Zobrazeno 1 - 10
of 91
pro vyhledávání: '"S. Pilo"'
Publikováno v:
Earth and Space Science, Vol 9, Iss 7, Pp n/a-n/a (2022)
Abstract Since the Argo program began, 568 floats returned almost 31,000 profiles, at high‐southern latitudes, with no measured position. These data are either disseminated with positions linearly interpolated between known positions, or with no ge
Externí odkaz:
https://doaj.org/article/8f1443f335924e8899229011a9fc74ac
Publikováno v:
Frontiers in Marine Science, Vol 7 (2021)
Marine heatwaves (MHWs) are prolonged extreme oceanic warm water events. Globally, the frequency and intensity of MHWs have been increasing in recent years, and it is expected that this trend is reflected in the Kerguelen Plateau region. MHWs can neg
Externí odkaz:
https://doaj.org/article/123844aafd2b49338a8767a2d125167e
Publikováno v:
Journal of Geophysical Research: Oceans. 127
Publikováno v:
Geophysical Research Letters. 49
Publikováno v:
Geophysical Research Letters. 46:14604-14612
Sustained extreme temperature events in the ocean, referred to as marine heatwaves (MHWs), generate substantial ecological, social, and economic impacts. Ocean models provide insights to the drivers, persistence, and dissipation of MHWs. However, the
Marine heatwave (MHW) characteristics - such as frequency, intensity and duration - are increasing, largely due to global warming. However, while corresponding marine cold spell (MCS) characteristi...
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::879e3dbd65b5572d124dd22c0a215156
https://doi.org/10.1002/essoar.10508759.1
https://doi.org/10.1002/essoar.10508759.1
Publikováno v:
Ocean Modelling. 131:71-85
It is expected that the assimilation of data in an ocean model disrupts the model’s dynamical balance. This disruption occurs because the analysis fields are not a precise solution to the equations of the model. Therefore, the model adjusts to the
Publikováno v:
Frontiers in Marine Science, Vol 7 (2021)
Marine heatwaves (MHWs) are prolonged extreme oceanic warm water events. Globally, the frequency and intensity of MHWs have been increasing in recent years, and it is expected that this trend is reflected in the Kerguelen Plateau region. MHWs can neg
Autor:
A. E. Kiss, A. McC. Hogg, N. Hannah, F. Boeira Dias, G. B. Brassington, M. A. Chamberlain, C. Chapman, P. Dobrohotoff, C. M. Domingues, E. R. Duran, M. H. England, R. Fiedler, S. M. Griffies, A. Heerdegen, P. Heil, R. M. Holmes, A. Klocker, S. J. Marsland, A. K. Morrison, J. Munroe, M. Nikurashin, P. R. Oke, G. S. Pilo, O. Richet, A. Savita, P. Spence, K. D. Stewart, M. L. Ward, F. Wu, X. Zhang
Publikováno v:
Geoscientific Model Development, Vol 13, Pp 401-442 (2020)
We introduce ACCESS-OM2, a new version of the ocean–sea ice model of the Australian Community Climate and Earth System Simulator. ACCESS-OM2 is driven by a prescribed atmosphere (JRA55-do) but has been designed to form the ocean–sea ice component
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2c9bcd9980f45bc95c1e9d50b7cb9cc3
https://www.geosci-model-dev.net/13/401/2020/
https://www.geosci-model-dev.net/13/401/2020/
Autor:
Stein Vidar Hagfors Haugan, S. Paltani, S. de la Torre, W. A. Holmes, Javier Graciá-Carpio, Ghassem Gozaliasl, Remi A. Cabanac, S. Niemi, Ibrahim Almosallam, S. Galeotta, X. Dupac, Natalia Auricchio, Lauro Moscardini, Carlo Giocoli, Giuseppe Longo, Valeria Pettorino, Carmelita Carbone, E. Zucca, Luigi Guzzo, C. Bodendorf, Enzo Branchini, A. Secroun, N. Martinet, H. Degaudenzi, M. Kilbinger, F. Raison, M. Kuemmel, Roberto P. Saglia, Stefano Cavuoti, Audrey Galametz, B. Gillis, Fabio Finelli, N. Mauri, Massimo Meneghetti, S. Kermiche, M. H. Fabricius, Ismael Tereno, D. Stern, Frank Grupp, P. B. Lilje, Pablo Fosalba, V. Scottez, Andy Taylor, A. Cappi, W. G. Hartley, Giulio Fabbian, E. Keihänen, V. Capobianco, C. C. Kirkpatrick, L. Patrizii, Martin Kunz, Doug Potter, Andrea Tramacere, P. Tallada Crespí, M. Poncet, A. Alvarez-Ayllon, Sandrine Pires, Andrea Biviano, S. Serrano, C. Colodro-Conde, Chiara Sirignano, Joshua S. Speagle, K. Markovic, Yu Wang, Marco Castellano, Andrea Zacchei, Gianluca Castignani, G. Congedo, Emiliano Merlin, G. Desprez, G. Zamorani, F. Sureau, Sebastiano Ligori, Domenico Sapone, I. Lloro, A. Renzi, S. Bardelli, O. Ilbert, Stefano Andreon, A. Da Silva, M. Tenti, Michele Moresco, V. Amaro, Davide Maino, R. Saha, Felix Hormuth, A. Ealet, P. W. Hatfield, Ole Marggraf, G. Polenta, A. Balaguera-Antolinez, S. Farrens, M. Frailis, Carlo Baccigalupi, R. Benton Metcalf, Simona Mei, Sotiria Fotopoulou, Andrew Humphrey, Mark Brodwin, Federico Marulli, M. Fumana, E. Medinaceli, Rafael Toledo-Moreo, Ralf Bender, Pedro G. Ferreira, Emanuel Rossetti, Jarle Brinchmann, G. Meylan, Hannu Kurki-Suonio, C. Padilla, Leonardo Corcione, M. Hailey, Jason Rhodes, Jean-Gabriel Cuby, N. Welikala, L. Conversi, J. De Vicente-Albendea, Thomas D. Kitching, Peter Schneider, Andrea Cimatti, Luca Valenziano, Hélène M. Courtois, Matt J. Jarvis, D. Tavagnacco, Julien Zoubian, T. Vassallo, N. Fourmanoit, S. Pilo, Joseph J. Mohr, Enrico Bozzo, F. Dubath, F. J. Castander, D. Bonino, Marian Douspis, Carlo Burigana, L. Stanco, Elisabetta Maiorano, E. Munari, C. S. Carvalho, G. Sirri, L. Whittaker, Stefano Camera, Matteo Viel, L. Popa, R. Cledassou, Matteo Maturi, Ricard Casas, Fabio Pasian, Jussi-Pekka Väliviita, Jean Coupon, Marco Baldi, F. Torradeflot, Y. Copin, Massimo Brescia, D. Di Ferdinando, C. A. J. Duncan, Mara Salvato, C. J. Conselice, B. Garilli, Clotilde Laigle, B. Kubik, S. Maurogordato, Richard Massey, Knud Jahnke, M. M. Rau, Giuseppe Riccio, S. Casas, R. Kohley, Lucia Pozzetti, W. Gillard, J. Carretero, E. Franceschi
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 644, pp.A31. ⟨10.1051/0004-6361/202039403⟩
2020, ' Euclid preparation : X. The Euclid photometric-redshift challenge ', Astronomy and Astrophysics, vol. 644, A31, pp. 1-24 . https://doi.org/10.1051/0004-6361/202039403
Astronomy & Astrophysics, 2020, Vol.644, pp.A31 [Peer Reviewed Journal]
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 644, pp.A31. ⟨10.1051/0004-6361/202039403⟩
instname
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 644, pp.A31. ⟨10.1051/0004-6361/202039403⟩
2020, ' Euclid preparation : X. The Euclid photometric-redshift challenge ', Astronomy and Astrophysics, vol. 644, A31, pp. 1-24 . https://doi.org/10.1051/0004-6361/202039403
Astronomy & Astrophysics, 2020, Vol.644, pp.A31 [Peer Reviewed Journal]
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 644, pp.A31. ⟨10.1051/0004-6361/202039403⟩
Forthcoming large photometric surveys for cosmology require precise and accurate photometric redshift (photo-z) measurements for the success of their main science objectives. However, to date, no method has been able to produce photo-zs at the requir
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8a2971f2b412808332d7d3e934aee402
http://hdl.handle.net/2318/1790147
http://hdl.handle.net/2318/1790147