Zobrazeno 1 - 10
of 19
pro vyhledávání: '"Luca Gallana"'
Publikováno v:
Journal of Turbulence. 15:311-334
The advection of a passive scalar through an initial flat interface separating two different isotropic decaying turbulent fields is investigated in two and three dimensions. Simulations have been performed for a range of Taylor’s microscale Reynold
Publikováno v:
Politecnico di Torino-IRIS
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::c5e5f792249d90f147298235a91ec6fe
http://hdl.handle.net/11583/2681657
http://hdl.handle.net/11583/2681657
Autor:
Michele Iovieno, John D. Richardson, Sophie M. Fosson, Luca Gallana, Enrico Magli, M. Opher, Federico Fraternale, Daniela Tordella
The Voyager probes are the furthest, still active, spacecraft ever launched from Earth. During their 38-year trip, they have collected data regarding solar wind properties (such as the plasma velocity and magnetic field intensity). Unfortunately, a c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a3d1d42e9fcf70ed258c3e3f474ef493
http://arxiv.org/abs/1510.04304
http://arxiv.org/abs/1510.04304
We consider a simplified physics of the could interface where condensation, evaporation and radiation are neglected and momentum, thermal energy and water vapor transport is represented in terms of the Boussinesq model coupled to a passive scalar tra
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::13f2bfaa3033e0416ef2c8173b6ac61b
http://arxiv.org/abs/1502.06918
http://arxiv.org/abs/1502.06918
Publikováno v:
Politecnico di Torino-IRIS
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::82af74e1b91e930f28d30f45cfd21165
http://hdl.handle.net/11583/2630416
http://hdl.handle.net/11583/2630416
Autor:
Luca Gallana, Daniela Tordella, John D. Richardson, Michele Iovieno, Federico Fraternale, Merav Opher
Plasma velocity and magnetic field measurements from the Voyager 2 mission are used to study solar wind turbulence in the slow solar wind at two different heliocentric distances, 5 and 29 astronomical units, sufficiently far apart to provide informat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2c99ce3757eee2ea20f1bf0e7276cb21
Autor:
Richardson, J. D., Belcher, J., Daniela Tordella, Federico Fraternale, Luca Gallana, Michele Iovieno
Publikováno v:
Politecnico di Torino-IRIS
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::4da6b4a4d0ca37d14ba1f7f49eb84d15
http://hdl.handle.net/11583/2630573
http://hdl.handle.net/11583/2630573
Autor:
Luca Gallana, M. Opher, John D. Richardson, Federico Fraternale, Daniela Tordella, Michele Iovieno
Fluctuations in the flow velocity and magnetic fields are ubiquitous in the Solar System. These fluctuations are turbulent, in the sense that they are disordered and span a broad range of scales in both space and time. The study of solar wind turbule
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c601e4f40def408fc0e7265898ef8e67
Autor:
Luca Gallana, Santi, Francesca, Di Savino, Silvio, Michele Iovieno, Richiardone, R., Daniela Tordella
Publikováno v:
Politecnico di Torino-IRIS
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::7ad3416a32d6e0093e6052f72f0f7388
http://hdl.handle.net/11583/2562539
http://hdl.handle.net/11583/2562539
Publikováno v:
Politecnico di Torino-IRIS
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::58952d27ca5596704900f04f5ab22825
http://hdl.handle.net/11583/2562543
http://hdl.handle.net/11583/2562543