Zobrazeno 1 - 10
of 2 336
pro vyhledávání: '"Froment, P"'
Autor:
Nóbrega-Siverio, D., Cabello, I., Bose, S., van der Voort, L. H. M. Rouppe, Joshi, R., Froment, C., Henriques, V. M. J.
Publikováno v:
A&A 686, A218 (2024)
Advancements in instrumentation have revealed a multitude of small-scale EUV events in the solar atmosphere. Our aim is to employ high-resolution magnetograms to gain a detailed understanding of the magnetic origin of such phenomena. We have used coo
Externí odkaz:
http://arxiv.org/abs/2403.11652
Autor:
Vazia, Corentin, Bousse, Alexandre, Froment, Jacques, Vedel, Béatrice, Vermet, Franck, Wang, Zhihan, Dassow, Thore, Tasu, Jean-Pierre, Visvikis, Dimitris
This paper proposes a novel approach to spectral computed tomography (CT) material decomposition that uses the recent advances in generative diffusion models (DMs) for inverse problems. Spectral CT and more particularly photon-counting CT (PCCT) can
Externí odkaz:
http://arxiv.org/abs/2403.10183
Autor:
Vazia, Corentin, Bousse, Alexandre, Vedel, Béatrice, Vermet, Franck, Wang, Zhihan, Dassow, Thore, Tasu, Jean-Pierre, Visvikis, Dimitris, Froment, Jacques
Using recent advances in generative artificial intelligence (AI) brought by diffusion models, this paper introduces a new synergistic method for spectral computed tomography (CT) reconstruction. Diffusion models define a neural network to approximate
Externí odkaz:
http://arxiv.org/abs/2403.06308
Autor:
Colomban, L., Kretzschmar, M., Krasnoselkikh, V., Agapitov, O. V., Froment, C., Maksimovic, M., Berthomier, M., Khotyainsev, Yu. V., Graham, D. B., Bale, S.
The evolution of the solar wind electron distribution function with heliocentric distance exhibits different features that are still unexplained, in particular, the increase of the Strahl pitch angle width. Wave-particle interactions between electron
Externí odkaz:
http://arxiv.org/abs/2402.06016
Autor:
Wang, Zhihan, Bousse, Alexandre, Vermet, Franck, Froment, Jacques, Vedel, Béatrice, Perelli, Alessandro, Tasu, Jean-Pierre, Visvikis, Dimitris
Spectral computed tomography (CT) offers the possibility to reconstruct attenuation images at different energy levels, which can be then used for material decomposition. However, traditional methods reconstruct each energy bin individually and are vu
Externí odkaz:
http://arxiv.org/abs/2311.00666
Autor:
Bizien, Nina, de Wit, Thierry Dudok, Froment, Clara, Velli, Marco, Case, Anthony W., Bale, Stuart D., Kasper, Justin, Whittlesey, Phyllis, MacDowall, Robert, Larson, Davin
Publikováno v:
ApJ 958 23 (2023)
Switchbacks are sudden and large deflections in the magnetic field that Parker Solar Probe frequently observes in the inner heliosphere. Their ubiquitous occurrence has prompted numerous studies to determine their nature and origin. Our goal is to de
Externí odkaz:
http://arxiv.org/abs/2310.12134
Autor:
Krasnoselskikh, Vladimir, Zaslavsky, Arnaud, Artemyev, Anton, Froment, Clara, de Wit, Thierry Dudok, Raouafi, Nour E., Agapitov, Oleksiy V., Bale, Stuart D., Verniero, Jaye L.
The exploration of the inner heliosphere by Parker Solar Probe has revealed a highly structured solar wind with ubiquitous deflections from the Parker spiral, known as switchbacks. Interchange reconnection (IR) may play an important role in generatin
Externí odkaz:
http://arxiv.org/abs/2310.12093
The solar corona produces coronal rain, hundreds of times colder and denser material than the surroundings. Coronal rain is known to be deeply linked to coronal heating, but its origin, dynamics, and morphology are still not well understood. The lead
Externí odkaz:
http://arxiv.org/abs/2305.08775
Autor:
Karbashewski, S., Agapitov, O. V., Kim, H. Y., Mozer, F. S., Bonnell, J. W., Froment, C., de Wit, T. Dudok, Bale, S. D., Malaspina, D., Raouafi, N. E.
Observations of the young solar wind by the Parker Solar Probe (PSP) mission reveal the existence of intense plasma wave bursts with frequencies between $0.05$ -- $0.20 f_\mathrm{ce}$ (tens of Hz up to ${\sim}300$ Hz) in the spacecraft frame. The wav
Externí odkaz:
http://arxiv.org/abs/2304.01185
Autor:
Froment, C., Agapitov, O. V., Krasnoselskikh, V., Karbashewski, S., de Wit, T. Dudok, Larosa, A., Colomban, L., Malaspina, D., Kretzschmar, M., Jagarlamudi, V. K., Bale, S. D., Bonnell, J. W., Mozer, F. S., Pulupa, M.
Publikováno v:
A&A 672, A135 (2023)
Context. Whistler waves are electromagnetic waves produced by electron-driven instabilities, that in turn can reshape the electron distributions via wave-particle interactions. In the solar wind, they are one of the main candidates for explaining the
Externí odkaz:
http://arxiv.org/abs/2302.01245