Zobrazeno 1 - 10
of 794
pro vyhledávání: '"O. Vainio"'
Publikováno v:
Veterinary and Animal Science, Vol 7, Iss , Pp - (2019)
Palatable oral pharmaceuticals are crucial for feline medication. The pharmaceutical industry prefers synthetic flavours over organic ones because of hygiene and regulatory issues. The aim of this study was to find a palatable synthetic flavour for f
Externí odkaz:
https://doaj.org/article/ddeee597400f4d05aeb78b0d982426bc
Publikováno v:
Animal, Vol 8, Iss 3, Pp 347-353 (2014)
Crib-biting in horses is a stereotypic oral behaviour. Genetic susceptibility has been suggested on a causal basis, together with environmental factors such as stress, gastric discomfort and frustration caused by stall restrictions. This study aimed
Externí odkaz:
https://doaj.org/article/fd3f1e8f6cea42d98e1c3b118d902d2f
Publikováno v:
Annals of Global Health, Vol 81, Iss 1 (2015)
Externí odkaz:
https://doaj.org/article/a6ba235d89234a7589515cc020851532
Publikováno v:
Annals of Global Health, Vol 80, Iss 3 (2014)
Externí odkaz:
https://doaj.org/article/8175eb4da7294261955b662fa8c26cd3
Publikováno v:
Clinical and Developmental Immunology, Vol 7, Iss 2-4, Pp 267-277 (2000)
Externí odkaz:
https://doaj.org/article/ac17720530814f99b53dc079de8f9636
Autor:
L Lehtonen, O Vainio, J Ahokas, J Järvinen, S Novotny, S Sheludyakov, K-A Suominen, S Vasiliev, V V Khmelenko, D M Lee
Publikováno v:
New Journal of Physics, Vol 20, Iss 5, p 055010 (2018)
We present an experimental study of electron spin waves in atomic hydrogen gas compressed to high densities of ∼5 × 10 ^18 cm ^−3 at temperatures ranging from 0.26 to 0.6 K in the strong magnetic field of 4.6 T. Hydrogen gas is in a quantum regi
Externí odkaz:
https://doaj.org/article/9c9a030365f843098ae7022bb56c29bc
Akademický článek
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Autor:
Vincent Evans, Daniel Heyner, Javier Rodriguez-Pacheco, Nina Dresing, Benoit Lavraud, Bob Wimmer, Raul Gomez-Herrero, George C. Ho, Virginia Angeli, Emma E. Davies, Timothy S. Horbury, R. J. Forsyth, Emilia Kilpua, Helen O'Brien, Simon Good, R. O. Vainio
Acceleration of energetic particles is a fundamental and ubiquitous mechanism in space and astrophysical plasmas. One of the open questions is the role of the sheath region behind the shock in the acceleration process. We analyze observations by Sola
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7ddeec4ce2431ad4d38e9b2aa608afd4
https://doi.org/10.5194/egusphere-egu21-9288
https://doi.org/10.5194/egusphere-egu21-9288
Autor:
Simon Good, Helen O'Brien, Daniel Price, R. Gomez Herrero, Diana E. Morosan, Emilia Kilpua, Javier Rodriguez-Pacheco, D. Heyener, Jan Gieseler, R. J. Forsyth, Timothy S. Horbury, Emma E. Davies, Robert F. Wimmer-Schweingruber, Vincent Evans, Benoit Lavraud, Nina Dresing, J. Pomoell, George C. Ho, Eleanna Asvestari, V. Angelini, R. O. Vainio
Publikováno v:
Astronomy & Astrophysics. 656:A8
Sheaths ahead of coronal mass ejections (CMEs) are large heliospheric structures that form with CME expansion and propagation. Turbulent and compressed sheaths contribute to the acceleration of particles in the corona and in interplanetary space, but
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dbbd0477fc8b54def9e5313524dbd91e
https://doi.org/10.1051/0004-6361/202140838
https://doi.org/10.1051/0004-6361/202140838
Akademický článek
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