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Titlebook: Russian Workers And The Socialist-Revolutionary Party Through The; Christopher Rice Book 1988 Palgrave Macmillan, a division of Macmillan

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21#
發(fā)表于 2025-3-25 05:20:31 | 只看該作者
Epilogue,ed by no more than the occasional signal from a handful of lesser centres — Arkhangelsk, Riga, Voronezh, Poltava, Kiev, Khar’kov and Sevastopol’. There was to be no substantial improvement in this situation before the outbreak of the First World War, despite a significant upturn in labour unrest bet
22#
發(fā)表于 2025-3-25 10:28:31 | 只看該作者
Christopher Ricelsed laser radiation in wavelengths ranging from far-IR to ultraviolet; and (3) to manufacture adaptive POEs for correcting and measuring nonstationary phase distortions in the time interval up to several milliseconds, by selecting the substrate materials of the mirror surface which provide their pr
23#
發(fā)表于 2025-3-25 12:17:02 | 只看該作者
Christopher Riceistort the spatial characteristics of the beam. When measuring the divergence of the radiation of high-power laser facilities, the energy density in the focal region of the beam is critically close to the optical breakdown threshold. Therefore, the search for the ways of deflecting and attenuating r
24#
發(fā)表于 2025-3-25 19:07:47 | 只看該作者
Christopher Rices consisting of a phase distortion corrector, a wavefront sensor and a control system. If the phase distortions, which must be compensated for, are smooth, the high quality correction can be obtained by using adaptive POEs with a continuously deformable surface. However, due to non-locality and non-
25#
發(fā)表于 2025-3-25 22:49:00 | 只看該作者
26#
發(fā)表于 2025-3-26 02:44:48 | 只看該作者
Christopher Rices, HRAS and Haystack, and Onsala participated in about half of the sessions. The MERIT and POLARIS observations were made with the third generation MARK III VLBI system using procedures and schedules designed to yield high quality geodetic information, including Earth rotation values. This paper bri
27#
發(fā)表于 2025-3-26 07:47:51 | 只看該作者
28#
發(fā)表于 2025-3-26 10:16:13 | 只看該作者
29#
發(fā)表于 2025-3-26 15:24:03 | 只看該作者
Christopher Ricem the radial velocity amplitude (.) disagrees with that derived from the ellipsoidal modulation (. assuming corotation). This mismatch was found before, but with our smaller inclination, the discrepancy is even larger than previously reported. Accounting for the rapid rotation of the A-star, instead
30#
發(fā)表于 2025-3-26 19:07:23 | 只看該作者
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