Zobrazeno 1 - 10
of 91
pro vyhledávání: '"J. L. Sans"'
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Publikováno v:
Materials & Design, Vol 83, Iss, Pp 85-94 (2015)
Materials and Design
Materials and Design, Elsevier, 2015, 83, pp.85-94. ⟨10.1016/j.matdes.2015.05.073⟩
Materials and Design
Materials and Design, Elsevier, 2015, 83, pp.85-94. ⟨10.1016/j.matdes.2015.05.073⟩
Three metallic coatings with textured surfaces, made of rhenium, tungsten and molybdenum, were studied in the frame of the Solar Probe Plus mission (NASA) as candidate materials. The role of these coatings is to dissipate a maximum of energy from a h
Publikováno v:
Corrosion science 126 (2017): 255–264. doi:10.1016/j.corsci.2017.07.007
info:cnr-pdr/source/autori:L. Charpentier, M. Balat-Pichelin, J-L. Sans, D. Sciti, L. Silvestroni/titolo:Effect of high temperature on the optical properties of HfC-based ceramics/doi:10.1016%2Fj.corsci.2017.07.007/rivista:Corrosion science/anno:2017/pagina_da:255/pagina_a:264/intervallo_pagine:255–264/volume:126
info:cnr-pdr/source/autori:L. Charpentier, M. Balat-Pichelin, J-L. Sans, D. Sciti, L. Silvestroni/titolo:Effect of high temperature on the optical properties of HfC-based ceramics/doi:10.1016%2Fj.corsci.2017.07.007/rivista:Corrosion science/anno:2017/pagina_da:255/pagina_a:264/intervallo_pagine:255–264/volume:126
Hafnium carbide (HfC) is a promising materials for high-temperature heat exchangers due to its high melting point (4170 K). Nevertheless, its fast oxidation into fragile hafnia prevents it from being used for open-air solar receivers. The incorporati
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=cnr_________::382f67a9d9c761bee4a73227b2abab97
Publikováno v:
Acta Materialia
Acta Materialia, Elsevier, 2015, 84, pp.305-316. ⟨10.1016/j.actamat.2014.10.050⟩
Acta Materialia, Elsevier, 2015, 84, pp.305-316. ⟨10.1016/j.actamat.2014.10.050⟩
The Solar Probe Plus mission (NASA) will be the first mission to enter the solar corona. The spacecraft will orbit the Sun at 8.5 solar radii from the Sun’s surface at closest approach. Some metallic parts of the two on-board instruments, SWEAP (a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2f13fd20d4a698f042812d93deab8e5a
https://hal.archives-ouvertes.fr/hal-02327218
https://hal.archives-ouvertes.fr/hal-02327218
Publikováno v:
Carbon
Carbon, Elsevier, 2015, 82, pp.39-50. ⟨10.1016/j.carbon.2014.10.022⟩
Carbon, Elsevier, 2015, 82, pp.39-50. ⟨10.1016/j.carbon.2014.10.022⟩
Two solar missions are designed to plunge into the solar corona, and respectively get as close as 8.5 and 3 Rs (solar radii) from the Sun’s surface. Heat shields will protect the payloads within their umbra from the thermal radiation and solar wind
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::51d26fd8204743ebbe9f788beb0a7e80
https://hal.archives-ouvertes.fr/hal-02327221
https://hal.archives-ouvertes.fr/hal-02327221
Autor:
P. Espigat, J. Collon, G. Villard, R. Morano, Patrick Snabre, A. Perez, E. Durand, C. Gregory, E. Pare, J-F. Olive, N. Briand, A. Cordier, M. Martin, T. Sako, Miroslav Palatka, Pascal Bruel, Petr Schovanek, A. Jouenne, F. Berny, J. Neveu, P. Cornebise, H. Manseri, J. Gilly, P. Manigot, Sebastien Incerti, O. Lodygensky, G. Morineaud, D.A. Smith, J.-L. Sans, B. Lott, M. Cerutti, L. Rob, P. Fleury, J. Québert, M. de Naurois, T. Reposeur, R. Bazer-Bachi, J.M. Noppe, L. Kalt, H. Manitaz, J.-C. Gouillaud, R. Legallou, Miroslav Hrabovsky, B. Balauge, A. Rebii, A. Musquere, Filip Münz, N. Hérault, D. Dumora, H. Bergeret, Ph. Roy, B. Fabre, G. Debiais, P. Eschstruth, J. Holder, J.-P. Dezalay
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 490:71-89
CELESTE is an atmospheric Cherenkov telescope based on the sampling method which makes use of the de-commissioned THEMIS solar electrical plant in the French Pyrenees. A large (2000 m 2 ) mirror surface area from 40 independent heliostats followed by
Publikováno v:
Journal of Alloys and Compounds
Journal of Alloys and Compounds, Elsevier, 2014, 585, pp.510-517. ⟨10.1016/j.jallcom.2013.09.184⟩
Journal of Alloys and Compounds, Elsevier, 2014, 585, pp.510-517. ⟨10.1016/j.jallcom.2013.09.184⟩
International audience; Measurements of the total directional and hemispherical emissivity of tungsten, rhenium and tungsten with 25% rhenium samples of various surface states was carried out in two wavelength ranges, 0.6–2.8 and 0.6–40 μm, from
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5f0ad8cbcb36f6f48cb3dfa6940af2ba
https://hal-univ-perp.archives-ouvertes.fr/hal-01178141
https://hal-univ-perp.archives-ouvertes.fr/hal-01178141
Autor:
J. Ball, M. Vognar, Z. Janout, A. P. Dzyubak, A. B. Lazarev, V.N. Matafonov, Yu. A. Plis, G. Durand, J.-L. Sans, C. Šimane, A. B. Neganov, Alexander Fedorov, Ivan Karnaukhov, J. Cerny, A.I. Kovalev, N. A. Bazhanov, A. A. Lukhanin, F. Lehar, Yu. A. Usov, N. S. Borisov, S. N. Shilov, G. M. Gurevich, I. Wilhelm
Publikováno v:
Czechoslovak Journal of Physics. 50:401-408
Experience with polarized targets and achieving of very low temperatures gave rise to the idea of using a new technique based on dissolving 3He in 4He to create a frozen spin polarized target. The short history of the development of such proton and d
Autor:
V.N. Matafonov, C. E. Allgower, H. M. Spinka, J.-L. Sans, I.L. Pisarev, M. Combet, Z. Janout, R.A. Kunne, Ph. Demierre, A. de Lesquen, G. Durand, D. Grosnick, M. Beddo, J. Bystrický, D. Rapin, J. Ball, D. Lopiano, T.E. Kasprzyk, R. Hess, A. N. Prokofiev, A.A. Popov, A. A. Zhdanov, B. Vuaridel, V. V. Vikhrov, Yu. A. Usov, B.A. Khachaturov, J.M. Fontaine, V.A. Kalinnikov, F. Lehar
Publikováno v:
The European Physical Journal C. 11:51-67
A polarized proton beam extracted from SATURNE II, the Saclay polarized target with $^6$ Li compounds, and a $\mathrm{CH}_2$ target were used to measure elastic and quasi-elastic pp spin-dependent observables in the angular region $60^{\circ} < \thet