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1. Lecture XVII.
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[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/1996/ph162/l17a.html -- 2.7 Кб -- 19.03.1996
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2. http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/uploads/MROIFastTipTilt.TechMeet9/FTT_mount_analysis_04.pdf
... Table 1: Acceptable temperature difference Invar36 0 .0 5 C А (the CTE was selected as 0.7 for the FEA) Stainless Steel 304 0.002 CА(the CTE was selected as 17.2 for the FEA) Aluminium6061 0.0015 CА(the CTE was selected as 23 for the FEA) (2) Analysis of the temperature gradients of the mount generated by an ambient temperature difference of 0.5 CА on both sides of the mount Invar , S.S. or Al ... Stainless steel material is added to Table 4 and 5 for comparison with Invar. ...
[ Текст ]  Ссылки http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/uploads/MROIFastTipTilt.TechMeet9/FTT_mount_analysis_04.pdf -- 49.6 Кб -- 24.06.2010
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3. Determining dust temperatures and masses in the Herschel era: The importance of
... The properties of the dust grains (e.g., temperature and mass) can be derived from fitting far-IR SEDs (т??100 ЮМm). Only with SPIRE on Herschel has it been possible to get high spatial resolution at 200 to 500 ЮМm that is beyond the peak (~160 ЮМm) of dust emission in most galaxies. Aims: We investigate the differences in the fitted dust temperatures and masses determined using only 200 ЮМm data is for deriving these dust properties. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/~kgordon/papers/2010A&A...518L..89G.html -- 5.4 Кб -- 21.01.2016
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4. polA Tsys high sep15
... 09sep15: calibration run shows that problem is not the cal values. 28sep15: TsysLoad, antenna show that large Tsys Difference only occurs on antenna . ... Their ratio cancels the cal value. bottom: Ratios polB/polA . ... Comparing the ratio of sefdA,B to the ratio of TsysA,B shows that the Tsys difference is independent of the cal value (so the problem is not a problem with the cal values) . Tsys on load,antenna from 28sep15 showed that the large pola,B difference only occurs on antenna. ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~phil/430ch/polATsys_hi_sep15.html -- 8.6 Кб -- 28.09.2015
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5. Project 4 - RFBR - Stepantsov, Determination of the space anisotropy of order
... Russian Foundation for Basic Research , Project number 98-02-17366 . ... A number of experiments proposes the d -type of the wave function, having two directions with positive and two (in orthogonal direction) - with negative sign of the order parameter. ... The effect of the wave function phase is most efficiently revealed in the experiments with Josephson structures, that are used for determination of the dependences on the pulse direction. ... The project goals are: . ...
[ Сохраненная копия ]  Ссылки http://www.cplire.ru/html/oxide233/proj4.html -- 9.7 Кб -- 01.09.2005
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6. RFBR Project 01-02-16473
Investigation of grain boundary faceting phase transitions in aluminium . Project 01-02-16473 funded by . ... Head of the project . ... The twins appear instead of {111}1/{115}2 or (110)S9CSL facet. ... Parallel elongated sides of the twin plate are formed by the coherent symmetric twin (1,–1,0,–2)1||(1,–1,0,–2)2 grain boundary (STGB) facets. ... Grain boundary faceting phase transitions in zinc (in Russian) . ... Faceting and roughening of the asymmetric twin grain boundaries in zinc . ...
[ Сохраненная копия ]  Ссылки http://www.issp.ac.ru/libm/rffi16473/ -- 9.6 Кб -- 12.01.2002
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7. Internal Structure of Stars
... Development of Ideas of Structure and Evolution of Stars. Integral Features of Stars, Which Determine Their Structure, Direction and Rate of Evolutuion. ... Connection between Potential and Thermal Energy of Star. ... Structure of a Main Sequence Star. Features of Massive Stars Evolution on the Main Sequence. Internal Structure of the Sun. ... White Dwarfs, Their Features. ... Evolution from the Main Sequence of Massive Stars. ... Evolution of Small Mass Stars till White Dwarfs Sequence. ...
[ Сохраненная копия ]  Ссылки http://space.univ.kiev.ua/courses/vnutr_bud_zir_e.html -- 6.6 Кб -- 23.02.2005
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