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Autor:
Hyun Su Lee, Sung Hun Kim, Youngmo Ku, Jong Hwi Jeong, Chan Hyeong Kim, Dong Ho Shin, Jong Hoon Park
Publikováno v:
Nuclear Engineering and Technology, Vol 51, Iss 2, Pp 533-538 (2019)
The mechanical-collimation imaging is the most mature technology in prompt gamma (PG) imaging which is considered the most promising technology for beam range verification in proton therapy. The purpose of the present study is to compare the performa
Publikováno v:
Results in Physics, Vol 17, Iss, Pp 103095-(2020)
Transmitted wavefronts are usually measured by a laser interferometer of the corresponding design wavelength. The Zernike coefficient can be used to describe the transmitted wavefront of a circular aperture. However, it has some limitations in optica
Publikováno v:
Results in Physics, Vol 8, Iss, Pp 933-938 (2018)
Near medium intense (NMI) fringe is a kind of intense fringe which can be formed near Kerr medium in high-power laser beam propagation. The formation properties of NMI fringe and the relations between NMI fringe and related important parameters are s
Autor:
On, behalf of ASTRO-H/SXI team, Inoue, Shota, Hayashida, Kiyoshi, Katada, Shuhei, Nakajima, Hiroshi, Nagino, Ryo, Anabuki, Naohisa, Tsunemi, Hiroshi, Tsuru, Takeshi Go, Tanaka, Takaaki, Uchida, Hiroyuki, Nobukawa, Masayoshi, Kawabata, Nobukawa Kumiko, Washino, Ryosaku, Mori, Koji, Isoda, Eri, Sakata, Miho, Kohmura, Takayoshi, Tamasawa, Koki, Tanno, Shoma, Yoshino, Yuma, Konno, Takahiro, Ueda, Shutaro
Publikováno v:
Nuclear Instruments & Methods in Physics Research. Section A, Accelerators, Spectrometers, Detectors and Associated Equipment. 831:415-419
著者人数: 22名
Accepted: 2016-03-22
資料番号: SA1160136000
Accepted: 2016-03-22
資料番号: SA1160136000
Gravitational wave detectors rely on ultra-high precision interferometry to detect dynamic strains arising from fluctuations in space-time from cataclysmic astrophysical events. The resulting displacements occur on the sub-attometer and smaller level
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4f3b56fb6428523f23c96cbef52da7f3
https://doi.org/10.1016/bs.aamop.2019.04.002
https://doi.org/10.1016/bs.aamop.2019.04.002
Autor:
Peter Hawkes, Erwin Kasper
Electron lenses are very sensitive to the energy and hence the wavelength of the electrons. The resulting chromatic aberrations are characterised by chromatic aberration coefficients, which are again needed in both real and asymptotic form. Formulae
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ea121b99b52cd152edb4bba40919e4fd
https://doi.org/10.1016/b978-0-08-102256-6.00026-2
https://doi.org/10.1016/b978-0-08-102256-6.00026-2
Autor:
Peter Hawkes, Erwin Kasper
Sector fields and combinations of sectors are employed whenever dispersion is wanted. Sectors typically have a circular optic axis within the device and are terminated by fringing fields that have a more complex structure, frequently replaced by the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::738cd3a988329a840b4afcf54a6b888f
https://doi.org/10.1016/b978-0-12-813369-9.00052-x
https://doi.org/10.1016/b978-0-12-813369-9.00052-x
Autor:
Peter Hawkes, Erwin Kasper
This chapter illustrates the deviation coefficients of systems characterized by a pair of regular symmetrical planes are of less interest at reasonably modest energies than those of rotationally symmetric components. Although, they are needed in two
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b27dcc838f0e21a75e3e5a8473b84e60
https://doi.org/10.1016/b978-0-08-102256-6.00029-8
https://doi.org/10.1016/b978-0-08-102256-6.00029-8
Autor:
Atsushi Harayama, Kei Genba, Yoshikatsu Kuroda, Tadayuki Takahashi, Hirokazu Odaka, Shin Watanabe, Yuto Ichinohe, Hiroshi Ikebuchi, Hiroyasu Tajima, Shin'ichiro Takeda, Tetsuya Tomonaka, Daisuke Matsuura
Publikováno v:
Nuclear Instruments & Methods in Physics Research. Section A, Accelerators, Spectrometers, Detectors and Associated Equipment. 787:207-211
著者人数: 12名
資料番号: SA1004998000
資料番号: SA1004998000
Autor:
Ł. Grudnik, A. Neronov, M. Grudzińska, P. J. Rajda, J. Blocki, Petr Schovanek, K. Lalik, J. Michałowski, Mohamed Rameez, Jacek Niemiec, Teresa Montaruli, M. Stodulska, W. Bilnik, J. Kasperek, M. Dyrda, A. Zagdański, L. D. Medina Miranda, E. jr. Schioppa, Dusan Mandat, J. Borkowski, Juanan Aguilar, K. Seweryn, R. Moderski, M. Janiak, K. Skowron, A. Porcelli, M. Sowiński, Vitalii Sliusar, M. Stodulski, Leszek Bogacz, I. Troyano Pujadas, B. Idźkowski, K. Ziȩtara, A. Marszałek, A. Frankowski, Łukasz Stawarz, P. Żychowski, R. Walter, M. Heller, M. Wiȩcek, E. Prandini, D. della Volpe, Miroslav Pech, Yannick Favre, Simona Toscano, P. Paśko, M. Curyło, E. Mach, Frank Raphael Cadoux, Marek Jamrozy, Tomasz Bulik, A. Christov, Michal Ostrowski, E. Lyard
The Cherenkov Telescope Array (CTA), the next generation very high energy gamma-rays observatory, will consist of three types of telescopes: large (LST), medium (MST) and small (SST) size telescopes. The SSTs are dedicated to the observation of gamma
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a0e61b7b76c5e0f04f3dc27e584fe7f9
https://biblio.vub.ac.be/vubir/characterization-and-commissioning-of-the-sst1m-camera-for-the-cherenkov-telescope-array(919fe94b-905b-41c6-821a-3527754eda31).html
https://biblio.vub.ac.be/vubir/characterization-and-commissioning-of-the-sst1m-camera-for-the-cherenkov-telescope-array(919fe94b-905b-41c6-821a-3527754eda31).html