Zobrazeno 1 - 10
of 18
pro vyhledávání: '"Yana Maneva"'
Autor:
Kirsti Kauristie, Jesse Andries, Peter Beck, Jens Berdermann, David Berghmans, Claudio Cesaroni, Erwin De Donder, Judith de Patoul, Mark Dierckxsens, Eelco Doornbos, Mark Gibbs, Krista Hammond, Haris Haralambous, Ari-Matti Harri, Edmund Henley, Martin Kriegel, Tiera Laitinen, Marcin Latocha, Yana Maneva, Loredana Perrone, Emanuele Pica, Luciano Rodriguez, Vincenzo Romano, Dario Sabbagh, Luca Spogli, Iwona Stanislawska, Lukasz Tomasik, Mpho Tshisaphungo, Kasper van Dam, Bert van den Oord, Petra Vanlommel, Tobias Verhulst, Volker Wilken, Andriy Zalizovski, Kari Österberg
Publikováno v:
Remote Sensing, Vol 13, Iss 18, p 3685 (2021)
This paper presents a review on the PECASUS service, which provides advisories on enhanced space weather activity for civil aviation. The advisories are tailored according to the Standards and Recommended Practices of the International Civil Aviation
Externí odkaz:
https://doaj.org/article/d32c645642864635bad9a36c962aae73
In this work, we investigate the properties of ion acoustic waves generated by negative heavy ions in a multi-component non-Maxwellian electrostatic plasma, consisting of electrons, positive and negative heavy ions, and a background population of dus
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6977a84adeeb08fee35308fe770f5103
https://lirias.kuleuven.be/handle/123456789/595310
https://lirias.kuleuven.be/handle/123456789/595310
Publikováno v:
Journal of Geophysical Research: Space Physics. 119:4223-4238
Preferential heating and acceleration of the solar wind He++ ions compared to protons in fast solar wind streams have been known for decades, thanks to in situ spacecraft measurements at 0.29-5 AU. Turbulent magnetic field fluctuations with approxima
In order to study chromospheric magnetosonic wave propagation including, for the first time, the effects of ion-neutral interactions in the partially ionized solar chromosphere, we have developed a new multi-fluid computational model, accounting for
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::42ffb8557f9d7a0f0af1152c80cce7a7
http://arxiv.org/abs/1611.08439
http://arxiv.org/abs/1611.08439
Publikováno v:
Journal of Geophysical Research: Space Physics. 118:2842-2853
[1] Both remote sensing and in situ measurements show that the fast solar wind plasma significantly deviates from thermal equilibrium and is strongly permeated by turbulent electromagnetic waves, which regulate the ion temperature anisotropies and re
Publikováno v:
47th AIAA Plasmadynamics and Lasers Conference.
Publikováno v:
AIP Conference Proceedings.
We compare the results from 1.5D and 2.5D hybrid simulations (with fluid electrons, and kinetic/particle-in-cell protons and α particles) to investigate the effect of the solar wind expansion on the evolution of ion relative drifts in collisionless
Publikováno v:
AIP Conference Proceedings.
Minor ions in the fast solar wind are known to have higher temperatures and to flow faster than protons in the interplanetary space. In this study we combine previous research on parametric instability theory and 2.5D hybrid simulations to study the
Autor:
Stefaan Poedts, Yana Maneva
Publikováno v:
Astronomy & Astrophysics. 613:A10
© ESO 2018. The power spectra of magnetic field fluctuations in the solar wind typically follow a power-law dependence with respect to the observed frequencies and wave-numbers. The background magnetic field often influences the plasma properties, s
Publikováno v:
The European Physical Journal D. 44:533-536
Absorbtion of Alfven waves is considered to be the main mechanism of heating in the solar corona. It is concluded that the sharp increase of the plasma temperature by two orders of magnitude is related to a self-induced opacity with respect to Alfven