Zobrazeno 1 - 10
of 44
pro vyhledávání: '"M. Nicot"'
Autor:
M. P. Marani, M. Nicot, H. W. Gerber, G. Clauss, J. Marvaldi, F. Gasparoni, G. DAnna, L. Beranzoli, P. Favali, F. Gamberi
Publikováno v:
Annals of Geophysics, Vol 49, Iss 2-3 (2006)
Seafloor long-term, multiparameter, single-frame observatories have been developed within the framework of European Commission and Italian projects since 1995. A fleet of five seafloor observatories, built-up starting from 1995 within the framework o
Externí odkaz:
https://doaj.org/article/72733211725040b4bdf9bfdf8af2ee51
Autor:
C. Engel, F. Pajot, J. Martignac, F. Bousqet, Y. Lepennec, S. Maestre, Nicolas Bray, Matthew Joseph Griffin, Peter A. R. Ade, A. Hughes, Silvia Masi, J. Narbonne, G. Foënard, René J. Laureijs, Frederi Mirc, Christopher Tibbs, J. M. Nicot, P. deBernardis, Y. André, G. Roudil, L. Rodriguez, Pierre Tapie, L. Bautista, B. Maffei, P. Etcheto, Etienne Perot, Peter Charles Hargrave, J. A. Tauber, J. P. Dubois, S. Grabarnik, B. Mot, M. Bouzit, L. Montier, O. Boulade, C. Marty, E. Doumayrou, Giampaolo Pisano, Isabelle Ristorcelli, H. Roussel, Nicolas Ponthieu, B. Leriche, A. Mangilli, X. Dupac, C. Tucker, Ph. Gelot, Y. Longval, Giorgio Savini, A. Lacourt, J. Aumont, V. Buttice, R. Misawa, M. Charra, Johan Montel, J. Pimentao, Muriel Saccoccio, W. Marty, B. Crane, M. Chaigneau, J.-P. Bernard, G. Parot, S. Stever, Maria Salatino, O. Simonella
Publikováno v:
Experimental Astronomy
Experimental Astronomy, 2019, 48, pp.265-295. ⟨10.1007/s10686-019-09648-6⟩
Experimental Astronomy, 2019, 48, pp.265-295. ⟨10.1007/s10686-019-09648-6⟩
International audience; The Polarized Instrument for Long-wavelength Observation of the Tenuous interstellar medium (PILOT) is a balloon-borne experiment that aims to measure the polarized emission of thermal dust at a wavelength of 240 µm (1.2 THz)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0bf9e552686c12be37cd6a310ff3b79f
http://hdl.handle.net/11573/1417357
http://hdl.handle.net/11573/1417357
Autor:
Nicolas Ponthieu, F. Pajot, J. M. Nicot, M. Chaigneau, G. Parot, Giorgio Savini, Y. André, M. Bouzit, Nicolas Bray, Johan Montel, C. Tucker, J.-P. Dubois, J. Martignac, J. Aumont, Maria Salatino, O. Simonella, V. Buttice, Bruno Maffei, R. J. Laureijs, R. Misawa, J.-Ph. Bernard, Frederi Mirc, B. Mot, J. Narbonne, Silvia Masi, O. Boulade, C. Engel, Etienne Perot, E. Doumayrou, A. Caillat, J. A. Tauber, C. Coudournac, A. Hughes, I. Ristorcelli, Y. Lepennec, S. Maestre, Pierre Tapie, Y. Longval, P. de Bernardis, F. Bousquet, G. Foenard, S. Grabarnik, Giampaolo Pisano, G. Roudil, P. Etcheto, P. Gélot, B. Leriche, Muriel Saccoccio, J. P. Crussaire, J. Pimentao, C. Marty, Matthew Joseph Griffin, Peter A. R. Ade, L. Baustista, M. Charra, F. Douchin, J.-P. Torre, L. Rodriguez, L. Montier, Peter Charles Hargrave, B. Crane, W. Marty, G. Versepuech
Publikováno v:
International Conference on Space Optics — ICSO 2016.
PILOT (Polarized Instrument for Long wavelength Observations of the Tenuous interstellar medium) is a balloonborne astronomy experiment designed to study the polarization of dust emission in the diffuse interstellar medium in our Galaxy. The PILOT in
Autor:
G. Roudil, B. Mot, Y. Longval, W. Marty, J. Aumont, R. Misawa, A. Caillat, Y. Lepennec, E. Doumayrou, G. Foënard, J. A. Tauber, A. Hughes, G. Parot, L. Montier, J. Pimentao, M. Chaigneau, F. Pajot, J.-Ph. Bernard, B. Crane, Johan Montel, B. Leriche, M. Bouzit, Nicolas Bray, V. Buttice, Nicolas Ponthieu, Pierre Tapie, Isabelle Ristorcelli, J. M. Nicot, Muriel Saccoccio, Giorgio Savini, F. Douchin, P. deBernardis, C. Coudournac, Frederi Mirc, J. Martignac, Etienne Perot, Bruno Maffei, J.-P. Torre, C. Engel, A. Mangilli, L. Rodriguez, Peter Charles Hargrave, S. Maestre, Y. André, Silvia Masi, L. Bautista, P. Etcheto, C. Marty, S. Stever, S. Grabarnik, Maria Salatino, O. Simonella, Giampaolo Pisano, J.-P. Dubois, Carole Tucker, P. Gélot, René J. Laureijs, F. Bousquet, Matthew Joseph Griffin, Peter A. R. Ade, J. Narbonne, Christopher Tibbs, O. Boulade
PILOT is a balloon-borne astronomy experiment designed to study the polarization of dust emission in the diffuse interstellar medium in our Galaxy at wavelengths 240 and 550 µm with an angular resolution of about two arc-min. PILOT optics is compose
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2b2ea70679b35a30e5c7752086aee7dc
http://hdl.handle.net/11573/1557103
http://hdl.handle.net/11573/1557103
Autor:
Laurent Artola, J.-M Nicot, J.-N Valdivia, Guillaume Hubert, J.-M Mouret, Ph Cocquerez, J.-R Meyer, A. Cheminet, Francoise Bezerra
Publikováno v:
IEEE Transactions on Nuclear Science. 61:1703-1709
Autor:
P. Etcheto, G. Foenard, I. Ristorcelli, W. Marty, F. Bousquet, Maria Salatino, O. Simonella, S. Grabarnik, Nicolas Ponthieu, Frederi Mirc, L. Rodriguez, J. A. Tauber, B. Mot, Pierre Tapie, Nicolas Bray, Giampaolo Pisano, Etienne Perot, R. Misawa, L. Montier, Giorgio Savini, Y. Lepennec, S. Maestre, Peter Charles Hargrave, B. Crane, J. Aumont, Bruno Maffei, C. Tucker, J.-P. Dubois, G. Parot, E. Doumayrou, L. Bautista, J.-Ph. Bernard, Johan Montel, V. Buttice, A. Caillat, M. Bouzit, Y. Longval, P. de Bernardis, R. J. Laureijs, C. Engel, Silvia Masi, J. Martignac, A. Hughes, G. Roudil, B. Leriche, Muriel Saccoccio, P. Gélot, M. Chaigneau, J. M. Nicot, J. Narbonne, Y. André, J.-P. Torre, J. P. Crussaire, J. Pimentao, C. Marty, F. Pajot, O. Boulade, M. Charra, F. Douchin, Matthew Joseph Griffin, Peter A. R. Ade
PILOT is a stratospheric experiment designed to measure the polarization of dust FIR emission, towards the diffuse interstellar medium. The first PILOT flight was carried out from Timmins in Ontario-Canada on September 20th 2015. The flight has been
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6538e90ba769dd2abe27bb54e3aea414
http://hdl.handle.net/11573/1018238
http://hdl.handle.net/11573/1018238
Autor:
J. Pimentao, G. Parot, L. Montier, J. Aumont, Bruno Maffei, M. Bouzit, L. Bautista, R. Misawa, B. Crane, B. Leriche, S. Grabarnik, A. Caillat, Nicolas Ponthieu, M. Charra, F. Bousquet, Peter Charles Hargrave, Giampaolo Pisano, Y. Lepennec, J. Narbonne, S. Maestre, Y. André, Maria Salatino, O. Simonella, F. Mirc, F. Douchin, A. Hughes, J.-P. Bernard, Matthew Joseph Griffin, P. Etcheto, Peter A. R. Ade, J. A. Tauber, Giorgio Savini, Carole Tucker, P. Gélot, G. Foënard, G. Roudil, J. P. Crussaire, W. Marty, C. Engel, Muriel Saccoccio, M. Chaigneau, F. Pajot, J. M. Nicot, Y. Longval, Isabelle Ristorcelli, L. Rodriguez, O. Boulade, P. de Bernardis, J.-P. Torre, Silvia Masi, Johan Montel, J. Martignac, E. Pérot, Nicolas Bray, B. Mot, V. Buttice, C. Marty, E. Doumayrou, René J. Laureijs, J.-P. Dubois, P. Tapie
Future cosmology space missions will concentrate on measuring the polarization of the Cosmic Microwave Background, which potentially carries invaluable information about the earliest phases of the evolution of our universe. Such ambitious projects wi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::113c83ff79f30f02c6d066d07527a293
http://hdl.handle.net/11573/944241
http://hdl.handle.net/11573/944241
Autor:
Christophe Laot, L. Delauney, Philippe Billand, J. Marvaldi, M. Nicot, Sidonie Hibral, Y. Degres, C. Lietard, A. M. Caujan, Jacques Legrand, F. Cabioch, B. Darbot, J. Guyomarch, Jean-Francois Masset, M. Jouannic
Publikováno v:
SEAFLOOR OBSERVATORIES ISBN: 9783642113734
The severe oil spill hazards that endangered environment and ecosystem equilibria in western European seas such as “Erika” (1999) and “Prestige” (2002), led the French government to open research funds under the RITMER (Reseau de recherche et
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6ddca7486be8ee312d5ef75817f38c3e
https://doi.org/10.1007/978-3-642-11374-1_9
https://doi.org/10.1007/978-3-642-11374-1_9
Publikováno v:
IEEE Transactions on Nuclear Science. 52:1795-1799
The effect of total ionizing dose on a commercial optomechanical microswitch has been studied in this paper. One microswitch was irradiated using a Co/sup 60//spl gamma/-ray radiation source at a dose rate of 330 rad/h to total dose up to 22.5 krad (
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