viñas, Adolfo F., Merka, Jan
We develop a model for the strahl population in the solar wind -- a narrow, low-density and high-energy electron beam centered on the magnetic field direction. Our model is based on the solution of the electron drift-kinetic equation at heliospheric
Externí odkaz:
http://arxiv.org/abs/1706.03464
Autor:
Ganse, Urs, Pfau-Kempf, Yann, Zhou, Hongyang, Juusola, Liisa, Workayehu, Abiyot, Kebede, Fasil, Papadakis, Konstantinos, Grandin, Maxime, Alho, Markku, Battarbee, Markus, Dubart, Maxime, Kotipalo, Leo, Lalagüe, Arnaud, Suni, Jonas, Horaites, Konstantinos, Palmroth, Minna
Publikováno v:
Geoscientific Model Development Discussions; 7/4/2024, p1-28, 28p
Autor:
Grandin Maxime, Luttikhuis Thijs, Battarbee Markus, Cozzani Giulia, Zhou Hongyang, Turc Lucile, Pfau-Kempf Yann, George Harriet, Horaites Konstantinos, Gordeev Evgeny, Ganse Urs, Papadakis Konstantinos, Alho Markku, Tesema Fasil, Suni Jonas, Dubart Maxime, Tarvus Vertti, Palmroth Minna
Publikováno v:
Journal of Space Weather and Space Climate, Vol 13, p 20 (2023)
The precipitation of charged particles from the magnetosphere into the ionosphere is one of the crucial coupling mechanisms between these two regions of geospace and is associated with multiple space weather effects, such as global navigation satelli
Externí odkaz:
https://doaj.org/article/ceff223109f241299e7c6b8cfac42cfc
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Akademický článek
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