Zobrazeno 1 - 10
of 48
pro vyhledávání: '"Federico Fraternale"'
Publikováno v:
The Astrophysical Journal Letters, Vol 974, Iss 1, p L15 (2024)
We introduce the first solar-cycle simulations from our 3D, global MHD-plasma/kinetic-neutrals model, where both hydrogen and helium atoms are treated kinetically, while electrons and helium ions are described as individual fluids. Using Voyager/PWS
Externí odkaz:
https://doaj.org/article/b9dfe603d6ea4f209090261f60ab48b8
Autor:
Federico Fraternale, Lingling Zhao, Nikolai V. Pogorelov, Luca Sorriso-Valvo, Seth Redfield, Ming Zhang, Keyvan Ghanbari, Vladimir Florinski, Thomas Y. Chen
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 9 (2022)
Turbulence is ubiquitous in space plasmas. It is one of the most important subjects in heliospheric physics, as it plays a fundamental role in the solar wind—local interstellar medium interaction and in controlling energetic particle transport and
Externí odkaz:
https://doaj.org/article/fb8acf95b6bb4820857fb123ed281e34
Autor:
Luca Sorriso-Valvo, Gaetano De Vita, Federico Fraternale, Alexandre Gurchumelia, Silvia Perri, Giuseppina Nigro, Filomena Catapano, Alessandro Retinò, Christopher H. K. Chen, Emiliya Yordanova, Oreste Pezzi, Khatuna Chargazia, Oleg Kharshiladze, Diana Kvaratskhelia, Christian L. Vásconez, Raffaele Marino, Olivier Le Contel, Barbara Giles, Thomas E. Moore, Roy B. Torbert, James L. Burch
Publikováno v:
Frontiers in Physics, Vol 7 (2019)
In weakly collisional space plasmas, the turbulent cascade provides most of the energy that is dissipated at small scales by various kinetic processes. Understanding the characteristics of such dissipative mechanisms requires the accurate knowledge o
Externí odkaz:
https://doaj.org/article/d83d1911c46d45a58f98165f261e3f20
In situ and remote observations of the outer regions of the heliosphere and in the local interstellar medium (LISM) by Voyager, New Horizons, and IBEX continue to present new challenging questions, reflecting the complex processes of the solar wind (
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9db127db684ad16e38e383834e8bd3ba
https://doi.org/10.5194/egusphere-egu23-11714
https://doi.org/10.5194/egusphere-egu23-11714
Autor:
Federico Fraternale, Laxman Adhikari, Horst Fichtner, Tae K. Kim, Jens Kleimann, Sean Oughton, Nikolai V. Pogorelov, Vadim Roytershteyn, Charles W. Smith, Arcadi V. Usmanov, Gary P. Zank, Lingling Zhao
The solar wind (SW) and local interstellar medium (LISM) are turbulent media. Their interaction is governed by complex physical processes and creates heliospheric regions with significantly different properties in terms of particle populations, bulk
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8478964405efa5b7b8bdff8f735aaab3
http://arxiv.org/abs/2207.14115
http://arxiv.org/abs/2207.14115
Autor:
Federico Fraternale, Paulina Quijia, C. L. Vásconez, Emiliya Yordanova, Silvia Perri, Raffaele Marino, Luca Sorriso-Valvo, Julia E. Stawarz
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 503 (4), pp.4815-4827. ⟨10.1093/MNRAS/STAB319⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 503 (4), pp.4815-4827. ⟨10.1093/mnras/stab319⟩
Monthly notices of the Royal Astronomical Society (Online) 503 (2021): 4815–4827. doi:10.1093/mnras/stab319
info:cnr-pdr/source/autori:Quijia, P.; Fraternale, F.; Stawarz, J.E.; Vasconez, C.L.; Perri, S.; Marino, R.; Yordanova, E.; Sorriso-Valvo, L./titolo:Comparing turbulence in a Kelvin-Helmholtz instability region across the terrestrial magnetopause/doi:10.1093%2Fmnras%2Fstab319/rivista:Monthly notices of the Royal Astronomical Society (Online)/anno:2021/pagina_da:4815/pagina_a:4827/intervallo_pagine:4815–4827/volume:503
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 503 (4), pp.4815-4827. ⟨10.1093/MNRAS/STAB319⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 503 (4), pp.4815-4827. ⟨10.1093/mnras/stab319⟩
Monthly notices of the Royal Astronomical Society (Online) 503 (2021): 4815–4827. doi:10.1093/mnras/stab319
info:cnr-pdr/source/autori:Quijia, P.; Fraternale, F.; Stawarz, J.E.; Vasconez, C.L.; Perri, S.; Marino, R.; Yordanova, E.; Sorriso-Valvo, L./titolo:Comparing turbulence in a Kelvin-Helmholtz instability region across the terrestrial magnetopause/doi:10.1093%2Fmnras%2Fstab319/rivista:Monthly notices of the Royal Astronomical Society (Online)/anno:2021/pagina_da:4815/pagina_a:4827/intervallo_pagine:4815–4827/volume:503
The properties of turbulence observed within the plasma originating from the magnetosheath and the magnetospheric boundary layer, which have been entrained within vortices driven by the Kelvin–Helmholtz Instability (KHI), are compared. The goal of
Autor:
Jens Kleimann, Konstantinos Dialynas, Federico Fraternale, André Galli, Jacob Heerikhuisen, Vladislav Izmodenov, Marc Kornbleuth, Merav Opher, Nikolai Pogorelov
Publikováno v:
Kleimann, Jens; Dialynas, Konstantinos; Fraternale, Federico; Galli, André; Heerikhuisen, Jacob; Izmodenov, Vladislav; Kornbleuth, Marc; Opher, Merav; Pogorelov, Nikolai (2022). The Structure of the Large-Scale Heliosphere as Seen by Current Models. Space science reviews, 218(4), p. 36. Springer 10.1007/s11214-022-00902-6
This review summarizes the current state of research aiming at a description of the global heliosphere using both analytical and numerical modeling efforts, particularly in view of the overall plasma/neutral flow and magnetic field structure, and its
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fb8e5287698a8eef6f0601ee7eeb3c21
https://boris.unibe.ch/170463/1/Kleimann2022_Article_TheStructureOfTheLarge-ScaleHe.pdf
https://boris.unibe.ch/170463/1/Kleimann2022_Article_TheStructureOfTheLarge-ScaleHe.pdf
Motivated by the recent discovery of a dispersive-to-nondispersive transition for linear waves in shear flows, we accurately explored the wavenumber-Reynolds number parameter map of the plane Poiseuille flow, in the limit of least-damped waves. We ha
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4aa9fd8753ea4a2257972f80ca7b0a5c
http://arxiv.org/abs/2103.04650
http://arxiv.org/abs/2103.04650
Autor:
Federico Fraternale, Daniela Tordella, Mattia Tomatis, Mina Golshan, Marco Vanni, Shahbozbek Abdunabiev
Publikováno v:
International Journal of Multiphase Flow
We use direct numerical simulation to study the temporal evolution of a perturbation localized on the turbulent layer that typically separates a cloud from the surrounding clear air. Across this shearless layer, a turbulent kinetic energy gradient na
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c9858d9ef22da5f4510e7531eca26bd4
http://arxiv.org/abs/2007.06497
http://arxiv.org/abs/2007.06497
Autor:
Shahbozbek Abdunabiev, Mina Golshan, Federico Fraternale, Daniela Tordella, Mattia Tomatis, Marco Vanni
This work focuses on the turbulent shearless mixing structure of a cloud/clear air interface with physical parameters typical of cumulus warm clouds. We investigate the effect of turbulence on the droplet size distribution, in particular, we focus on
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::65e836d0d9b004c75b507387e08fa8b2
https://doi.org/10.5194/egusphere-egu2020-22539
https://doi.org/10.5194/egusphere-egu2020-22539