Results 11 to 20 of about 217,614 (319)
Application of OCT to examination of easel paintings [PDF]
, 2004 We present results of applying low coherence interferometry to gallery paintings. Infrared low coherence interferometry is capable of non-destructive examination of paintings in 3D, which shows not only the structure of the varnish layer but also the ...Cucu, R., Culshaw B., Dobre, George, Jackson, David A., Liang, H., Lopez-Higuera J.M., Pannell, C., Pedro, J., Podoleanu, Adrian G.H., Saunders, D. +9 morecore +1 more sourceLandau-Zener-Stuckelberg interferometry [PDF]
, 2010 A transition between energy levels at an avoided crossing is known as a
Landau-Zener transition. When a two-level system (TLS) is subject to periodic
driving with sufficiently large amplitude, a sequence of transitions occurs.Abragam, Amin, Ankerhold, Ao, Aravind, Arbo, Ashhab, Ashhab, Ashhab, Astafiev, Autler, Averbukh, Banerjee, Barone, Baruch, Benderskii, Berns, Berns, Bishop, Burkard, Bychkov, Bylander, Calero, Child, Chu, Clarke, Coffey, Cooper, Damski, Damski, Delone, Delos, Devoret, Di Giacomo, Dutta, Duty, Eckel, Farhi, Fink, Franco Nori, Frasca, Fregenal, Fuchs, Földi, Földi, Førre, Gaitan, Gallagher, Garanin, Garanin, Garraway, Gorelik, Goswami, Gradshteyn, Grajcar, Greenberg, Greenberg, Grifoni, Grossmann, Grossmann, Grossmann, Hausinger, Heinrich, Henry, Ho, Il’ichev, Il’ichev, Irish, Ithier, Izmalkov, Izmalkov, Ji, Johansson, Kayanuma, Kayanuma, Kayanuma, Krainov, Kral, LaHaye, Landau, Landau, Landau, Leggett, Li, Liao, Liu, Lopez-Castillo, Maeda, Majorana, Makhlin, Mark, Mark, Marzlin, McDermott, Mukherjee, Mullen, Nagaya, Nakamura, Nalbach, Nikitin, Nikitin, Nikitin, Oh, Oliver, Oliver, Paila, Pegg, Persson, Petta, Pezze, Pokrovsky, Pokrovsky, Rabi, Ribeiro, Ritus, Rodrigues, Rodrigues, Rotvig, Rotvig, Rudner, S. Ashhab, S.N. Shevchenko, Saito, Saito, Saito, Sambe, Sarandy, Shevchenko, Shevchenko, Shevchenko, Shimshoni, Shirley, Shnyrkov, Shnyrkov, Shytov, Shytov, Sillanpää, Sillanpää, Sillanpää, Son, Stückelberg, Sun, Sun, Teranishi, Thorwart, Thorwart, Tong, Tong, Tornes, van Ditzhuijzen, Vitanov, Vitanov, Vitanov, Vitanov, Wallraff, Wang, Wei, Wen, Wendin, Wernsdorfer, Wilhelm, Wilson, Wilson, Wittig, Wubs, Wubs, Yoakum, You, Zagoskin, Zel’dovich, Zener, Zenesini, Zhang, Zhang, Zhou, Zhou, Zhu, Zueco, Zurek, Zwanziger +179 morecore +1 more sourceNarrow linewidth single laser source system for onboard atom
interferometry [PDF]
, 2014 A compact and robust laser system for atom interferometry based on a
frequency-doubled telecom laser is presented. Thanks to an original
stabilization architecture on a saturated absorption setup, we obtain a
frequency-agile laser system allowing fast ...Bidel, Yannick, Bresson, Alexandre, Cadoret, Malo, Carraz, Olivier, Renon, Geoffrey, Theron, Fabien, Zahzam, Nassim +6 morecore +2 more sourcesMultichannel W-Band SAR System on a Multirotor UAV Platform With Real-Time Data Transmission Capabilities
IEEE Access, 2020 In recent years, the demand for small-scale remote sensing, which is used in disaster monitoring, agriculture, and ground subsidence has increased. A multichannel synthetic aperture radar (SAR) system can provide image and topographic information of the ...Sumin Kim, Se-Yeon Jeon, Jeongbae Kim, Ui-Min Lee, Seungha Shin, Youngwoo Choi, Min-Ho Ka +6 moredoaj +1 more sourceModern optical astronomy: technology and impact of interferometry [PDF]
, 2002 The present `state of the art' and the path to future progress in high
spatial resolution imaging interferometry is reviewed. The review begins with a
treatment of the fundamentals of stellar optical interferometry, the origin,
properties, optical ...Ables, J. G., Aime, C., Akeson, R., Anderson, J. A., Angel, J. R. P., Angel, J. R. P., Angel, J. R. P., Angel, J. R.,, Antoshkin, L. V., Aretxaga, I., Armstrong, J.,, Arnold, L., Ayers, G. R., Baba, N., Baba, N., Baba, N., Babcock, H. W., Babcock, H. W., Bagnuolo, W. G., Jr., Baldwin, J., Baldwin, J., Baldwin, J., Baldwin, J. E., Baldwin, J. E., Balick, B., Barlow, M. J., Barnaby, D., Beckers, J. M., Bedding, T., Bedding, T. R., Beichman, C., Benson, J., Berger, J., Berio, P., Berio, P., Bester, M., Blazit, A., Blöcker, T., Boccaletti, A., Boccaletti, A., Boden, A.,, Bonneau, D.,, Bonneau, D.,, Bouvier, J., Bracewell, R. N., Brandl, B., Brandner, W., Bruns, D., Burge, J. H., Burns, D., Burns, D., Butler, R.,, Cadot, O., Callados, M.,, Carleton, N., Cassinelli, J., Charbonneau, D., Clampin, M., Clampin, M., Close, L., Colavita, M., Colavita, M., Colavita, M.,, Conan, J.-M., Conan, R., Cooper, D., Cornwell, T. J.,, Coudé du Foresto, V., Coulman, C. E., Coulman, C. E., Currie, D., Danchi, W. C., Danchi, W. C., Dantowitz, R., Davidge, T. J., Davidge, T. J., Davis, J., Davis, J., Davis, J., Davis, J., Dayton, D., Dejonghe, J., Denker, C., Derie, F., DiBenedetto, G. P., Drummond, J., Dullemond, C. P., Dyck, H., Dyck, H., Ebstein, S., Eke, V., Elias, N. M., Falcke, H., Faucherre, M., Fienup, J. R., Fischer, O., Fizeau, H., Foy, R., Foy, R., Fried, D. L., Fugate, R., Gauger, A., Gerchberg, R. W., Gies, R., Glindemann, A., Golimowski, D. A., Gonsalves, S. A., Gorham, P. W., Greenwood, D. P., Haguenauer, P., Hajian, A., Hale, D., Hale, D., Hanbury Brown, R., Hanbury Brown, R., Haniff, C., Harmanec, P., Hartley, M., Harvey, J. W., Harvey, J. W., Hawley, S. A., Hege, E., Hestroffer, D., Heydari, M., Hill, J. M., Hinz, P., Hofmann, K.-H., Hummel, C., Hutchings, J., Hutchings, J., Hutchings, J., Högbom, J., Jefferies, S., Jennison, R. C., Karovska, M., Kenworthy, M., Kervella, P., Knox, K., Koechlin, L., Korff, D., Kunz, M., Labeyrie, A., Labeyrie, A., Labeyrie, A., Labeyrie, A., Labeyrie, A., Labeyrie, A., Labeyrie, A., Labeyrie, A., Labeyrie, A., Lai, O., Lai, O., Lane, B., Lannes, A., Lawson, P., Lawson, P., Lawson, P. R., Lawson, P. R., Ledoux, C., Lee, J., Lefèvre, H. C., Liang, J., Lindengren, L., Lipman, E., Liu, Y. C., Lloyd-Hart, M., Lloyd-Hart, M., Lohmann, A., Lopez, B., Lovelock, J. E., Lucy, L., Lynds, C., Léger, A., Machida, Y., Mackay, C. D., Magain, P., Malbet, F., Marco, O., Masciadri, E., Mason, B., Mason, B. D., Mayor, M., McAlister, H., Mennesson, B., Men’shchikov, A., Michelson, A. A., Michelson, A. A., Millan-Gabet, R., Monnier, J., Monnier, J., Monnier, J., Morel, S., Morel, S., Mouillet, D., Mourard, D., Mourard, D., Mozurkewich, D., Márquez, I., Nakajima, T., Nakajima, T., Natta, A., Nelkin, M., Nisenson, P., Nisenson, P., Nordgren, T., Northcott, M. J., Nota, A., Nulsen, P., Padilla, C., Papaliolios, C., Papaliolios, C., Pauls, T., Paxman, R., Pedretti, E., Pedretti, E., Pehlemann, E., Penny, A., Perrin, G., Perrin, G., Perrin, G., Perryman, M. A. C., Poulet, F., Pourbaix, D., Prieur, J., Quirrenbach, A., Quirrenbach, A., Quirrenbach, A., Rabbia, Y., Ragazzoni, R., Reinheimer, T., Richardson, W. H., Ridgway, S. T., Rimmele, T. R., Robbe, S., Robertson, N. A., Roddier, C., Roddier, F., Roddier, F., Roddier, F., Roddier, F., Roggemann, M. C., Rouan, D., Rouan, D., Rouan, D., Rousselet-Perraut, K., Rousset, G., Ryan, S., Saha, S. K., Saha, S. K., Saha, S. K., Saha, S. K., Saha, S. K., Saha, S. K., Sams, B. J., Sato, K., Schertl, D., Schöller, M., Seldin, J., Seldin, J., Serabyn, E., Shannon, C. J., Shao, M., Shao, M., Shao, M., Sicardy, B., Simon, M., Stee, P., Stee, P., Swapan K. Saha, Tango, W. J., Tatarski, V. I., Thom, C., Thompson, L. A., Timothy, J. G., Torres, G., Townes, C. H., Traub, W. A., Traub, W. A., Traub, W. A., Troxel, S. E., Tuthill, P., Tuthill, P., Tuthill, P. G., Tuthill, P. G., Tuthill, P. G., Ulrich, M., Unwin, S., Vakili, F., Vakili, F., van Belle, G., van Belle, G., van Belle, G., Von der Lühe, O., Walkup, J. F., Wallace, J., Weigelt, G., Weigelt, G., Weigelt, G., Weigelt, G., Weigelt, G., Weinberger, A., Wilken, V., Wilson, R., Wittkowski, M., Wittkowski, M., Wittkowski, M., Wittkowski, M., Wood, P., Wood, P., Worden, S. P., Wyngaard, J. C., Young, A. T., Young, J. +312 morecore +2 more sourcesSensitivity of a Bolometric Interferometer to the CMB power spectrum [PDF]
, 2008 Context. The search for B-mode polarization fluctuations in the Cosmic
Microwave Background is one of the main challenges of modern cosmology. The
expected level of the B-mode signal is very low and therefore requires the
development of highly sensitive ...Bunn, Bunn, C. Cressiot, C. Rosset, Hobson, J. Kaplan, J.-Ch. Hamilton, Knox, M. Piat, R. Charlassier, White, Zaldarriaga +11 morecore +3 more sources
