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21. A Kernel Model for Precision Timekeeping
The technical memorandum: A Kernel Model for Precision Timekeeping (PostScript) describes an engineering model which implements a precision time-of-day function for a generic operating system. ... The model changes the way the system clock is adjusted in time and frequency, as well as provides mechanisms to discipline its time and frequency to an external precision timing source, such as a pulse-per-second (PPS) signal. ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/~er/xntp/kern.html -- 4.0 Кб -- 21.12.2007
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22. Models recipes
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[ Сохраненная копия ]  Ссылки http://comet.sai.msu.ru/~dmbiz/Lmodeler.html -- 2.6 Кб -- 27.01.2003
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23. Description of SED models
... FTP access the basic models is here . ... Below, we put short descriptions of the used SED models for the photometric redshifts providing by the current server . ... The uniqueness of this model consists in expanding to the near IR (NIR) of Rocca-Volmerange and Guiderdoni's (1988) atlas of synthetic spectra with a revised stellar library, which includes parameters of cool stars. ... Homepage of the GISSEL model). ... Another model used earlier is the model of synthetic spectra of Poggianti (1997). ...
[ Сохраненная копия ]  Ссылки http://sed.sao.ru/sed_E_models.html -- 9.2 Кб -- 12.01.2005
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24. Set of 8pcs Hot Cartoon Minion Dave Characteristic 5 to 6cm Collection Figure
... Set of 8pcs Hot Cartoon Minion Dave Characteristic 5 to 6cm Collection Figure Model . ... Figure Height: 5~6 cm . ... Animation Models . ... Package Contents: 8 x Figure Model . ...
[ Сохраненная копия ]  Ссылки http://astrokuban.info/astroku5558.html -- 26.4 Кб -- 14.02.2016
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25. Modeling of Very Luminous Stars in the M33
... We find a transition of LBV star from the LBV instability strip to the region of classical WN for the first time. ... Numerical modeling of the atmospheres of these objects are very important for understanding the evolutionary relationship WR and LBV stars, as well as of the physical causes of LBVs variability. We studied spectra of two very luminous stars in the M33 galaxy - LBV V532 and late WN star FSZ35. ... Bottom: The spectrum of FSZ35 with the final model . ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/Doc-en/SciNews/2012/Maryeva/ -- 5.9 Кб -- 02.10.2012
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/Doc-en/SciNews/2012/Maryeva/ -- 5.9 Кб -- 02.10.2012