.

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... 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. ...

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• http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/uploads/MROIFastTipTilt.TechMeet9/FTT_mount_analysis_05.pdf

... 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. ...

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• Enhanced dust heating in the bulges of early-type spiral galaxies
• STIS Data Handbook
• cgvc 121

... 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. ...

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• sbc4_hiTsys_27aug12
• ALFA Performance at 1665 MHz
• ALFA performance at 1.665 GHz AO Technical Memo 2004-01

... 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: . ...

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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 . ...

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• B. Straumal homepage

... 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. ...

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Dimmings or transient coronal holes (i.e. regions of decreased intensity of soft X-ray and EUV emission), which are observed on the solar disk after halo coronal mass ejections (CMEs), are analyzed using SOHO/EIT data simultaneously in three coronal lines Fe IX/X (171 A), Fe XII (195 A) and Fe IX (284 A) sensitive to temperatures Te~1.2, 1.5 and 2.0 MK, respectively, as well as in the transition region line He II (304 A; Te~(0.02-0.08) MK). ...

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• Oct-Nov 2003
• The Basille Day 2000 Event

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Context We report on the plasma properties of small-scale transient events identified in the quiet Sun, coronal holes and their boundaries. ... We measure Doppler shifts using single and multiple Gauss fits of transition region and coronal lines as well as electron densities and temperatures. ... Most of these events represent X-ray jets from pre-existing or newly emerging coronal bright points at X-ray temperatures. ...

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• J.G. Doyle, Research Astronomer
• Climatology

... Orion's Star Colors . ... Red stars are cool, with temperatures of around 3,000 degrees Kelvin (K), while blue stars are hotter and can have temperatures over 30,000 degrees K. Our own lovely yellow Sun's temperature is a comforting 6,000 degrees K. Differences in star colors are dramatically illustrated in the above photo of the constellation Orion , made using a "star trail step-focus" technique . ... Publications with keywords: Orion . ... LDN 1622: Dark Nebula in Orion . ... Orion s Cradle . ...

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• Star Colors in Orion
• Journal "Peremennye Zvezdy"
• Астронет > Orion's Star Colors

spaceweb@oulu.fi - last update: 11 May 1998, 0900 UT . Matter in the known universe can be classified in terms of four states: solid, liquid, gaseous, and plasma . The basic distinction between solids, liquids and gases lies in the difference between the strength of the bonds that hold their constituent particles together. ... On the other hand, the transition from a gas to an ionized gas, i.e., plasma , is not a phase transition, since it occurs gradually with increasing temperature. ...

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• LLBL [Oulu]
• Plasma sheet and PSBL [Oulu]
• Boundary layer [Oulu]

This colorful display shows tiny differences (or "anisotropies") in the Cosmic Microwave Background (CMB) over the entire sky. The average temperature is just 2.73 kelvins (2.73 degrees Celsius above absolute zero), and the temperature differences span mere millionths of a degree. ... Until now, part of the Milky Way's motion inferred from the variation in the CMB was unexplained. Astronomers have discovered that the Milky Way and neighboring galaxies are being pushed from the Local Void. ...

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• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B13DC91B0-7BE4-41EA-94A9-DE72A041CFE2%7D
• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B7C6622B9-66AA-480C-807E-540F67691D54%7D
• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B3E0CFFB6-07D2-428F-BDC0-4837CEF5A043%7D

... August 29, 1998 . Orion Star Colours . ... Explanation: What determines a star's colour? ... Red stars are cool, around 3,000 kelvins (K), while blue stars are hotter and can have temperatures over 30,000 K. Our own lovely yellow Sun's temperature is a comforting 6,000 K. Differences in star colours are dramatically illustrated in the above photo of the constellation Orion , made using a "star trail step-focus" technique . ... About APOD > . ...

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• APOD: 2013 March 25 - Planck Maps the Microwave Background
• APOD: November 4, 1996 - The Martian Spring
• APOD: 2002 December 24 - Spring Dust Storms at the North Pole of Mars

Microsymposium 34, MS058, 2001 ANOMALIES OF THE MOON'S THERMAL EMISSION IN THE IR SPECTRAL RANGE (10.5 - 12.5 micron). ... Sternberg State Astronomical Institute, Moscow, 119899, Russia, pugach@sai.msu.ru Summary: New satellite measurements of the lunar-surface radiation temperature were used to construct the spatial angular function of thermal radiation of the Moon in the infrared (10.5-12.5 micron) spectral range. ... These thermal anomalies are observed only in the limited range of phase angles. ...

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• http://selena.sai.msu.ru/Pug/Publications/ms38/ms080.pdf
• http://selena.sai.msu.ru/Symposium/RadioMoonE.doc
• http://selena.sai.msu.ru/Symposium/RadioMoonE.pdf

. ASME Paper 95-GT-437. Jacques Lewalle, jlewalle@syr.edu

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• Boundary layer transition
• Additional problems at the transition

... Table shows a table of association rules that has been created to associate bias exposures with scientific frames. ... ABS(:MJD_LOC-REFVAL(:MJD_LOC)) is the absolute difference between the time of the scientific frame that is being studied and the time of a dark exposure . ... The graphs of Figure illustrate the association of two dark exposures with each of two scientific images from our observing run: susi0006.bdf and susi0009.bdf. ... Table: Rules for the association of DARK exposures (cf. ...

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• Zeiss-1000 TCS state
• BTA Control Info

lsst.tcc љ 1.2.2-3-g89ecb63 . ... Classes . Files . ClassљList . ... Weath . ... tcc::Weath Class Reference . include < weath.h > . ... computeRefCo (double &refCoA, double &refCoB, double wavelen, double elev, double lat) const . ... Definition at line 9 of file weath.h . ... double tcc::Weath::airTemp . ... double tcc::Weath::humid . ... double tcc::Weath::press . ... double tcc::Weath::primBackFrontTemp . ... double tcc::Weath::primFrontTemp . ... double tcc::Weath::secBackFrontTemp . ...

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• ARC 3.5m | Closure Conditions
• Figure 7
• Temperature Measurement System For A 3.5-Meter Borosilicate mirror

The primary purpose of KM-7 is to measure the temperature of cold electrons Te in Plasmasphere. ... The spacecraft potential can be evaluated from these measurements. ... MLT . ... Fig.1 . KM-7 measurements in MRK mode during the whole orbit 124 , 27.IX.96. ... Preliminary results . In period considered SC passed the plasmasphere at low and middle latitudes near L < 4 at heights = 8000-10000 km. At L > 4-5 and heights > 8000-10000 km SC was in auroral zone. ...

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• КОНКУРС НАУЧНЫХ РАБОТ ИКИ РАН 2008-2009 гг

Variations of total ozone content and lower ozone stratosphere temperature in Antarctic Region during winter-spring period A.V. Grytsai National Taras Shevchenko University of Kyiv Astronomy and Space Physics Department assen@univ.kiev.ua Data, used in the work work Total ozone: Total Ozone Mapping Spectrometer (TOMS) measurements during 1979 - 2005 and Ozone Monitoring Instrument (OMI) ones for 2006, for http://toms.gsfc.nasa.gov/ftpdata.html. ... A long-term TOC decrease is significant. ...

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• UPS 116/115 temperature

Next: Infrared Data Up: Contents Previous: Optical Photometry . ... For example, one method is to derive the spectral energy distribution (SED) for a target star and compare it to the SED of a dereddened standard star. ... Temperature can be determine via the B - V color (Gilliland 1985): . ... The results produced small extinctions to the background stars of between A and A . ... The most accurate extinction calculation requires both IR and spectral data. Infrared Data . Spectroscopic Data . ...

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• Differences Between Funtools and IRAF Regions
• Through Thick and Thin - Links
• Differences Between QPOE Files and Image Arrays