Zobrazeno 1 - 10
of 995
pro vyhledávání: '"M MICELI"'
Autor:
Teddi Herring, Antoni G. Lewkowicz, Alexandre Chiasson, Yifeng Wang, Robert G. Way, Joseph M. Young, Duane Froese, Sharon L. Smith, Brielle Andersen, Olivier Bellehumeur-Génier, Alexandre R. Bevington, Philip P. Bonnaventure, Maxime A. Duguay, Bernd Etzelmüller, Michael N. Gooseff, Sarah E. Godsey, Christina M. Miceli
Publikováno v:
Arctic Science (2024)
Permafrost landscapes are becoming increasingly susceptible to widespread thaw due to climate change. Collating historical and ongoing data are critical for assessing permafrost conditions and spatiotemporal changes. Electrical resistivity tomography
Externí odkaz:
https://doaj.org/article/3a63ff9ca64a489da47699485f23df4e
Autor:
I. C. Jebaraj, O. V. Agapitov, M. Gedalin, L. Vuorinen, M. Miceli, C. M. S. Cohen, A. Voshchepynets, A. Kouloumvakos, N. Dresing, A. Marmyleva, V. Krasnoselskikh, M. Balikhin, J. G. Mitchell, A. W. Labrador, N. Wijsen, E. Palmerio, L. Colomban, J. Pomoell, E. K. J. Kilpua, M. Pulupa, F. S. Mozer, N. E. Raouafi, D. J. McComas, S. D. Bale, R. Vainio
Publikováno v:
The Astrophysical Journal Letters, Vol 976, Iss 1, p L7 (2024)
In this study, we present the first-ever direct measurements of synchrotron-emitting heliospheric traveling shocks, intercepted by the Parker Solar Probe (PSP) during its close encounters. Given that much of our understanding of powerful astrophysica
Externí odkaz:
https://doaj.org/article/44b29211b9c6440c879dff30044199f8
Autor:
W. Yao, A. Fazzini, S. N. Chen, K. Burdonov, P. Antici, J. Béard, S. Bolaños, A. Ciardi, R. Diab, E. D. Filippov, S. Kisyov, V. Lelasseux, M. Miceli, Q. Moreno, V. Nastasa, S. Orlando, S. Pikuz, D. C. Popescu, G. Revet, X. Ribeyre, E. d’Humières, J. Fuchs
Publikováno v:
Matter and Radiation at Extremes, Vol 7, Iss 1, Pp 014402-014402-14 (2022)
Collisionless shocks are ubiquitous in the Universe and are held responsible for the production of nonthermal particles and high-energy radiation. In the absence of particle collisions in the system, theory shows that the interaction of an expanding
Externí odkaz:
https://doaj.org/article/d3ab1b77b1d7463aaa6c05fe19ba19a7
Autor:
W. Yao, A. Fazzini, S.N. Chen, K. Burdonov, J. Béard, M. Borghesi, A. Ciardi, M. Miceli, S. Orlando, X. Ribeyre, E. d'Humières, J. Fuchs
Publikováno v:
J.Plasma Phys.
J.Plasma Phys., 2023, 89 (1), pp.915890101. ⟨10.1017/S002237782300003X⟩
J.Plasma Phys., 2023, 89 (1), pp.915890101. ⟨10.1017/S002237782300003X⟩
Colliding collisionless shocks appear in a great variety of astrophysical phenomena and are thought to be possible sources of particle acceleration in the Universe. We have previously investigated particle acceleration induced by single super-critica
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b0091ec0086590ba64bbedaa472c7595
https://hdl.handle.net/10447/587434
https://hdl.handle.net/10447/587434
Autor:
O Petruk, V Beshley, S Orlando, F Bocchino, M Miceli, S Nagataki, M Ono, S Loru, A Pellizzoni, E Egron
The detected polarized radio emission from remnant of SN1987A opens the possibility to unveil the structure of the pre-supernova magnetic field in the circumstellar medium. Properties derived from direct measurements would be of importance for unders
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3ded1c34964c449e9655c527d52f270e
https://hdl.handle.net/10447/588814
https://hdl.handle.net/10447/588814
Publikováno v:
Journal of Gynecologic Surgery. 38:287-293
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 515:1676-1689
We present the results of a cluster search in the gamma-ray sky images of the Large Magellanic Cloud (LMC) region by means of the Minimum Spanning Tree (MST) and DBSCAN algorithms, at energies higher than 6 and 10 GeV, using 12 years of Fermi-LAT dat
Autor:
S. Orlando, A. Wongwathanarat, H.-T. Janka, M. Miceli, S. Nagataki, M. Ono, F. Bocchino, J. Vink, D. Milisavljevic, D. J. Patnaude, G. Peres
Publikováno v:
Astronomy and Astrophysics, 666:A2. EDP Sciences
Observations of the SNR Cassiopeia A (Cas A) show asymmetries in the reverse shock that cannot be explained by models describing a remnant expanding through a spherically symmetric wind of the progenitor star. We investigate whether a past interactio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a6b943e2e3ce693212f3d82c26d0f0fc
https://hdl.handle.net/10447/573826
https://hdl.handle.net/10447/573826
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