... Registration of energy loss spectrum for the particles produced signals in both detectors allows to evaluate ionization losses spectrum for such particles. ...
... spectrum), and below f0 the spectrum is flat. [pic] Figure 7 Time spectrum of ... spectrum of temperature pulsations E2(m) for problem with rigid boundary conditions ... spectrums of kinetic energy EK2(m) for rigid (r = 6000) boundary conditions. [pic ...
... of background in the hp 0 mass spectrum by the wavelet analysis is presented ... aim is the estima tion of background in the mass spectrum of p 0 p 0 p + p meson ... of hmeson at m = 0:549 GeV in mass spectrum of p 0 p + p system are selected (fig ...
... Energy spectrum of outgoing particles) . (Energy spectrum of alphas) . ... Energy spectrum of alphas) . (Energy spectrum of deuterons) . ... Energy spectrum of deuterons) . (Energy spectrum of fission fragments) . ...
... can provide to carry measurements only in the oxygen line of the IS spectrum ... measure the hydrogen line of the IS spectrum and to change over to measurements of ... measurements with complex impulse and to register hydrogen line of IS spectrum ...
... The spectrum of the brightest star, our Sun, shows several dark gaps perpendicular ... е und 3934 е), the strongest lines in the solar spectrum (see table 1 and figure 1 ... Figure 1 : Spectrum of the Sun with it’s absorption lines. [SuW] . Name . ...
... The SHG angular spectrum has a 50° corresponded to the dip in the linear narrow peak at reflection spectrum and attributed to the fundamental field Downloaded 25 Nov 2002 to 131.174.178.245. ...
[
Текст
]
Ссылки http://shg.phys.msu.ru/ruscon/articles/pdf/02_AppPhysLett_81.pdf -- 147.1 Кб -- 12.03.2008 Похожие документы
... Solid lines correspond to a purely blackbody spectrum with T = 4000K. Short dashes correspond to a diluted blackbody spectrum with T = 20000K. Draine (1978) interstellar field is shown with medium dashes. ...
[
Текст
]
Ссылки http://www.inasan.rssi.ru/~akimkin/presentations/UVUniverse2010.pdf -- 256.1 Кб -- 12.03.2013 Похожие документы
... The 0.3-10 keV X-ray spectrum of BL Lacertae observed by Swift/XRT can be described ... This spectrum is harder than that found in any previous Swift/XRT observation ... of BL Lacertae (B2200+420, J2202+4216) across the electromagnetic spectrum ...