Zobrazeno 1 - 2
of 2
pro vyhledávání: '"T. C. Koch"'
Autor:
Peter A. R. Ade, V. Yurchenko, F. Piacentini, R. Pons, M. Nexon, G. Recouvreur, Christopher G. Paine, C. Dumesnil, Philippe Camus, J. Pahn, O. Perdereau, M. Tristram, Sarah E. Church, M.-A. Miville-Deschênes, A. Coulais, J. J. Bock, F.-X. Désert, J. Lande, G. Serra, J. F. Macías-Pérez, F. Pajot, J.-L. Beney, F. Bouchet, Simon Prunet, J.-P. Torre, C. Leroy, N. Ponthieu, Bruno Maffei, E. Bréelle, M. Giard, B. P. Crill, J.-L. Puget, L. Vibert, W. A. Holmes, T. C. Koch, E. Hivon, J. Haissinski, R. V. Sudiwala, B. Mansoux, L. Montier, K. Dassas, C. Renault, C. Evesque, R. S. Bhatia, Alain Benoit, J. Charra, Sophie Henrot-Versille, W. C. Jones, Y. Blanc, P. de Bernardis, A. Arondel, F. Couchot, C. Rosset, Martin Crook, C. Marty, Stéphane Plaszczynski, B. Leriche, Etienne Pointecouteau, D. Rambaud, D. Santos, J.-F. Sygnet, M. Charra, Tom Bradshaw, J.-M. Delouis, I. Ristorcelli, P. Eng, Jan Tauber, Thierry Maciaszek, Karim Benabed, H. Lagardère, D. Yvon, A. Moneti, J. Narbonne, Giorgio Savini, Andrew E. Lange, X. Dupac, Y. Longval, A. Catalano, R. Gispert, P. de Marcillac, P. Lami, George Efstathiou, C. Mercier, Silvia Masi, Jacques Delabrouille, J. A. Murphy, Ken Ganga, J.-Ph. Bernard, M. Piat, Adam Woodcraft, J.-M. Lamarre, G. Guyot, L. Guglielmi, P. Stassi, J.-J. Fourmond
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2010, 520, pp.A9. ⟨10.1051/0004-6361/200912975⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2010, 520, pp.A9. ⟨10.1051/0004-6361/200912975⟩
Astronomy and Astrophysics-A&A, 2010, 520, pp.A9. ⟨10.1051/0004-6361/200912975⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2010, 520, pp.A9. ⟨10.1051/0004-6361/200912975⟩
Context. The High Frequency Instrument (HFI) is one of the two focal instruments of the Planck mission. It will observe the whole sky in six bands in the 100 GHz–1 THz range.\ud \ud Aims. The HFI instrument is designed to measure the cosmic microwa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fb231804a51db41ef8e2fb53c3ac6c43
https://resolver.caltech.edu/CaltechAUTHORS:20101111-100415286
https://resolver.caltech.edu/CaltechAUTHORS:20101111-100415286
Autor:
T. C. Koch, D. P. Divincenzo
Publikováno v:
Physical Review B. 30:7092-7096
Presentation d'un modele du champ moyen pour le diagramme de phases du graphite intercale a Li. Des observations recentes indiquent la formation de differents composes Li-graphite. Ce phenomene, qui est une consequence du potentiel du graphite, est e