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Статті в журналах з теми "Liquid nitrogen cooled detector"
Barkan, Shaul. "Si(Li) detector for microanalysis cooled by thermoelectric device." Proceedings, annual meeting, Electron Microscopy Society of America 50, no. 2 (August 1992): 1736–37. http://dx.doi.org/10.1017/s042482010013331x.
Повний текст джерелаAnugu, Narsireddy, António Amorim, Paulo Garcia, Paulo Gordo, Tiago Frederico, and Jorge Abreu. "A Low Cost Auto-filling and Refrigeration Rate Regulated Liquid Nitrogen Controller for Near Infrared Instruments." U.Porto Journal of Engineering 1, no. 2 (March 19, 2018): 45–51. http://dx.doi.org/10.24840/2183-6493_001.002_0006.
Повний текст джерелаYakovlevs, O., V. Malgin, and V. Gostilo. "Development of Unified Spectrometric Module Based on HPGE Detectors with Electric Machine Cooling." Nuclear and Radiation Safety, no. 3(79) (August 28, 2018): 48–55. http://dx.doi.org/10.32918/nrs.2018.3(79).08.
Повний текст джерелаCovi, M., B. Pressl, T. Günthner, K. Laiho, S. Krapick, C. Silberhorn, and G. Weihs. "Liquid-nitrogen cooled, free-running single-photon sensitive detector at telecommunication wavelengths." Applied Physics B 118, no. 3 (February 4, 2015): 489–95. http://dx.doi.org/10.1007/s00340-015-6019-y.
Повний текст джерелаDi Mascio, Paolo, Etelvino J. H. Bechara та Joel C. Rubim. "Dioxygen NIR FT-Emission (1Δg → 3Σ−g) and Raman Spectra of 1,4-Dimethylnaphthalene Endoperoxide: A Source of Singlet Molecular Oxygen". Applied Spectroscopy 46, № 2 (лютий 1992): 236–39. http://dx.doi.org/10.1366/0003702924125528.
Повний текст джерелаBarkan, S., K. F. Ihrig, and M. B. Abott. "Unprecedented Performance Improvement For Thermoelectrically Cooled Si(Li) Detector for EDS." Microscopy and Microanalysis 4, S2 (July 1998): 198–99. http://dx.doi.org/10.1017/s1431927600021115.
Повний текст джерелаWu Hao, 吴昊, 朱一帆 Zhu Yifan, 丁青峰 Ding Qingfeng, 张金峰 Zhang Jinfeng, 上官阳 Shangguan Yang, 孙建东 Sun Jiandong та 秦华 Qin Hua. "液氮制冷的AlGaN/GaN HEMT太赫兹探测器阵列特性研究". Infrared and Laser Engineering 51, № 12 (2022): 20220225. http://dx.doi.org/10.3788/irla20220225.
Повний текст джерелаNicholls, A. W., and P. E. Bovey. "A Cryo-transfer facility for the VG HB501 STEM." Proceedings, annual meeting, Electron Microscopy Society of America 47 (August 6, 1989): 746–47. http://dx.doi.org/10.1017/s0424820100155700.
Повний текст джерелаKeltner, Zachary, Katherine Kayima, Adam Lanzarotta, Luis Lavalle, Marina Canepa, Anthony E. Dowrey, Gloria M. Story, Curtis Marcott, and André J. Sommer. "Prism-Based Infrared Spectrographs Using Modern-Day Detectors." Applied Spectroscopy 61, no. 9 (September 2007): 909–15. http://dx.doi.org/10.1366/000370207781745982.
Повний текст джерелаRen, Hao, Qun Zeng, and Xi Hui Liang. "Characterization of Nd:Y3Al5O12 Thin Films Prepared by Electron Beam Evaporation Deposition." Applied Mechanics and Materials 320 (May 2013): 150–54. http://dx.doi.org/10.4028/www.scientific.net/amm.320.150.
Повний текст джерелаДисертації з теми "Liquid nitrogen cooled detector"
Lozza, Valentina. "Low energy low background photon counter for wisp search experiments." Doctoral thesis, Università degli studi di Trieste, 2010. http://hdl.handle.net/10077/3719.
Повний текст джерелаRemarkable interest has recently arisen about the search for Weakly Inter- acting Sub-eV Particles (WISPs), such as axions, Axion Like Particles (ALPs), Minicharged and chameleon particles, all of which are not included in the Stan- dard Model. Precision experiments searching for WISPs probe energy scales as high as 10^6 TeV and are complementary to accelerator experiments, where the energy scale is a few TeV. The axion, in particular, is the oldest studied and has the strongest theoretical motivation, having its origin in Quantum Chromodynamics. It was introduced for the first time in 1973 by Peccei and Quinn to solve the strong CP problem, while later on the cosmological implications of its postulated existence also became clear: it is a good candidate for the cold dark matter, and it is necessary to fully explain the evolution of galaxies. Among the different interactions of axions, the most promising for its detection, from an experimental point of view, is the coupling to two photons (Primakoff effect). Using this coupling, several bounds on the axion mass and energy scale have been set by astrophysical observations, by laboratory experiments and by the direct observation of celestial bodies, such as the Sun. Most of these considerations, as was recently recognized, not only constrain the mass and coupling of the axion, but are more generally applicable to all ALPs. The current best limits on the coupling, over a wide range of ALP masses, come from the the CAST (Cern Axion Solar Telescope) experiment at Cern, which looks for ALPs produced in the solar core. The experiment is based on the Primakoff effect in a high magnetic field, where solar ALPs can be reconverted in photons. The CAST magnet, a 10 T, 10 m long LHC superconducting dipole, is placed on a mobile platform in order to follow the Sun twice a day, during sunrise and sunset, and has two straight bores instrumented with X-ray detectors at each end. The re- generated photon flux is, in fact, expected to be peaked at a few keV. On the other hand, there are suggestions that the problem of the anomalous temperature profile of the solar corona could be solved by a mechanism which could enhance the low energy tail of the regenerated photon spectrum. A low energy photon counter has, for this reason, been designed and built to cover one of the CAST ports, at least temporarily. Low energy, low background photon counters such as the one just mentioned, are also crucial for most experiments searching for WISPs. The low energy photon counting system initially developed to be coupled to CAST will be applicable, with proper upgrades, to other WISPs search experiments. It consists of a Galilean telescope to match the CAST magnet bore cross section to an optical fiber leading photons to the sensors, passing first through an optical switch. This last device allows one to share input photons between two different detectors, and to acquire light and background data simultaneously. The sensors at the end of this chain are a photomultiplier tube and an avalanche photodiode operated in Geiger mode. Each detector was preliminary characterized on a test bench, then it was coupled to the optical system. The final integrated setup was subsequently mounted on one of the CAST magnet bores. A set of measurements, including live sun tracking, was carried out at Cern during 2007-2008. The background ob- tained there was the same measured in the test bench measurements, around 0.4 Hz, but it is clear that to progress from these preliminary measurements a lower background sensor is needed. Different types of detectors were considered and the final choice fell on a Geiger mode avalanche photodiode (G-APD) cooled at liquid nitrogen temperature. The aim is to drastically reduce the dark count rate, al- though an increase in the afterpulsing phenomenon is expected. Since the detector is designed to be operated in a scenario where a very low rate of signal photons is predicted, the afterpulsing effect can be accepted and corrected by an increase in the detector dead time. First results show that a reduction in background of a factor better than 10^4 is obtained, with no loss in quantum e ciency. In addition, an optical system based on a semitransparent mirror (transparent to X-rays and re ective for 1-2 eV photons) has been built. This setup, covering the low energy spectrum of solar ALPs, will be installed permanently on the CAST beamline. Current work is centered on further tests on the liquid nitrogen cooled G-APD concept involving different types of sensors and different layouts of the front-end read-out electronics, with a particular attention to the quenching cir- cuit, whether active or passive. Once these detector studies are completed, the final low background sensor will be installed on the CAST experiment. It is important to note that the use of a single photon counter for low energy photons having a good enough background (<1 Hz at least) is not limited to the CAST case, but is of great importance for most WISPs experimental searches, with special regard for photon regeneration experi- ments, and, in general, for the field of precision experiments in particle physics.
Negli ultimi tempi è riemerso un notevole interesse nel campo della ricerca di particelle leggere debolmenti interagenti (Weakly Interacting Sub-eV Particles - WISPs), come ad esempio assioni, particelle con comportamenti simili agli assioni (Axion Like Particles - ALPs), particelle con carica frazionaria e particelle camaleonte; tutti tipi di particelle non inclusi nel Modello Standard. Vista la loro natura debolmente interagente, la scala di energia coinvolta è dell'ordine dei 10^6 TeV, queste particelle non sono visibili nelle collisioni realizzabili negli attuali acceleratori e possono invece essere studiate in esperimenti di precisione, che, sotto questo punto di vista, diventano complementari agli esperimenti su acceleratori. L'assione in particolare è la prima particella, da un punto di vista cronologico, ad essere stata ipotizzata, ed inoltre la sua esistenza è supportata da forti basi teoriche: la sua origine va infatti ricercata all'interno della Cromodinamica Quantistica (QCD). L'assione fu introdotto per la prima volta nel 1973 da Peccei e Quinn come soluzione del problema di violazione di CP nelle interazioni forti, mentre le sue implicazioni cosmologiche risultarono chiare solo in seguito. L'assione infatti può essere considerato un buon candidato per la materia oscura fredda e la sua introduzione è necessaria per spiegare l'evoluzione delle galassie. Tra le diverse interazione degli assioni con la materia e la radiazione, la più interessante da un punto di vista sperimentale è l'accoppiamento con due fotoni (effetto Primakoff). Usando questo tipo di accoppiamento numerosi limiti, sia sulla massa dell'assione che sulle scale di energia coinvolte, possono essere ottenuti da osservazioni astrofisiche e da esperimenti di laboratorio così come dalla diretta osservazione di oggetti celesti tipo il Sole. Queste considerazioni possono essere applicate non solo all'assione ma più in generale a tutte le ALPs. Attualmente i limiti migliori sulla costante di accoppiamento, su un largo spettro di masse di ALPs, si sono ottenuti dall'esperimento CAST (Cern Axion Solar Tele- scope) al Cern, che guarda agli ALPs prodotti nel Sole. L'esperimento è basato sull'effetto Primakoff in un campo magnetico elevato, dove gli ALPs solari sono riconvertiti in fotoni. Il magnete dell'esperimento CAST è costituito da un prototipo per un dipolo superconduttore di LHC, lungo 10 m e con un campo magnetico totale di 10 T. Il magnete è posto su di un affusto mobile per poter seguire il sole durante le fasi di alba e tramonto. Alle due estremità del magnete sono disposti quattro rivelatori sensibili nel campo degli X molli. Il picco del usso di fotoni rigenerato è infatti atteso a pochi keV. Tuttavia, ci sono suggerimenti che il prob- lema ancora aperto del profilo di temperatura della corona solare può essere risolto tramite un meccanismo che contemporaneamente incrementerebbe le code a bassa energia dell'atteso usso di fotoni rigenerati. A questo scopo un contatore di fotoni sensibile nell'intervallo del visibile è stato progettato ed assemblato per coprire una delle quattro porte del magnete di CAST, almeno temporaneamente. I contatori di fotoni studiati hanno un largo campo di applicazione e possono essere usati in altri tipi di esperimenti per la ricerca di WISPs. Il sistema inizialmente sviluppato per CAST consiste in un telescopio Galileiano per accoppiare una fibra ottica all'apertura del magnete di CAST, la fibra ottica è quindi collegata ad un interruttore ottico che permette di utilizzare due rivelatori contemporaneamente. La fibra in ingresso è infatti collegata alternativamente a due fibre in uscita, in questo modo ciascun rivelatore acquisisce per metà del tempo segnale e per metà del tempo fondo, lasciando inalterato il tempo totale di integrazione. I sensori utilizzati fino ad ora al termine della catena ottica sono un tubo fotomoltiplicatore e un avalanche photodiode operato in modalità Geiger. Ciascun rivelatore è stato preliminarmente caratterizzato su un banco di prova e quindi collegato al sistema ottico. Il sistema finale è stato quindi installato su CAST. Una serie di misure, che includono reali prese dati, sono state condotte al Cern durante il 2007-2008. La misura del fondo ottenuta a CAST è stata la stessa misurata durante i test di prova a Trieste, circa 0.4 Hz, ma risulta chiaro che il vero sviluppo futuro è basato su un sensore a fondo molto più basso. A questo scopo sono stati considerati diversi tipi di sensore e la scelta finale è ricaduta su di un avalanche photodiode operato in modalità Geiger e raffreddato all'azoto liquido. Lo scopo è quello di ridurre drasticamente i conteggi di fondo, sebbene a queste temperature sia atteso un incremento del rateo di afterpulses. Tuttavia il rivelatore è pensato per essere utilizzato in un applicazione a basso rateo e quindi il fenomeno degli afterpulses può essere ridotto agendo direttamente sul tempo morto del rivelatore, cioè aumentandolo. I primi test condotti sul rivelatore mostrano un decremento del fondo pari ad un fattore meglio di 10^4, senza rilevabili variazioni in efficienza. In aggiunta a questo sistema, per ottenere un'installazione permanente sul fascio di CAST, è stato realizzato uno specchio semitrasparente, che lascia pressocchè inalterato il fascio di raggi X e invece de ette il fascio di fotoni con energia nel visibile. Il lavoro attuale è incentrato sullo sviluppo del rivelatore a basso fondo raffreddato all'azoto liquido, includendo anche lo studio di diversi tipi di sensore e diversi tipi di elettronica di lettura, con particolare attenzione all'elettronica di quenching del circuito con le varianti attiva e passiva. Una volta terminati gli studi sui diversi tipi di rivelatori, l'apparato finale sarà installato su CAST. E' comunque importante notare che l'uso di un rivelatore a singolo fotone sensibile tra 1-2 eV con un fondo sufficientemente basso (<1 Hz almeno) non è limitato all'uso su CAST ma in tutti gli altri esperimenti per la ricerca di WISPs, con particolare riguardo agli esperimenti di rigenerazione risonante, e in generale, nel campo di applicazione degli esperimenti di precisione alla fisica delle particelle.
1982
Bergner, Sandra, and Sandra Nilsson. "Screening of volatile compounds in washing water and cloths from the sponge cloth process." Thesis, Linköping University, Department of Physics, Chemistry and Biology, 2010. http://urn.kb.se/resolve?urn=urn:nbn:se:liu:diva-57114.
Повний текст джерелаFreudenberg Household Products AB in Norrköping are manufacturer of sponge cloths with the well-known brand names of Wettex® and Vileda®. The production is based on the viscose fiber process and involves a high chemical demand. Recent customer complaints involve a diffuse smell from the cloths that is like a “garage odor” and occurs after a few uses. The company’s theory is that the smell derives from a chemical used in the process called Exxal 9.
The aim was to screen the washing water from two sections and the cloth before and after wash for the presence of Exxal 9 and other prominent components. The washing water samples consisted of a salt solution from one section and a water condensate from another section. A method to qualitatively and quantitatively examine the production samples was developed. To evaluate the variation over a short period of time, twelve samples were taken during four weeks. The focus for the analysis lay on production line Wx4, but comparisons with two other production lines, Wx7 and SL1, were also made. The method of choice was gas chromatography in combination with two different detectors; mass spectrometer for identification and flame ionization detector for quantification.
Exxal 9 could be identified in both of the washing water sections but in very various concentrations. At the production line Wx4, the mean concentration in the mother lye was 61.96 µl/l whereas the mean concentration in the condensate was 0.24 µl/l. The comparison between the different production lines showed significant variations, where Wx4 had the highest concentration. In the cloths, Exxal 9 could only be found before it had been washed. The concentration in the cloths was not high enough for quantification. In both the washing waters and cloths, additional unknown peaks were found. Attempts to identify all the unknowns were made but only two compounds were included in the commercial library; 2-ethyl-1-hexanol and 2-(2-butoxyethoxy)-ethanol.
Книги з теми "Liquid nitrogen cooled detector"
M, Zhang Z., and National Institute of Standards and Technology (U.S.), eds. Liquid-nitrogen-cooled high Tc electrical substitution radiometer as a broadband IR transfer standard. Gaithersburg, MD: U.S. Dept. of Commerce, Technology Administration, National Institute of Standards and Technology, 1996.
Знайти повний текст джерелаM, Zhang Z., and National Institute of Standards and Technology (U.S.), eds. Liquid-nitrogen-cooled high Tc electrical substitution radiometer as a broadband IR transfer standard. Gaithersburg, MD: U.S. Dept. of Commerce, Technology Administration, National Institute of Standards and Technology, 1996.
Знайти повний текст джерелаM, Zhang Z., and National Institute of Standards and Technology (U.S.), eds. Liquid-nitrogen-cooled high Tc electrical substitution radiometer as a broadband IR transfer standard. Gaithersburg, MD: U.S. Dept. of Commerce, Technology Administration, National Institute of Standards and Technology, 1996.
Знайти повний текст джерелаM, Zhang Z., and National Institute of Standards and Technology (U.S.), eds. Liquid-nitrogen-cooled high Tc electrical substitution radiometer as a broadband IR transfer standard. Gaithersburg, MD: U.S. Dept. of Commerce, Technology Administration, National Institute of Standards and Technology, 1996.
Знайти повний текст джерелаLiquid-nitrogen-cooled high Tc electrical substitution radiometer as a broadband IR transfer standard. Gaithersburg, MD: U.S. Dept. of Commerce, Technology Administration, National Institute of Standards and Technology, 1996.
Знайти повний текст джерелаLiquid-nitrogen-cooled high Tc electrical substitution radiometer as a broadband IR transfer standard. Gaithersburg, MD: U.S. Dept. of Commerce, Technology Administration, National Institute of Standards and Technology, 1996.
Знайти повний текст джерелаЧастини книг з теми "Liquid nitrogen cooled detector"
Zhang, Y., H. Schütt, H. Bousack, W. Wolf, A. Schirdewan, M. Burghoff, and L. Trahms. "Magnetocardiography Using SQUIDs Cooled by Liquid Nitrogen." In Biomag 96, 158–61. New York, NY: Springer New York, 2000. http://dx.doi.org/10.1007/978-1-4612-1260-7_40.
Повний текст джерелаLi, Q., X. Li, T. Jiang, and G. E. McIntosh. "Optimal Thermal Design of Helium Dewar with Liquid Nitrogen and Vaporized Helium Cooled Intercepts." In Advances in Cryogenic Engineering, 841–47. Boston, MA: Springer US, 1990. http://dx.doi.org/10.1007/978-1-4613-0639-9_101.
Повний текст джерелаLi, Q., X. Li, G. E. McIntosh, and R. W. Boom. "Minimization of Total Refrigeration Power of Liquid Neon and Nitrogen Cooled Intercepts for SMES Magnets." In Advances in Cryogenic Engineering, 833–40. Boston, MA: Springer US, 1990. http://dx.doi.org/10.1007/978-1-4613-0639-9_100.
Повний текст джерелаBijnen, F. G. C., T. Brugman, F. J. M. Harren, and J. Reuss. "A Liquid Nitrogen Cooled CO Laser in a Photoacoustic Set-Up Monitors Low Gas Concentrations." In Photoacoustic and Photothermal Phenomena III, 34–37. Berlin, Heidelberg: Springer Berlin Heidelberg, 1992. http://dx.doi.org/10.1007/978-3-540-47269-8_9.
Повний текст джерелаTræholt, C., C. Rasmussen, A. Kühle, S. Krüger Olsen, K. Høj Jensen, O. Tønnesen, D. W. A. Willén, M. Däumling, and C. N. Rasmussen. "Operating a Cryogenic Test RIG for a 10 Meter Long Liquid Nitrogen Cooled Superconducting Power Cable." In Advances in Cryogenic Engineering, 1517–24. Boston, MA: Springer US, 2000. http://dx.doi.org/10.1007/978-1-4615-4215-5_72.
Повний текст джерелаVisscher, Martijn, Matthias Holling, Joost Pouw, and Bennie ten Haken. "A Magnetometer Cooled with Liquid Nitrogen for the Characterization and Quantification of Magnetic Nanoparticles in Biological Samples at Room Temperature." In Springer Proceedings in Physics, 377–78. Berlin, Heidelberg: Springer Berlin Heidelberg, 2012. http://dx.doi.org/10.1007/978-3-642-24133-8_65.
Повний текст джерелаAnwar, Saeed, and Toshifumi Yokota. "Rapid Freezing of Skeletal and Cardiac Muscles Using Isopentane Cooled with Liquid Nitrogen and Tragacanth Gum for Histological, Genetic, and Protein Expression Studies." In Methods in Molecular Biology, 45–53. New York, NY: Springer US, 2022. http://dx.doi.org/10.1007/978-1-0716-2772-3_3.
Повний текст джерелаOota, Tomoya, and Atsuko Fukaya. "Axial-Gap Superconducting Synchronous Motors Cooled by Liquid Nitrogen." In World Scientific Series in Applications of Superconductivity and Related Phenomena, 451–62. WORLD SCIENTIFIC, 2016. http://dx.doi.org/10.1142/9789814749268_0033.
Повний текст джерелаAshworth, S. P., C. Beduz, R. G. Scurlock, and Y. Yang. "STABILITY OF HIGH Tc SUPERCONDUCTORS COOLED IN A LIQUID NITROGEN POOL." In Proceedings of the Twelfth International Cryogenic Engineering Conference Southampton, UK, 12–15 July 1988, 943–49. Elsevier, 1988. http://dx.doi.org/10.1016/b978-0-408-01259-1.50182-0.
Повний текст джерела"Tensile Testing at Low Temperatures." In Tensile Testing, 239–49. 2nd ed. ASM International, 2004. http://dx.doi.org/10.31399/asm.tb.tt2.t51060239.
Повний текст джерелаТези доповідей конференцій з теми "Liquid nitrogen cooled detector"
Trojnar, Eugeniusz, Stanislaw Trojanowski, Roman Czechowicz, Mariusz Derwiszynski, and Krzysztof Kocyba. "Liquid-nitrogen-cooled low-noise radiation pulse detector amplifier." In Szczecin - DL tentative, edited by Wieslaw L. Wolinski, Bohdan K. Wolczak, Jerzy K. Gajda, Danuta Gajda, and Ryszard S. Romaniuk. SPIE, 1991. http://dx.doi.org/10.1117/12.57171.
Повний текст джерелаIkamas, Kestutis, Arnoldas Solovjovas, Dovile Cibiraite-Lukenskiene, Viktor Krozer, Alvydas Lisauskas, and Hartmut G. Roskos. "Optical Performance of Liquid Nitrogen Cooled Transistor-Based THz Detectors." In 2020 45th International Conference on Infrared, Millimeter and Terahertz Waves (IRMMW-THz). IEEE, 2020. http://dx.doi.org/10.1109/irmmw-thz46771.2020.9370863.
Повний текст джерелаBleuse, Joël, Jean-François Jacquot, Robert Picard, Joël Bonnet-Gamard, and Philippe Tribolet. "Development of a fast mid-infrared integrating optical mutichannel analyzer." In The European Conference on Lasers and Electro-Optics. Washington, D.C.: Optica Publishing Group, 1996. http://dx.doi.org/10.1364/cleo_europe.1996.ctho2.
Повний текст джерелаBijnen, F. G. C., F. J. M. Harren, J. Reuss, and J. H. P. Hackstein. "Gas detector measures parts per trillion: periodic CH4 and H2O release from a single cockroach." In The European Conference on Lasers and Electro-Optics. Washington, D.C.: Optica Publishing Group, 1994. http://dx.doi.org/10.1364/cleo_europe.1994.cwi1.
Повний текст джерелаKearney, Ian, and Mark Dipsey. "Trends in Discrete Power MOSFET and Power System In-Package Fault Isolation." In ISTFA 2017. ASM International, 2017. http://dx.doi.org/10.31399/asm.cp.istfa2017p0419.
Повний текст джерелаHastie, D. R., H. I. Schiff, G. W. Harris, D. Karecki, and G. I. Mackay. "Detection of trace atmospheric species at sub-parts-per-billion levels using tunable diode lasers." In OSA Annual Meeting. Washington, D.C.: Optica Publishing Group, 1987. http://dx.doi.org/10.1364/oam.1987.tut2.
Повний текст джерелаZhao, Y., J. Lawler, P. Foroughi, and M. Ohadi. "Development of an Electrohydrodynamic (EHD) Micro Pump for LN2 Spot Cooling." In ASME 2003 International Mechanical Engineering Congress and Exposition. ASMEDC, 2003. http://dx.doi.org/10.1115/imece2003-55625.
Повний текст джерелаPadalko, A. G., V. B. Lazarev, and F. S. Perry. "Medium impedance room temperature indium antimonide thin layer detectors." In The European Conference on Lasers and Electro-Optics. Washington, D.C.: Optica Publishing Group, 1994. http://dx.doi.org/10.1364/cleo_europe.1994.cthi54.
Повний текст джерелаMcNulty, Ian. "Low-noise charge-coupled device camera for soft-x-ray imaging." In OSA Annual Meeting. Washington, D.C.: Optica Publishing Group, 1990. http://dx.doi.org/10.1364/oam.1990.mmm4.
Повний текст джерелаChwala, A., F. Bauer, R. IJsselsteijn, R. Stolz, M. Schulz, N. Oukhanski, E. O. Köstlin, and H. G. Meyer. "Liquid Nitrogen cooled SQUID magnetometer for TEM." In 10th SAGA Biennial Technical Meeting and Exhibition. European Association of Geoscientists & Engineers, 2007. http://dx.doi.org/10.3997/2214-4609-pdb.146.11.4.
Повний текст джерелаЗвіти організацій з теми "Liquid nitrogen cooled detector"
Bigu, J. Improved 220Rn measurement characteristics of scintillation cells cooled to liquid nitrogen temperatures. Natural Resources Canada/CMSS/Information Management, 1993. http://dx.doi.org/10.4095/328834.
Повний текст джерелаRice, Joseph P. Liquid-nitrogen-cooled high Tc electrical substitution radiometer as a broadband IR transfer standard. Gaithersburg, MD: National Bureau of Standards, 1996. http://dx.doi.org/10.6028/nist.tn.1414.
Повний текст джерелаLiquid nitrogen-cooled diamond-wire concrete cutting. Innovative technology summary report. Office of Scientific and Technical Information (OSTI), December 1998. http://dx.doi.org/10.2172/325787.
Повний текст джерела