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http://www.issp.ac.ru/lhpp/PapersMeletov/paper57.pdf.
http://www.issp.ac.ru/lhpp/PapersMeletov/paper57.pdf.
1. LHPP ISSP RAS
... High-pressures experiments are mostly aimed at studying phase transformations in solids, synthesising new phases and studying their composition, crystal and magnetic structure, physical and thermodynamical properties. ... The specific feature of investigations at LHPP that distinguishes it from most other high-pressure laboratories is combining in situ measurements with studies at ambient pressure of new high-pressure phases fixed by quenching to liquid nitrogen temperature. ...
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Ссылки http://www.issp.ac.ru/lhpp/indexen.html -- 9.7 Кб -- 03.04.2014
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2. http://www.atnf.csiro.au/whats_on/workshops/synthesis2003/talks/mmatca.pdf
... 2000 Orion SiO 86.243 GHz Recent Results at 3 and 12 mm Wright, Jorgensen, van Dishoeck, Wong , 2002 ) Pre-planetary disks around young stars (Minier, Lineweaver, Burton, Purcell, Longmore, Norris, 2003) (Wilner, Bourke, Planetary water masers in extra-solar systems Search for biomolecules in Sgr B2 Burton, Wong , Purcell, Hill, Longmore, Barnes, 2002 2003) (Jones, Hunt, 2002 ) (Minier, Massive star ... Massive star formation in the LMC HCO+/HCN in N113 Chin et al. ...
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Ссылки http://www.atnf.csiro.au/whats_on/workshops/synthesis2003/talks/mmatca.pdf -- 945.4 Кб -- 22.05.2003
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3. Phil's public html listings
... page modification history gain curves sefd curves system performance (all receivers) cal values focus curves system temperature multi frequency measurements temperature: platform,bowl,turret room, gain dependence stokes calibration miscellaneous . ... Alfa multi beam . ... sband wide (1.7-3 Ghz) . ... cband (4-6 Ghz) . ... System Temperatures all rcvrs . ... galfacts caldeflection (alfa gain stability) . ... Ao compute server list . ... System gain stability vs rotary floor room temperature (cband) ...
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4. Karazin University
... Schools . ... Dean?s Office . Departments . ... Aquatic Ecology Laboratory . ... School of History . ... Ancient and Medieval History Department . ... History ofљEastern Europe Department . Modern and Contemporary History Department . Ukrainian History Department . ... University History Museum . ... School of Physics . ... The Problem Research Laboratory of Low Temperature Physics was established in 1966 by decisive of Ukrainian Government in V.N. Karazin Kharkov National University. ...
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Ссылки http://www.univer.kharkov.ua/en/departments/physics/laboratory/problem-solving_laboratory_for_low-temperature_physics -- 40.9 Кб -- 09.04.2016
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5. http://www.cplire.ru/html/oxide233/publication06/gao06phc.pdf
Physica C 1 PHYSICA C C ELSEVIER CONDUCTIVITY and Antiferromagnetism of CaCuO2 Thin Films Doped by Sr Gennady A. Ovsyannikova,b*, Viktor V. Demidovb, Yuli V. Kislinskib, Philippe V. Komissinskia,b, Dag Winklera a Chalmers ... revised date here; accepted date here Abstract The results of electrical and magnetic investigations of epitaxial CaxSr1-xCuO2 ( CSCO ) thin films grown by pulsed laser deposition are presented ... Temperature dependence EPR amplitude for two CSCO films with =0.15 ...
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Ссылки http://www.cplire.ru/html/oxide233/publication06/gao06phc.pdf -- 226.2 Кб -- 31.01.2007
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6. http://zebu.uoregon.edu/1998/ph101/l17.html
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Ссылки http://zebu.uoregon.edu/1998/ph101/l17.html -- 4.8 Кб -- 01.12.1998
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7. Incoherent scatter [Oulu]
... The basic principles of incoherent scatter: . ... Because of the electron movement, spectrum of the observed signal is broad and it has shape which depends, e.g., on the temperature. ... ion temperature . ... According to the theory, Ti should be replaced by (2Ti,perp + Ti,par)/3 (Williams and Jain,1986; Glatthor and Hernandez, 1990; Winser et al., 1990). ... Glatthor, N., and R. Hernandez, Temperature anisotropy of drifting ions in the auroral F-region, observed by EISCAT, J. atmos. terr. ...
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Ссылки http://www.iki.rssi.ru/magbase/REFMAN/SPPHTEXT/incoherent.html -- 4.9 Кб -- 21.12.2007
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8. Temperature and humidity data
Next: Pressure Up: Additional information Previous: Additional information . ... Although the ESO Archive standard is to record temperatures in kelvins, this is often inconvenient. ... Therefore, if the temperatures are not in kelvins, the appropriate units should be provided in the table file (if temperatures are in a column), or as a comment. ... If filter and detector temperatures are otherwise regulated or recorded, it may still be useful to record DOMETEMP in the data file as a Real*4 column. ...
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Ссылки http://www.sao.ru/precise/Midas_doc/doc/94NOV/vol2/node642.html -- 5.6 Кб -- 23.02.1996
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9. Mars2
MAtrix Radiometric System project MARS. ... Three-module experimental radiometric matrix was designed and put in operation successfully. Flowchart of the one channel is shown in Figure 1. ... Figure 1. ... In figure 2 the receiver module and switch assembly is shown. ... The elementary radiometers are combined ( figure 3 ) into the microwave unit ( one pair of horns shown is out of use ), where they integrated to use unified systems for calibration, power supply and temperature control. ...
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Ссылки http://mavr.sao.ru/hq/lrk/gifs/mars2en.html -- 4.9 Кб -- 09.04.2016
[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/lrk/gifs/mars2en.html -- 4.9 Кб -- 10.04.2016
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/lrk/gifs/mars2en.html -- 4.9 Кб -- 09.04.2016
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[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/lrk/gifs/mars2en.html -- 4.9 Кб -- 09.04.2016
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10. Soyuz panel: Pressure and temperature indicator
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Ссылки http://www.vsm.host.ru/soyuzpan/pti.htm -- 1.2 Кб -- 24.05.1999
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11. http://www.mso.anu.edu.au/~wood/lectures/2007/assignment_1.pdf
... A molecular cloud in the interstellar medium may be considered as spherical and of uniform density and fixed temperature as it undergoes expansion or contraction. Assume the opacity of material in the molecular cloud has a value . ... How will this affect cloud fragmentation? (e) In the stages of collapse of a gas cloud before it becomes optically thick, its temperature is determined by the balance between compressional heating and radiation of energy from the cloud. ...
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Ссылки http://www.mso.anu.edu.au/~wood/lectures/2007/assignment_1.pdf -- 41.2 Кб -- 08.03.2007
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12. Theoretical Astrophysics
Subject, Problems and Objects of Theoretical Astrophysics. ... Stellar Photospheres, Their Features. ... Physics of Continuous Radiation Absorption in Stellar Photospheres. ... Continuous Radiation Absorption in Stellar Photospheres of Various Spectral Classes. Solar Type Photospheres. ... Characterisics of Absorption Lines. ... Interstellar Absorption Lines, Their Features. ... Physical and Dynamic Features of Interstellar Medium, Which Follows from Observations of Interstellar Absorption Lines. ...
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Ссылки http://space.univ.kiev.ua/courses/teor_astroph_e.html -- 8.7 Кб -- 23.02.2005
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13. Molecular hydrogen emission in the interstellar medium of the Large Magellanic
We present the detection and analysis of molecular hydrogen emission towards ten interstellar regions in the Large Magellanic Cloud. We examined low-resolution infrared spectral maps of 12 regions obtained with the Spitzer infrared spectrograph (IRS). ... The excitation diagrams of the detected H2 transitions are used to determine the warm H2 gas column density and temperature. ... We find the excitation of H2 by this process is equally efficient in both atomic- and molecular-dominated regions. ...
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Ссылки http://www.stsci.edu/~kgordon/papers/2015MNRAS.446.2490N.html -- 4.8 Кб -- 21.01.2016
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14. http://www.mrao.cam.ac.uk/~kjbg1/lectures/lect1_1.pdf
... Luminosity (L) · · · · A source's luminosity is the power that it emits in radiation. ... NB Astronomers often say `flux' when they mean `flux density' · SI units are Wm-2Hz -1 -26 filter · Also used are Jy 10 Wm-2Hz -1 E= РРРF d dA dt Specific Intensity, Surface Brightness (I) · Specific intensity (or surface brightness) is the power received (or emitted) per unit area per unit frequency per unit solid angle. ч F at surface of a spherical source = I · · Specific intensity is independent of distance...
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Ссылки http://www.mrao.cam.ac.uk/~kjbg1/lectures/lect1_1.pdf -- 117.5 Кб -- 07.10.2002
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15. Vertical Structure of the Secondary: Hydrostatic Model
... In this section, we develop a physical model of the secondary as a disk that is centrifugally supported in the radial direction and hydrostatically supported in the vertical direction. We assume that the disk is vertically isothermal and well mixed. ... where is the mean molecular mass of the gas, is the orbital period at the outer edge of the disk in years, and all of the mass of the secondary has been assumed to be concentrated near its center, so the Keplerian approximation is valid. ...
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Ссылки http://hea-www.harvard.edu/~swolk/thesis/node89.html -- 10.7 Кб -- 01.10.2012
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16. Winer Observatory Engineering Weather Page
Winer Observatory P.O. Box 797, Sonoita, Arizona 85637-0797, USA . ... Irvin M. Winer . ... Weather . ... Temperature ( F) . ... 0.00 . ... AAG IR Sky Temperature ( C) . ... AAG Adjusted IR Sky Temperature ( C) . ... AAG Ambient Temperature ( C) . ... AAG Temperature Split ( C) . ... 39321 D,01/23,01:10:10, 67, 20,25.43,270, 8, 38, 0.00, 6.18, 63,!251 at 2016.04.09 19:45:25 . ... S-cmd: "(null)" at 2016.04.09 19:45:25 . ... Page last updated on: February 16, 2016 . ... 2013 Winer Observatory. ...
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Ссылки http://www.winer.org/Site/engWeather.php -- 18.9 Кб -- 09.04.2016
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17. http://selena.sai.msu.ru/Symposium/RadioMoonE.doc
TEMPERATURE OF REGOLITH IN COLD TRAPS ON THE MOON A.A. Berezhnoi Sternberg Astronomical Institute Moscow, Russia The hypothesis of the existence of the lunar ice in cold traps was stated in (Watson et al., ... Arnold, 1979) estimated the mean temperature on the surface of lunar cold traps as 40-90 K. We plotted the dependence of regolith mean temperature on depth for these two values of mean temperature on the surface (see figure 1). ... Arnold J.R. Ice in the lunar polar regions, J. Geophys. ...
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Ссылки http://selena.sai.msu.ru/Symposium/RadioMoonE.doc -- 98.0 Кб -- 06.10.2008
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18. Data gathering
... Measurements of fluctuations of the streamwise and vertical components of wind velocity were performed by two-component sonic anemometer of continuous radiation with capacitor microphones. Measurements of temperature fluctuations were performed with the aid of resistance thermometer. ... Average wind velocity at the 5 meters height was about 5 m/s. With the aid of multichannel registrator the simultaneous recordings of pulsations of temperature and velocity components were made. ...
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Ссылки http://www.sai.msu.su/~er/mf2.html -- 3.1 Кб -- 01.10.2012
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19. Effective temperatures
. Next: Diameters Up: Stellar parameters from calibrations Previous: Gravities Contents . Temperatures of stars are derived from their spectral type and luminosity class. Calibrations are stored in files spec_par.V, spec_par.IV, spec_par.III, spec_par.II, spec_par.I in oyster/starbase . teff_stars Compute effective temperature for all stars in startable. teff_star ( spectrum _char ) Function. Return effective temperature for star with specified spectrum. Christian Hummel 2015-04-28
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Ссылки http://www.eso.org/~chummel/oyster/manual/node116.html -- 3.5 Кб -- 28.04.2015
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20. Mechanics and Cryogenics
The drawing presented in Figure 6 suggests a cryo-mechanical design based on a cylindrical vacuum shell, with total size dictated by total length of the optical system and wheels diameter. ... internal support structure for cold optics and detector; . cold optics, focal masks and filter wheels; . ... The detector, in thermal contact with the cold plate, will have an active temperature control, with an RDT sensor and a heater, both connected to an independent temperature controller. ...
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Ссылки http://www.arcetri.astro.it/irlab/instr/nics/generale/meccani.html -- 6.1 Кб -- 28.07.2005
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